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The Journal of Neurophysiology Vol. 83 No. 2 February 2000, pp. 808-827
Copyright ©2000 by the American Physiological Society
1Department of Neurobiology, University of California at Los Angeles, Los Angeles, California 90095; 2Laboratory of Neuropsychology, National Institute of Mental Health, National Institutes of Health; and 3Laboratory of Developmental Neurobiology, National Institute of Child Health and Human Development, National Institutes of Health, Bethesda, Maryland 20892
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ABSTRACT |
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Latham, P. E., B. J. Richmond, P. G. Nelson, and S. Nirenberg. Intrinsic Dynamics in Neuronal Networks. I. Theory. J. Neurophysiol. 83: 808-827, 2000. Many networks in the mammalian nervous system remain active in the absence of stimuli. This activity falls into two main patterns: steady firing at low rates and rhythmic bursting. How are these firing patterns generated? Specifically, how do dynamic interactions between excitatory and inhibitory neurons produce these firing patterns, and how do networks switch from one firing pattern to the other? We investigated these questions theoretically by examining the intrinsic dynamics of large networks of neurons. Using both a semianalytic model based on mean firing rate dynamics and simulations with large neuronal networks, we found that the dynamics, and thus the firing patterns, are controlled largely by one parameter, the fraction of endogenously active cells. When no endogenously active cells are present, networks are either silent or fire at a high rate; as the number of endogenously active cells increases, there is a transition to bursting; and, with a further increase, there is a second transition to steady firing at a low rate. A secondary role is played by network connectivity, which determines whether activity occurs at a constant mean firing rate or oscillates around that mean. These conclusions require only conventional assumptions: excitatory input to a neuron increases its firing rate, inhibitory input decreases it, and neurons exhibit spike-frequency adaptation. These conclusions also lead to two experimentally testable predictions: 1) isolated networks that fire at low rates must contain endogenously active cells and 2) a reduction in the fraction of endogenously active cells in such networks must lead to bursting.
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INTRODUCTION |
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In the absence of stimuli, neurons in many areas of the
mammalian CNS remain active. This activity falls into two
main patterns: low, steady firing in the 1- to 5-Hz range and rhythmic
bursting. The former has been widely observed in sensory cortex, motor
cortex, and spinal cord and has been seen in both awake-behaving and
anesthetized animals (Collins 1987
; Gilbert
1977
; Herrero and Headley 1997
; Lamour et
al. 1985
; Leventhal and Hirsch 1978
;
Mednikova and Kopytova 1994
; Ochi and Eggermont
1997
; Salimi et al. 1994
; Szente et al. 1988
; Zurita et al. 1994
); the latter is
fundamental to central pattern generators, which generate rhythmic
behavior such as respiration, locomotion, and chewing (for reviews see
Marder and Calabrese 1996
; Rekling and Feldman
1998
). Both patterns may occur in the same neural tissue, with
neuromodulators inducing a reversible switch between steady firing and
bursting (Berkinblit et al. 1978
; Kudo and Yamada
1987
; Zoungrana et al. 1997
).
From a theoretical point of view, it has been relatively easy to
understand how large neuronal networks might generate rhythmic bursting
(Feldman and Cleland 1982
; Perkel and Mulloney
1974
; Rekling and Feldman 1998
; Rybak et
al. 1997
; Smith 1997
) but difficult to
understand how such networks might generate steady, low firing rates
(Abeles 1991
). Several investigators have explored the
latter problem theoretically (Amit and Treves 1989
;
Buhmann 1989
; Treves and Amit 1989
).
Their approach was to use simulated networks and attempt to generate
low firing rates through dynamic interactions between excitatory and
inhibitory neurons. The networks they used were (1) highly
interconnected, (2) isolated from any external sources of
input, and (3) comprised of neurons whose resting membrane potentials were far enough below threshold that several
near-synchronous excitatory postsynaptic potentials (EPSPs) were
necessary to trigger an action potential. Networks with these seemingly
standard properties were unable to produce maintained low firing rates;
the lowest numerically generated mean rates were ~20 Hz,
significantly larger than the background firing rates observed in
biological networks.
These experimental and numerical findings raise three main questions. First, why were networks with the above "standard" properties unable to fire at low rates? Did the numerical studies simply miss a parameter regime that would have generated low firing rates, or were the properties actually too restrictive? Second, what are the conditions that allow networks to fire robustly at low rates? And third, what is the relation between steadily firing networks and rhythmically bursting ones? In particular, is there a single parameter, or a small set of parameters, that allow networks to switch naturally from one state to the other?
To answer these questions, we developed a model that allowed us to explore analytically the intrinsic dynamics of large, isolated networks in the low firing rate regime. Our main assumptions were conventional: excitatory input to a neuron increases its firing rate, inhibitory input decreases it, and neurons exhibit spike-frequency adaptation (their firing rates decrease during repetitive firing). We found theoretically, and verified using large, simulated networks of spiking neurons, that a single parameter plays a dominant role in controlling intrinsic firing patterns. That parameter is the fraction of endogenously active cells; i.e., the fraction of cells that fire without input. Our primary result is that there is a sharp distinction between networks in which the fraction of endogenously active cells is zero and those in which it is greater than zero. When the fraction is zero, a stable, low firing rate equilibrium cannot exist; networks are either silent or fire at high rates. Only when the fraction is greater than zero are low average firing rates possible. In this regime there is a further subdivision into networks that burst and those that fire steadily, the former having fractions below a threshold and the latter having fractions above threshold. Connectivity also plays a role in shaping firing patterns, but to a lesser degree; it determines whether activity occurs at a constant mean firing rate or oscillates around that mean.
These theoretical results imply that an isolated network that fires at
low rates must contain endogenously active cells. We tested this
strong, parameter-free prediction experimentally in cultured neuronal
networks and consistently found a large fraction of endogenously active
cells, ~30% on average, in networks that displayed low firing rates.
We also investigated experimentally the transition between steady
firing and bursting as the fraction of endogenously active cells
changed, and we found that networks that fired steadily could be
induced to burst by reducing the fraction of endogenously active cells.
Both of these experimental results are presented in the following paper
(Latham et al. 2000
).
The above analysis applies to networks that receive external input as well as to isolated ones. This is because cells that receive sufficient external input to make them fire are effectively endogenously active, in the sense that they can fire without receiving input from other neurons within the network. These pseudoendogenously active cells control firing patterns in the same way that truly endogenously active ones control firing patterns in isolated networks. In particular, for networks receiving external input, firing patterns follow the same set of transitions as discussed above: as activity produced by external input increases there is a transition first from silence to bursting, and then from bursting to steady firing.
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METHODS |
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In RESULTS we make a series of predictions about the behavior of large neuronal networks, then test those predictions by performing large-scale network simulations. In this section we describe the single neuron equations and synaptic coupling used in the simulations, discuss our choice of simulation parameters, and provide a particular realization of a reduced network model that is used to illustrate the general principles derived in RESULTS.
Network simulations
Our predictions about the behavior of large neuronal networks are based on a simplified firing rate model. To verify these predictions, we perform large-scale simulations with synaptically coupled model neurons. Following are the single neuron equations used in the simulations, the prescription for choosing single neuron parameters and synaptic coupling, and a complete list of network parameters.
SINGLE NEURON EQUATIONS.
Our simulated network consists of N synaptically coupled
neurons, NE of which are excitatory and
NI of which are inhibitory. The time evolution
equation for the membrane potential of neuron i,
Vi, may be written
|
(1) |
|
(2) |
V
Vt
Vr is the nominal gap between resting
(Vr) and threshold (Vt)
voltages and Rcell is the membrane resistance of
the cell (Fig. 1). Typically,
Vr =
65 mV and Vt =
50 mV, producing a nominal gap of 15 mV. In the absence of synaptic
drive and afterhyperpolarization currents, Eq. 1 with
Ispike,i given by Eq. 2 is
identical to the
-neuron model introduced by Ermentrout and
Kopell (1986)
-neuron
rather than a conductance-based model is that relatively large time
steps can be used, on the order of 1 ms rather than the 0.1- to 0.2-ms
time steps required to accurately represent the rapidly varying
membrane potential during a true action potential.
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-neuron model [which is
related to our model by the change of variables
Vi ~ tan (
/2) + constant] an action
potential would occur whenever Vi reaches +
(the spike apex), at which point the voltage would be reset to 
(the spike repolarization). For numerical work, however, it is
necessary to use finite spike apex and repolarization voltages. The
apex we use in our simulations, denoted Vapex,
is 20 mV, and the reset value, Vrepol, is
80 mV.
The fast and slow afterhyperpolarization currents may be written
|
(3a) |
|
(3b) |
K is the potassium reversal
potential and gK,i and
gK
Ca,i are potassium
conductances. The latter quantities obey the time evolution equations
|
(4a) |
|
(4b) |
and
gK
Ca,
are the equilibrium value
of the fast and slow potassium conductances,
K
Ca and
K
Ca are their time constants,
tiµ is time of the µth spike on neuron
i, and the
-function,
(t
tiµ), provides an impulse whenever
t = tiµ. Those impulses
causes discrete increases,
gK and
gK
Ca, in
gK,i and
gK
Ca,i, respectively.
For simplicity we assume that the equilibrium conductances, gK,
and
gK
Ca,
, and the time constants,
K
Ca and
K
Ca are independent of voltage.
Then, without loss of generality, we may assume that
gK,i and
gK
Ca,i are zero at rest,
which implies that gK,
= gK
Ca,
= 0.
Combining Eqs. 1-4, the network evolution equations become
|
(5a) |
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(5b) |
|
(5c) |
cell
RcellCcell is the cell
time constant and quantities with a hat have been multiplied by
Rcell:
Îa,i
RcellIa,i,
etc. Note that both Îa,i and
Îsyn,i have units of voltage,
whereas the conductances,
K and
K
Ca, and their increments, 
K and

K
Ca, are dimensionless.
The normalized synaptic current, Îsyn, is
written
|
(6) |
j is the reversal potential
associated with the ligand-gated receptor on the cell that is
postsynaptic to neuron j. The weight matrix, Wij, is always nonnegative. This ensures that
excitatory drive (activity from neurons with
j greater than the threshold for the emission
of an action potential) increases the probability that a postsynaptic
neuron fires, whereas inhibitory drive (activity from neurons with
j less than threshold) decreases the probability.
The conductance change on a postsynaptic neuron is mediated by the
fraction of open channels, sij. That fraction
increases instantaneously when a spike occurs at neuron j
and decays exponentially between spikes: for all i
|
(7) |
|
(8) |
|
(9a) |
|
(9b) |
i and 
,i evolve according to
|
(10a) |
|
(10b) |
i and

,i, Eq. 10, can
be used to determine the synaptic current, and
sij drops out of the equations.
DISTRIBUTION OF APPLIED CURRENTS.
The applied current, Îa,i,
determines how close a neuron is to the threshold for generating an
action potential, or, if it is above threshold, its endogenous firing
rate. This quantity is chosen probabilistically:
Îa,i has a boxcar distribution,
uniform between 0 and Îmax and 0 outside those two values. We use this distribution because it gives us precise
control over the number of neurons that are endogenously active. The
precise control arises because neuron i is endogenously active if and only if Îa,i >
V/4
Îthresh. Consequently, when Îmax < Îthresh no neurons are endogenously active, and when Îmax > Îthresh the fraction of endogenously active cells is (Îmax
Îthresh)/Îmax.
NETWORK CONNECTIVITY. Connectivity is specified by the weight matrix, Wij. This quantity determines both whether two neurons are connected and, if they are, the strength of that connection. Like the applied current, the weight matrix is chosen probabilistically, and the probability that neuron j connects to neuron i is denoted Pij. If there is a connection, the strength of that connection is set by considerations of EPSP and inhibitory postsynaptic potential (IPSP) sizes. If there is no connection, Wij is set to zero.
We use two models of connectivity, infinite range and local, when constructing Pij. For infinite range connectivity, Pij depends only on the types of neurons i and j
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(11a) |
|
(11b) |
|
(12a) |
|
(12b) |
), where r is radius and
is azimuthal angle. Neurons are randomly assigned a position according
to the probability distribution P(r,
) where
P(r,
)rdrd
is the probability
that a neuron falls within the area bounded by [r,
r + dr] and [
,
+ d
]. For
P(r,
) we use the azimuthally symmetric
function
|
(13) |
r is the width of the transition
region between approximately constant density and near zero density;
i.e., the distribution P(r,
) is approximately
flat for radius r < 1
r and drops rapidly to nearly zero in a
transition region of width 2
r.
Using the probability distribution given in Eq. 13 to assign
a position, xi
(ri cos
i,
ri sin
i), to every
neuron i, the distance between two neurons is then given simply by the Euclidean norm, dij
|xi
xj|. We use a Gaussian profile for local
connectivity, for which the probability of making a connection is
modulated by the factor exp(
dij2/2
Tj2)
where
Tj is a parameter that determines
the axonal spread of neurons of type j. Thus
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. In
our calculations we use an approximate expression for the normalization, valid in the limit that
r
1 [so that P(r,
) = 1/
when
r
1 and zero when r > 1]. In this
limit
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PTiTj
, which
can always be satisfied by taking the limit
Tj
(in this limit
ZTj
1). We impose the condition ZTj
PTiTj
in all
our simulations.
We consolidate the infinite range and local connectivity models by
using the local connectivity description and setting
Tj =
whenever we want to recapture
the infinite range case.
The strength of a connection, once one is made, is determined by the
size of Wij. To ensure that
Wij is in a biophysically reasonable range, we
need a relation between it and the sizes of both excitatory and
inhibitory PSPs. To derive such a relation, we use Eq. 5a to
compute, as a function of Wij, the peak voltage in response to a single presynaptic action potential. For definiteness we consider a neuron whose resting membrane potential is the nominal one, Vr (which implies that
Îa = 0), and assume that the neuron has
not produced an action potential for a sufficiently long time that both
K and
K
Ca have decayed to zero.
Under these conditions, Eq. 5a for the membrane potential can be combined with Eq. 6 for the synaptic current to yield
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Vi
Vi
Vr, linearizing the
resulting equation, and assuming the synaptic drive is small, we find
that
Vi evolves according to
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0) = rs
exp(
t/
s) (recall that
s is the decay time of the open channels and
rs is the use parameters; see Eq. 7).
Combining this time dependence for sij with the
initial condition
Vi (t = 0) = 0, the above equation has the solution
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Vi(t)| is maximum when
t = ln
(
cell/
s)/(
s
1
cell
1)
t0.
Defining VPSPij
Vi(t0), it is
straightforward to show that
|
(14) |
PARAMETERS. Table 1 contains a list of all parameters used in our simulations. Parameters followed by an asterisk are the ones we vary; for those, a range or set of values is given. Parameters not followed by an asterisk remain constant throughout the simulations. The grouping into single-cell, synaptic, and network parameters is in most cases clear; the exceptions are VEPSP and VIPSP, the nominal amplitudes of the excitatory and inhibitory postsynaptic potentials. These are usually thought of as synaptic or single-cell properties, but in our simulations we use them only to determine the connectivity matrix, Wij, via Eq. 14. Specifically, VPSPij = VEPSP when neuron j is excitatory and VPSPij = VIPSP when neuron j is inhibitory. Thus they are listed under network parameters.
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K and

K
Ca, which are both
dimensionless. To convert these to their correct physical units (Amps
for current and Siemans for conductance) divide by the cell membrane resistance.
Simulations were performed with a fourth-order Runge-Kutta integration
scheme. In all simulations reported we used a time step of 1 ms. We
occasionally checked that this was short enough by decreasing the time
step to 0.5 ms, and in no cases did we see a change in our results.
Choice of simulation parameters
In choosing parameters we attempted to stay close to values
observed in two different systems: networks of cortical neurons, and
networks of cultured mouse spinal cord neurons in which we did
experiments relevant to the theoretical predictions made here (Latham et al. 2000
). These two systems differ primarily
in their connectivity and postsynaptic potential amplitude, the former having high connectivity and small PSPs, the latter low connectivity and large PSPs. Thus most parameters were the same for the two model
networks used in our simulations, and these were relatively standard;
the parameters that differed pertained to connectivity and PSP
amplitude, mirroring the differences between cortical and cultured
spinal cord networks.
As is well-known, connectivity in cortex is high; each neuron connects
to approximately 7,000 others (Braitenberg and Schüz 1991
). The size of a local circuit, assuming such a thing
exists, is more difficult to determine. However, given that axonal
spread is measured in hundreds of micrometers and the density of
neurons is ~105/mm3 (Braitenberg and
Schüz 1991
), a local circuit on the order of 100,000 neurons is a reasonable estimate. Unfortunately, we do not yet have the
computational power to model such large networks. Consequently, we
considered networks of only 10,000 neurons, each of which made ~1,000
connections. To make up for the reduced connectivity in our model
network we increased the size and frequency of the postsynaptic
potentials: instead of using the more realistic numbers of 0.2 mV for
EPSPs (Komatsu et al. 1988
; Matsumura et al.
1996
) and
1 mV for IPSPs (Tamás et al.
1998
), we typically used 1.0 and
1.5 mV. The frequency of
PSPs was increased in our model by ignoring failures, so
neurotransmitter was released every time an action potential occurred.
Unlike cortex and spinal cord in vivo, cultured spinal cord networks
are intrinsically localized. However, connectivity in our particular
preparation has not been characterized. We thus made estimates as
follows. The number of connections a neuron makes is
A
PA, where A is the
area of the axonal arborization,
is the number of neurons per area,
and PA is the probability that a neuron connects
to another neuron within its axonal arborization. We measured axonal
arborization from neurons visualized after intracellular injection with
horseradish peroxidase (Neale et al. 1978
), and found it
to be 2.0 ± 0.86 mm2 (mean ± SD,
n = 12 neurons). The density of our cultures,
, was
23.7 ± 10.2 neurons/mm2 (n = 10 culture dishes). Thus a single neuron is capable of connecting to
~475 others. Finally, in paired recordings (Nelson et al.
1981
), approximately one-half the cell pairs tested were
connected. This gives a connectivity of ~240 connections/neuron. We
used 200 connections/neuron in most of our simulations, although we
explored a range of values.
The size of the postsynaptic potentials is large in cultured spinal
cord neurons; on the order of 3-10 mV for EPSPs and approximately
6
mV for IPSPs (Nelson et al. 1981
, 1983
). In contrast to cortex, transmission failures
are not observed; this is because a presynaptic neuron makes a large
number of connections (~100) on each of its postsynaptic targets
(Nelson et al. 1983
; Pun et al. 1986
). In our simulations we typically used EPSP and IPSP amplitudes of 4 and
6
mV, respectively, and, for simplicity, we did not include variation.
The parameters given in Tables 1 and 2 were the ones we used in the bulk of our simulations. In APPENDIX A we studied the effects of varying these parameters. In no cases did changing parameters produce network behavior that was inconsistent with our model. This suggests that our model made robust predictions and that our simulation results were not due simply to a particular choice of parameters.
Reduced network model
The reduced network model we use in our analysis is based on the
Wilson and Cowan equations (Wilson and Cowan 1972
), in
which the dynamical variables are the mean excitatory and inhibitory firing rates. Those equations are given in generic form in Eq. 16 of RESULTS. Here we write down a particular
realization of Wilson and Cowan-type equations that we augment by
including spike-frequency adaptation.
Although it would be desirable to start with the equations describing
the full network simulations and derive from those a set of mean firing
rate equations, this is essentially impossible to do analytically
except in highly idealized cases (van Vreeswijk and Sompolinsky
1998
), and extremely difficult numerically. Thus we propose a
set of reduced equations designed to capture qualitative, but not
quantitative, features of large-scale networks. Denoting
E and
I
as the mean excitatory and inhibitory firing rates (averaged over
neurons), and GE and GI
as the mean level of spike-frequency adaptation of the excitatory and
inhibitory populations, we let these variables evolve according to
|
(15a) |
|
(15b) |
|
(15c) |
|
(15d) |
E and
I are the time scales for relaxation to a
firing rate equilibrium,
SFA is the
characteristic time scale for changes in the level of spike-frequency
adaptation, A is the overall amplitude of the gain
functions, the CLM, L, M = E, I, correspond to
connectivity among the excitatory (E) and inhibitory
(I) populations,
G corresponds to the coupling between firing rate and spike-frequency adaptation,
max
controls network excitability, and g(x) is a
thresholding function that saturates at
max, the maximum
firing rate of the neurons,
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Ca in the network simulations,
G is related to

K
Ca, and
max is related to Îmax.
The qualitative features that these equations capture are 1)
the gain functions, g(...), are generally increasing
functions of excitatory firing rate and decreasing functions of
inhibitory firing rate [the CLM are all
positive and g(x) is a nondecreasing function of
x], 2) increasing the firing rate increases
spike-frequency adaptation (
G is positive), 3)
increasing the level of spike-frequency adaptation reduces firing
rates, 4) the gain functions are approximately threshold-linear, consistent with the numerical gain functions in Fig.
1A, and 5) the gain is reduced by a divisive
term proportional to the inhibitory firing rate. The divisive term,
which has been proposed as a mechanism for gain control in cortical
neurons (Carandini and Heeger 1994
; Carandini et
al. 1997
; Heeger 1992
; Nelson
1994
), was included for two reasons. First, it was observed in
our simulations: Fig. 1A in APPENDIX B shows a
pronounced drop in gain as the inhibitory firing rate increases.
Second, curved nullclines are essential for the existence of the
saddle-node bifurcation that produces bursting (Fig. 5), and the
divisive term increases nullcline curvature, thus making bursting more robust.
We are interested in understanding the dynamics represented by
Eq. 15 in the regime in which
E
and
I are on the order of the membrane time
constant, ~10 ms, and
SFA is on the order
of the spike-frequency adaptation time, which can be as high as several
seconds. Thus
E,
I
SFA, and
we can use the fast/slow dissection proposed by Rinzel
(1987)
to analyze the dynamics. With this approach, the full
four-dimensional system is reduced to two subsystems: a fast one
corresponding to the population firing rates,
E and
I, and a slow one corresponding to the
level of spike-frequency adaptation, GE and
GI. Although this represents a major
simplification, it still leaves us with three main behaviors: steady
firing, oscillations, and bursting. The first two can be readily
understood in terms of the two-dimensional firing rate dynamics with
GE and GI held fixed;
only the third, bursting, requires the interaction of all four
variables. We thus briefly discuss a method for its analysis.
The idea behind the fast/slow dissection is that
E and
I
relax rapidly to an attractor (either a steady state or oscillations)
compared with the time scale over which GE and
GI change. Motion in the
GE
GI plane is
then determined be Eqs. 15c and 15d with
E and
I
evaluated on their attractor. In the purely bursting regime, for
attainable levels of spike-frequency adaptation the network is either
silent or fires steadily; the attractor is a fixed point for given
values of GE and GI. In
this steady-state regime, the mean inhibitory firing rate,
I, is a single-valued function of the mean excitatory rate,
E (see Fig.
3B). The dynamics associated with Eq. 15 can thus
be reduced to three dimensions, and the important features of the
dynamics are captured by a three-dimensional bifurcation diagram that
consists of a sheet whose height above the GE
GI plane represents the value of
E. Bifurcations (sudden changes in
firing rate) occur at folds in the sheet.
For a particular set of parameters, the trajectory in the
GE
GI plane is
typically a closed curve that exhibits sudden changes of direction at
bifurcation points. If the trajectory collapses onto, or almost onto, a
single curve, we may make a further, approximate, reduction to a
two-dimensional bifurcation diagram of
E versus GE. For
the parameters considered in RESULTS (Fig. 6), the curve in
the GE
GI plane
collapsed almost to a line, resulting in the two-dimensional
bifurcation diagrams shown in Fig. 6, C-E. For each of
these diagrams the lines were found numerically using least-squares
regression. The equations for the lines were as follows: Fig.
6C (
max = 0), GI = 0.00 + 0.64GE,
R2 = 1.0000; Fig. 6D
(
max = 0.25), GI = 0.01 + 0.65GE, R2 = 0.9996; Fig. 6E (
max = 0.52),
GI = 0.03 + 0.65GE,
R2 = 0.9999.
| |
RESULTS |
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In this section we investigate how single neuron and network properties affect intrinsic firing patterns. We use as our model system large, isolated networks with random, sparse connectivity and develop a theory that describes the firing patterns in such networks in the low firing rate regime. We then test specific predictions of this theory by performing simulations with large networks of spiking neurons. Robustness of the theory is verified in APPENDIX A, where we examine a broad range of single neuron and network parameters.
Theory
The theoretical development is divided into three parts: 1) analysis of networks that do not exhibit adaptation, 2) analysis of the more realistic, and more biologically relevant, case of networks that do exhibit adaptation, and 3) analysis of the stability of low firing rate equilibria.
LOW FIRING RATE EQUILIBRIA IN SPARSE, RANDOMLY CONNECTED
NETWORKS WITHOUT ADAPTATION.
To describe the dynamics of large, sparse, randomly connected networks,
we start with the model proposed by Wilson and Cowan (1972)
. We use as our dynamical variables the mean excitatory and inhibitory firing rates, denoted
E
and
I, respectively. In terms of these
variables, the Wilson and Cowan model can be cast in the form
|
(16a) |
|
(16b) |
E and
I
are time constants that determine how fast the network relaxes to its
equilibria and
E and
I are the excitatory and inhibitory gain
functions. The gain functions determine the network firing rates at one
instant of time given the firing rates at an earlier time.
Specifically, if the average excitatory and inhibitory firing rates at
time t are
E and
I, then
E and
I are the average excitatory and inhibitory
firing rates at times t +
E
and t +
I, respectively. In
the original Wilson and Cowan equations the gain functions consisted of
two terms, one associated with the neurons' refractory period and one
with the "subpopulation response function" (Wilson and Cowan 1972
E/dt and
d
I/dt to zero, are
|
(17a) |
|
(17b) |
E,
I) plane. These curves are referred to
as the excitatory and inhibitory nullclines, respectively (for a
discussion of nullclines similar to ours, see Rinzel and
Ermentrout 1998
I is large, both gain functions
approach zero as
E approaches zero,
rise rapidly as
E increases past some
critical value, and approach the maximum neuronal firing rate as
E becomes large. Similarly, when
E is large, the gain functions are
sigmoidal versus
I but with negative
slope. At very low firing rates, however, the gain functions become
sensitive to both single neuron and network properties. It is the
single neuron properties, however, that have the largest effect on the
gain functions, because at very low firing rates the gain functions are
determined primarily by the responses of neurons at rest to a very
small number of EPSPs. This led us to divide networks into three
regimes based on single neuron response properties. Each regime
produces qualitatively different gain functions and thus, as we will
show, qualitatively different nullclines. Those regimes are as follows:
| 1 | None of the cells have their resting membrane potential within one EPSP of threshold for the generation of an action potential; i.e., no cell fires in response to a single EPSP, which in turn implies that no cells are endogenously active. |
| 2 | Some cells have their resting potential within one EPSP of threshold, but none are endogenously active. |
| 3 | Some cells are endogenously active. |
E(
E, 0)
versus
E for these three regimes. We
chose
I = 0 in this plot because it
accentuates the differences among the gain function. The three regimes
are distinguished by the value and the slope of the gain function at
the origin of the (
E,
I) plane. In regime 1 the
cells are far enough from threshold that a single action potential
cannot cause any neurons to fire, so the gain function and its slope
are both zero at the origin. In regime 2, as in regime
1, the neurons cannot fire without input, so
E(0, 0) is again zero. However, a single
action potential can cause cells to fire and thus ignite network
activity; consequently the origin is unstable and the slope there is
greater than one. In regime 3 a fraction of the neurons fire
without input, so
E(0, 0) > 0.
|
I(0,
I) versus
I, again for the three regimes listed
above. The behavior here is somewhat simpler: in regimes 1 and 2,
I(0,
I) = 0 for all values of
I, whereas in regime 3,
I(0,
I) is
greater than zero when
I = 0 and
decreases monotonically with increasing
I.
Armed with the shapes of the gain functions in the three regimes, we
are now in a position to construct the nullclines. That construction is
done graphically: starting with the excitatory nullcline, we plot the
function
E(
E,
I) versus
E for various values of
I and look for intersections with the
line
E =
E. This is shown in Fig.
3A for regime 1 (no
cells within one EPSP of threshold). Each of the intersections,
including the one at the origin, is a solution to Eq. 17a
and thus corresponds to a point on the excitatory nullcline. Dashed
lines connect the intersections to the excitatory nullcline, which is
drawn in gray in the two dimensional
(
E,
I)
plane directly below the gain curves (Fig. 3C). Note that
the gain curves in Fig. 3A that correspond to low values of
the inhibitory firing rate have three intersections with the line
E =
E. In
addition, all gain curves intersect at the origin, which implies that
the
I axis is part of the excitatory
nullcline. For a similar construction in an all-excitatory network, see
O'Donovan et al. (1998)
|
I axis). Between those two extremes is
a threshold. That threshold, which lies on the region of the nullcline
with positive slope, represents an unstable equilibrium at fixed
inhibitory drive. These differences in stability naturally divide the
excitatory nullcline: the region with positive slope is an unstable
branch; the regions with negative slope, including the
I axis (which is considered to have a
slope of 
), are stable branches.
Construction of the inhibitory nullcline is also done graphically:
again we plot
I(
E,
I) versus
I for various values of
E and look for intersections with the
line
I =
I
(Fig. 3B). These intersections correspond to points on the
inhibitory nullcline, which is drawn in black in the two-dimensional
(
E,
I)
plane to the right of the gain curves (Fig. 3C). In contrast
to the excitatory one, which has both stable and unstable branches, the inhibitory nullcline has a single branch that is everywhere stable at
fixed
E.
Construction of the nullclines in the other two regimes is a
straightforward extension of the above method. We thus turn our attention to how those nullclines affect the stability and location of
firing rate equilibria. We begin with regime 1, in which no cells are within one EPSP of threshold.
In regime 1 we find three intersections between the
excitatory and inhibitory nullclines, and thus three equilibria (Fig. 4A). A necessary condition for
the local stability of an equilibrium is that the inhibitory nullcline
intersect the excitatory one from below (Rinzel and Ermentrout
1998
|
E,
I)
plane and the unstable branch of the excitatory nullcline, as shown in
Fig. 4, A-C. The gap arises because neurons cannot fire
below 0 Hz. This lower bound effectively cuts off the bottom portion of
the excitatory nullclines, as seen in the nullcline construction, Fig.
3, A and C. Thus it is the lower bound on firing
rate that ultimately constrains the nullclines to have the shapes
depicted in Fig. 4, A-C. Given those shapes, simple
geometrical arguments determine the location and stability of the
firing rate equilibria.
In regime II, in which some neurons have their resting membrane
potential within one EPSP of threshold, a single action potential can
cause a chain reaction that ignites the network. Consequently, an
arbitrarily small excitatory firing rate is sufficient to produce network activity. This eliminates the gap in Fig. 4, A-C,
resulting in the nullclines illustrated in Fig. 4D. Figure
4D shows a low firing rate equilibrium (marked M, again for
metastable) that does not require the nullclines to have strong
curvature, so it can exist even in high connectivity networks. However,
the parameter range in which the equilibrium is stable is still
relatively narrow: small changes in single neuron properties can cause
resting membrane potentials to shift downward so that none of the cells
are within one EPSP of threshold, or upward so that some cells cross
threshold and become endogenously active. In addition, because
fluctuations can cause a drop to zero firing rate, where the network
will remain forever, the equilibrium is metastable. Again, this effect
can be traced to the fact that neurons cannot fire below 0 Hz.
The nullclines for regime 3, in which some cells are
endogenously active, are presented in Fig. 4E. The addition
of endogenously active cells eliminates the equilibrium along the
I axis, transforming the excitatory
nullcline from two distinct curves into one continuous one. This
transformation allows a robust, globally stable, low firing rate
equilibrium at the intersection between the excitatory and inhibitory
nullclines (marked S in Fig. 4E). The corresponding set of
nullclines in the high connectivity regime is shown in Fig.
4F.
The existence of a robust, stable low firing rate equilibrium when
endogenously active cells are present, and the absence of such an
equilibrium when they are not, leads to the following prediction: an
isolated network that fires steadily at low rate for an infinitely long
time must contain endogenously active cells. This does not mean that
such cells are absolutely essential for finite-lifetime, low firing
rate states; long-lived metastable states can exist in networks where
all cells have their resting membrane potential below threshold.
However, the parameter regime for this is narrow, and, as we will see
below, it vanishes altogether when spike-frequency adaptation is taken
into account.
These conclusions apply whether endogenous activity arises through an
intrinsic membrane property (e.g., a persistent inward current),
noise-driven voltage fluctuations, or any other mechanism. They also
apply to networks that receive external input. For example, consider a
network that has no endogenously active cells, but instead receives
sufficient external input that some cells fire without input from
neurons within the network. The existence of these pseudoendogenously
active cells place the network in regime 3, which allows a
robust low firing rate equilibrium to exist. If, on the other hand, the
same network receives external input that is too weak to cause any
neurons to fire, then a robust low firing rate equilibrium is not possible.
EFFECT OF ADAPTATION ON FIRING PATTERNS. So far we have assumed that the gain curves, and thus the nullclines, are static. In fact, this is not the case for real neurons. Because of spike-frequency and/or synaptic adaptation, nullclines are dynamic objects that depend on the history of activity, not just the activity at a single point in time. To incorporate this history into our analysis, we assume that neurons adapt slowly compared with the time it takes a network to reach equilibrium. Consequently, at any instant in time the equilibrium firing rates occur at the intersection of the excitatory and inhibitory nullclines, just as they did above. However, the equilibria are not fixed: adaptation causes slow changes in the nullclines, and thus in the equilibrium firing rates.
This process, slow changes in the level of adaptation accompanied by rapid relaxation to a local firing rate equilibrium, can have two distinct outcomes. One is that the firing patterns change very little: the firing rates may simply shift slightly, or, perhaps, oscillate slowly as adaptation affects the equilibrium and vice versa. The other is that adaptation-induced shifts in firing rate may be large enough that firing rate equilibria are created and destroyed. This much more dramatic effect occurs as follows. Consider a network that starts in a state characterized by the nullclines given in Fig. 5A. The black dot at the intersection of the excitatory and inhibitory nullclines corresponds to a firing rate equilibrium at a fixed level of adaptation. As the level of adaptation increases, the nullclines shift. Small shifts lead to a bistable state (Fig. 5B) but produce only a small change in firing rate. With larger shifts, however, the nullclines pull apart (Fig. 5C), and bistability gives way to a single stable state at zero firing rate. When this happens the network firing rate crashes to zero, at which point the level of adaptation starts to decrease. When the adaptation has dropped enough that the equilibrium at zero firing rate disappears (Fig. 5A via Fig. 5B), firing resumes and a new cycle starts.
|
max, which can be thought of as
the amount of constant depolarizing current that is injected into each
neuron. As long as
max > 0, the fraction of
endogenously active cells increases monotonically with
max, when
max = 0 the fraction of
endogenously active cells vanishes, and as
max becomes
negative, neurons are pushed below the threshold for the emission of an
action potential. The behavior of the model is shown in Fig.
6. Figure 6A confirms that
max, and thus the fraction of endogenously active cells, controls firing patterns: the network fires steadily when
max is large (many endogenously active cells are
present), makes a transition to bursting when
max falls
below a threshold, and becomes silent when
max drops
below zero and endogenously active cells vanish from the network.
Figure 6B summarizes the behavior of the model in the
bursting regime: the mean excitatory firing rate,
E, periodically makes sudden jumps in
firing rate, whereas the mean level of spike-frequency adaptation for the excitatory population, denoted GE, increases
slowly when the network is active and decreases slowly when the network
is silent. Bifurcation diagrams showing the equilibrium firing rate as
a function of the level of spike-frequency adaptation (the heavy black
curve) and the GE nullclines (the heavy gray
line) are given in Fig. 6, C-E for three regimes: silence
(C), bursting (D), and steady firing
(E). The thin, gray dashed path in the bifurcation diagrams
indicates the trajectory in firing rate/spike-frequency adaptation
space. It is the sudden jumps in this trajectory, at the "knees" of
the heavy black curve, that produce bursting.
|
STABILITY OF LOW FIRING RATE EQUILIBRIA.
Although endogenously active cells are necessary for the existence of a
stable, low firing rate equilibrium, such cells do not guarantee either
of these properties. As parameters change, a low firing rate
equilibrium can become unstable via a Hopf bifurcation (Marsden
and McCracken 1976
), or it can be driven to high firing rate.
In this section we investigate stability, then discuss conditions under
which a network is both stable and fires at low rate.
±, are
|
|
L,M

L/
M,
L, M = E, I, and the
partial derivatives are evaluated at the equilibrium. This last
quantity,
L,M, is proportional to coupling from neurons of type M to neurons of type
L; e.g.,
I,E is
proportional to excitatory to inhibitory coupling.
For an equilibrium to be stable both
+ and

must be negative. This requires that the determinant
of the above matrix, D, be positive and the trace,
T, negative. After minor manipulations of the determinant,
we find that to satisfy the first condition, D > 0, we
must have
|
(18) |
I,I and
E,I are negative.) It is not hard to show that Eq. 18 is satisfied as long as the slope of the
excitatory nullcline is less than the slope of the inhibitory one. As
can be seen in Fig. 4E, an equilibrium with this property is
guaranteed to exist in networks with endogenously active cells.
The second condition for stability, T < 0, may be
written
|
(19) |
I,I)/
I
(
E,E
1)/
E >
, where
depends primarily on
the level of spike-frequency adaptation.
Coupling affects overall firing rate as well as stability. We can
determine the relation between coupling and firing rate by first
categorizing its effect on the nullclines and then examining how shifts
in the nullclines affect firing rate. This is a straightforward application of previous analysis [e.g., increasing
I-I coupling lowers the inhibitory nullcline in
the (
E,
I) plane, which in turn increases the
excitatory firing rate]. The results, however, depend on the location
of the equilibrium; i.e., whether it occurs on the unstable (positively
sloped) branch of the excitatory nullcline, as in Fig. 4E,
or on the stable (negatively sloped) branch, as would occur if the
inhibitory nullcline in Fig. 4E were raised slightly. In
APPENDIX B we show that the excitatory nullcline has its
minimum at a very small value of the excitatory firing rate. The
precise value depends on single neuron and network properties, but for
high connectivity networks typical of the mammalian cortex, we estimate
in APPENDIX B that the minimum occurs below ~0.1 Hz. This
implies that if excitatory firing rates above ~0.1 Hz are observed in
a network firing at low rates, then the equilibrium must be
on the unstable branch of the excitatory nullcline. In fact, networks
exhibiting purely inhibitory activity are unusual: whole cell
recordings in vivo (Calabresi et al. 1990SUMMARY OF THEORETICAL ANALYSIS. The tool we used to analyze network behavior was a simplified firing rate model, in which the dynamics of networks containing greater than 104 neurons was reduced to a small number of equations describing average quantities. Rather than using a particular firing rate model, we used geometrical arguments to derive generic network behavior. Our primary assumptions were that, on average, excitatory input to a neuron increases its firing rate, inhibitory input decreases it, and neurons exhibit spike-frequency adaptation. With these assumptions, we were able to show that 1) endogenous activity is necessary for low firing rates, 2) decreasing the fraction of endogenously active cells causes a network to burst, and 3) firing patterns, especially transitions between steady firing and oscillations, are dependent on network connectivity. A specific realization of a simplified firing rate model corroborated these predictions.
Simulations
To test the predictions made in the previous section, we performed simulations with large networks of spiking model neurons, as described in METHODS. We examined 1) the effect of the distribution of applied depolarizing currents, Ia, on firing patterns and 2) how relative connection strengths among excitatory and inhibitory populations affect network behavior.
We used two networks, denoted A and B. These
networks differed primarily in their connectivity and the sizes of the
PSPs of their constituent neurons. Network A was designed to
simulate cortical networks. It contained 8,000 excitatory and 2,000 inhibitory neurons, and each neuron connected, on average, to 1,000 others. Connectivity was infinite range (meaning the probability of 2 neurons connecting did not depend on the distance between them; see
METHODS), and PSPs were on the order of 1 mV. Network
B was chosen to be consistent with our experiments (Latham
et al. 2000
) and to test whether the predictions made for
infinite range connectivity apply also to local connectivity, for which
the connection probability depends on distance between neurons. It had
fewer connections per neuron than Network A (200 instead of
1,000), local rather than infinite range connectivity, larger PSPs (on
the order of 5 mV rather than 1 mV), and a higher fraction of
inhibitory neurons (30% instead of 20%). A complete list of the
parameters for each network is given in Tables 1 and 2 of
METHODS.
Networks A and B behaved similarly, so in the bulk of this section we concentrate on Network A. At the end of the section we summarize the results of Network B.
ENDOGENOUS ACTIVITY. For networks without spike-frequency adaptation, the theoretical analysis presented above led to the following predictions. If endogenously active cells are present, then a stable, low firing rate equilibrium is possible. If endogenously active cells are absent, a low firing rate equilibrium is still possible. However, it is metastable; the network will eventually decay to a zero firing rate state. In this case there is a further distinction between networks in which some cells have their resting membrane potential within one EPSP of threshold and networks in which none do. This distinction has primarily qualitative bearing on firing patterns. In networks containing cells that are one EPSP from threshold, a single action potential can ignite activity in a silent network, so finite firing rate states tend to be long lived. In networks with no cells within one EPSP of threshold, finite firing rate states tend to have shorter lifetimes.
Networks with spike-frequency adaptation differ from those without it in two ways. First, as discussed in detail in the previous section, networks with spike-frequency adaptation exhibit a transition from steady firing to bursting as the fraction of endogenously active cells decreases. Second, in networks containing cells that are one EPSP from threshold but no endogenously active ones, the lifetime of the metastable state is extremely short
on the order of the
spike-frequency adaptation timescale, which is the inverse of the mean
network firing rate.
To test this set of predictions, and especially to examine how networks
with and without spike-frequency adaptation differed, we performed
simulations in which we varied the distribution of applied current,
Ia, both with and without spike-frequency
adaptation. We used a boxcar distribution in which
Ia was restricted to values between 0 and
Îmax. This distribution, which is
completely determined by Îmax, may be
divided into three regimes. These correspond to the three regimes just
discussed and to the ones listed in Theory.
| 1 | Îmax < ÎE1, where ÎE1 is the normalized applied current above which the resting membrane potential is within one EPSP of threshold. None of the cells have their resting membrane potential within one EPSP of threshold for the generation of an action potential, which implies that none are endogenously active. |
| 2 | ÎE1 < Îmax < Îthresh, where Îthresh is the threshold for endogenous activity. Some cells have their resting potential within one EPSP of threshold, but none are endogenously active. |
| 3 | Îthresh < Îmax. Endogenously active cells are present. |
cell. This is only 2%
(0.07/Îthresh) of the rheobase current for
a model cell whose resting membrane potential is 15 mV below threshold.
|
|
Îmax
3.5 and had a Gaussian tail for Îmax > 3.5. In the other, we
used a boxcar distribution but introduced noise-driven fluctuations in
the membrane voltage capable of generating endogenous activity. Both
simulations produced identical results, and those results were largely
in agreement with the sharp cutoff/no noise simulations. When there was
no spike-frequency adaptation, as the width of the Gaussian tail or the
noise increased we saw a transition from networks in which essentially
only the endogenously active cells fired to networks in which most of
the neurons were active. When spike-frequency adaptation was present, we observed transitions from silence to bursting to steady firing with
increasing tail width or noise. The only new phenomenon was a narrow
regime in which the network displayed irregular bursts. These bursts
were associated with the small number of endogenously active cells,
either in the tail of the distribution or produced by a relatively low
level of noise. Those cells caused random transitions between the
equilibria labeled "S" and "M" in Fig. 4B.
CONNECTIVITY. The theoretical predictions concerning the effect of coupling on stability and firing rate were 1) decreasing I-I and increasing E-E coupling both lead to oscillations in firing rate and 2) increasing same-type coupling (E-E or I-I) causes mean firing rates to go up, whereas increasing opposite-type coupling (E-I or I-E) causes mean firing rates to go down.
To test these predictions we performed simulations in which we varied the relative number of connections among the excitatory and inhibitory populations. This was done by adjusting the bias parameters, BE and BI (see METHODS), defined by BE
PIE
/PEE
and
BI
PII
/PEI
,
where PLM
is the probability of making a
connection from a neuron of type M to a neuron of type
L. Increasing BE increases
E-I (excitatory to inhibitory) coupling and
decreases E-E coupling; increasing BI increases I-I coupling
and decreases I-E coupling. Both occur without
changing the mean number of connections per neuron.
In terms of the bias parameters, the above predictions imply that
1) increasing BI and decreasing
BE cause firing rates to go up and 2)
decreasing both BE and BI
lead to oscillations. In addition, because spike-frequency adaptation
is most pronounced at high firing rates, we should see a transition to
bursting when the firing rate is high enough.
Mean excitatory and inhibitory firing rates are plotted in Fig.
9 versus time for a range of bias
parameters. These plots confirm the above predictions: increasing
BI and decreasing BE both
produced higher firing rates, networks with small
BI oscillated, and high firing rates were
accompanied by bursting. Bursting, however, was not guaranteed: we
increased BI to 2.4 with
BE fixed at 1.0 without observing bursting, even
though the excitatory firing rate at these parameters approached 40 Hz.
|
K
Ca,E, corresponds to the mean level of excitatory spike-frequency
adaptation (
K
Ca,E
NE
1
i
E
K
Ca,i, where the sum is
over excitatory neurons; see Eq. 5c);
K
Ca,E is
analogous to GE in the reduced firing rate model
(Eq. 15c). Like GE in Fig. 6B,
K
Ca,E increases when
the network is active and decreases when the network is silent.
The transition from oscillations to steady firing was gradual and never
quite complete; even at high values of BI, where
the fixed points should be attracting, there was an oscillatory
component to the firing rates. However, the amplitude of the
oscillations decreased when the number of neurons increased: in Fig. 9,
B, C, E, and F, the variance in the firing rate
(for Fig. 9F the variance only during bursts) dropped by a
factor of ~2 when we doubled the number of neurons (data not shown).
This indicates that the oscillations at large BI
result from the finite size of the network, which allows fluctuations
that are converted to oscillations by the dynamics. In contrast,
doubling the number of neurons had virtually no effect on the variance
in the firing rate when the inhibitory-inhibitory coupling was low
enough to produce oscillations, as in Fig. 9, A and
D.
Finally, to ensure that the oscillations in Fig. 9A were not
caused by spike-frequency adaptation, we performed simulations with the
same parameters except that spike-frequency adaptation was eliminated
(
K
Ca was set to zero; see
METHODS). We found a decrease in the oscillation period,
from 180 to 120 ms, but no other change in the firing pattern.
LOCAL CONNECTIVITY. The above simulations were repeated with parameters corresponding to Network B, in which the connectivity is local rather than infinite range (meaning neurons that are close together are more likely to connect than those that are far apart), the number of connections per neuron is smaller than in Network A, and the PSPs are larger (see Tables 1 and 2). The results are summarized in Figs. 10 and 11.
|
|
K
Ca,E.
Again the results were substantially the same as for the network with
infinite range connectivity. There were, however, differences in the
details. For example, we did not see regular oscillations for any of
the examples shown: for all plots the variance in the firing rate dropped by a factor of ~2 when we doubled the number of neurons, indicating that the observed fluctuations were caused by the finite size of the network. Oscillations did occur when we reduced
I-I coupling, but not until
BI was below ~0.6. In addition, the local connectivity network burst more easily than the infinite range one and
the bursting was more irregular. Bursting was observed for
BE = 1.0 and BI
1.0, whereas in Fig. 9 bursting was not observed at all for
BE = 1.0.
These plots indicate that, in spite of the differences between
Networks A and B, the two networks generated
strikingly similar results. This indicates that our model is robust to
changes in connectivity (especially infinite range vs. local) as well
as the number of connections per neuron and PSP size.
SUMMARY OF SIMULATION RESULTS. We performed simulations with two very different networks: an infinite range, high connectivity network with small PSPs, and a local, low connectivity network with large PSPs. We also examined a broad range of parameters, including the distribution of applied currents, spike-frequency adaptation, and network connectivity. The results of all simulations were as predicted: for networks without spike-frequency adaptation, we observed transitions from silence to steady firing as the fraction of endogenously active cell increased. For networks with spike-frequency adaptation, there was an intermediate regime in which the networks burst. Finally, when the I-I coupling was strengthened, we observed transitions from oscillations to steady firing to bursting and an increase in firing rate.
| |
DISCUSSION |
|---|
|
|
|---|
We have investigated, both theoretically and through simulations with spiking model neurons, the intrinsic dynamics in large networks of neurons. The goal of this work was twofold: 1) to understand how dynamic interactions between excitatory and inhibitory neurons lead to stable, low firing rates, such as those widely observed in the mammalian central nervous system, and 2) to determine the conditions under which networks switch from steady firing to bursting.
An understanding of the mechanism for generating stable, low firing
rates in large, isolated neuronal networks has been elusive (Abeles 1991
; Amit and Treves 1989
;
Buhmann 1989
; Treves and Amit 1989
). The
elusiveness stems from the difficulty in controlling the powerful
recurrent excitation that exists in such networks. To compensate for
this recurrent excitation, inhibitory feedback is required. To
stabilize low firing rates, that feedback must be strong enough that
the inhibitory firing rate is more sensitive to input from excitatory
cells than the excitatory firing rate. Or, in the language of dynamics,
the inhibitory nullcline in average firing rate space must be steeper
than the excitatory one at the equilibrium (e.g., Fig. 4E).
We found that for isolated networks, the above condition occurs
robustly at low firing rate only when endogenously active
cells are present; without such cells networks are either silent or
fire at high rate. This led to the following prediction: if low firing
rates are observed in an isolated network, then that network must
contain endogenously active cells. This prediction was confirmed by
large-scale network simulations, which included the exploration of a
broad range of parameters to ensure that the simulations were robust
(APPENDIX A). It was also corroborated by experiments in
cultured neuronal networks, as described in the accompanying paper
(Latham et al. 2000
).
Although endogenously active cells are necessary for the existence of a
low firing rate equilibrium, they do not guarantee its stability. In
particular, we found that a high level of spike-frequency adaptation
leads to bursting: repetitive firing can introduce a hyperpolarizing
current sufficient to temporarily eliminate endogenously active cells,
resulting in a crash to zero firing rate; after the cells stop firing,
the hyperpolarizing current decays and firing resumes. (Interestingly,
our analysis implies that synaptic adaptation, because it does not
affect the fraction of endogenously active cells, cannot produce
bursting.) The probability of bursting is highest if there are few
endogenously active cells to begin with, and for that reason the
fraction of such cells plays a key role in determining firing patterns.
Specifically, networks with no endogenously active cells are typically
silent; at some finite fraction of endogenously active cells there is a
transition to bursting; and at an even higher fraction there is a
second transition to steady firing at low rate. This scenario was also
confirmed by network simulations, and it was corroborated by
experiments in neuronal cell culture (Latham et al.
2000
).
Although the fraction of endogenously active cells plays the dominant role in determining the primary firing patterns (silence, bursting, or steady firing), another parameter, network connectivity, influences secondary features of the firing patterns. Specifically, when inhibitory-inhibitory coupling becomes too weak or excitatory-excitatory coupling becomes too weak or excitatory-excitatory coupling becomes too strong, a low firing rate equilibrium can be destabilized via a Hopf bifurcation. This leads to oscillations in firing rate that can occur in both the "steady" firing and the bursting regimes. In the latter case, the oscillations occur during the active phase of the burst.
These theoretical findings were based on the analysis of isolated networks with random, infinite-range connectivity. However, theoretical considerations indicate that they apply to networks that receive external input, and simulations indicate that they are valid for networks with local connectivity, in which the connection probability is a decreasing function of distance between neurons. The validity of the model for local connectivity suggests that these findings will hold for the more structured architecture that exists in the cortex.
Implications
Two firing patterns that are ubiquitous in the mammalian CNS are
steady firing at low rates and rhythmic bursting. We have shown that,
in isolated networks, both firing patterns are controlled largely by a
single parameter, the fraction of endogenously active cells. As long as
the fraction of such cells is above a threshold, steady firing is
possible; below that threshold the network bursts. The threshold
depends on the degree of spike-frequency adaptation, a property of
neurons that has been shown to be modulatable [e.g., by
neuromodulators (Burke and Hablitz 1996
; Cole and
Nicoll 1984
; McCormick et al. 1993
;
Pedarzani and Storm 1993
; Spain, 1994
)]. Thus the model described here both accounts for the low firing rates
observed in networks throughout the mammalian CNS and provides a
natural mechanism for switching between steady firing and bursting. A
switch between these two patterns is necessary for behavior that is
activated episodically, such as locomotion, scratching, and swallowing
(Berkinblit et al. 1978
; Kudo and Yamada
1987
; Zoungrana et al. 1997
).
Although endogenously active cells may account for the observed firing
patterns in mammalian neuronal networks, they are not necessarily responsible for those firing patterns. This is
because the brain is neither isolated nor comprised of a single
network. Instead, it receives sensory input and consists of distinct
areas that interact through long-range connections. Because external input to a network can drive cells even when they are not receiving input from within the network (making those cells effectively endogenously active), it is possible that the low firing rates observed
in cortex are generated by sensory input, or, as has been proposed by
Amit and Brunel (1997)
, by input from other brain areas.
The source of the input does not affect our model, however; the model
applies whether the input is external or endogenous.
The theory developed here provides a framework for understanding intrinsic firing patterns and their dynamics in large networks of neurons. This does more than simply explain observed firing patterns; it provides a link between basic properties of networks and a way to understand how firing patterns could be modified by patterned external input. This link is critical for developing models of how computations are performed by real neuronal networks.
| |
APPENDIX A: ROBUSTNESS TO VARIATION IN PARAMETERS |
|---|
|
|
|---|
To exhaustively check the robustness of our model would require
a complete exploration of the full parameter space, which is
impractical for the 26-dimensional space that describes our model.
Instead, we varied a selected subset of the parameters. Our starting
point was a set of parameters taken from two networks, Networks
A and B. Recall that most of the parameters of those networks are given in Tables 1 and 2; the parameters whose values are
not listed there were given the following values:
Îmax = 5.0, BE = BI = 1.0, and

K
Ca = 0. This set of
parameters resulted in mean excitatory firing rates of 5.59 and 4.51 Hz
for Networks A and B, respectively, and
inhibitory rates of 5.59 and 4.46 Hz. The firing patterns were steady;
i.e., no bursting or oscillations. Starting with this initial set of parameters, the ones we varied to explore the robustness of our model
were as follows: 1) the amplitude of the excitatory and inhibitory postsynaptic potentials, VEPSP and
VIPSP, 2) the fraction of inhibitory
cells, 3) the voltage threshold, Vt,
4) the cell time constant,
cell,
5) the mean number of connections per neurons, K,
6) the number of neurons, N, 7) the
distribution of applied current, and 8) for Network
B (the one with local connectivity), the axonal spreads of the
excitatory and inhibitory populations,
E and
I.
The first four items in this list had the strongest effect on
firing rate: for both networks, a 50% increase in EPSP amplitude, a
50% decrease in IPSP amplitude, and a 25% decrease in the fraction of
inhibitory cells all caused an increase in firing rate of ~50%; increasing the distance between the nominal resting membrane potential and threshold, Vt
Vr,
from 15 to 25 mV while keeping the fraction of endogenously active
cells fixed resulted in a drop in firing rate of ~50%, and doubling
the time constant resulted in a drop in firing rate of ~40%.
Increasing the mean number of connections per neuron, K, also had a moderately strong effect on firing rate: a 20% increase in K resulted in a decrease in firing rate of 12% for Network A and 14% for Network B. Somewhat surprisingly, increasing the amplitudes of both EPSPs and IPSPs did not have the same effect as increasing the number of connections: a 20% increase in VEPSP and VIPSP led to a 7% decrease in firing rate for Network A and a 4% increase in firing rate for Network B. The reason for the difference is as follows. Although increasing PSP amplitude and connectivity have approximately the same effect on mean synaptic drive, the former has a larger effect on variance. Because larger input variance leads to higher firing rate, increasing PSP amplitude is more effective in causing a cell to fire than increasing connectivity. This is why firing rates were higher with a 20% increase in PSP amplitude than they were with a 20% increase in the number of connections.
Increasing the number of neurons had almost no effect on firing rate (<7% change when the number of neurons doubled). However, there was a substantial reduction in fluctuations: doubling the number of neurons in Network A caused the variance in the firing rate to drop by a factor of 2.3, and doubling the number in Network B reduced the variance by a factor of 1.93. Both of these are close to the factor of 2 suggested by 1/N scaling.
The analysis in the main text was based on gain curves constructed from
a unimodal distribution of applied depolarizing currents, Ia. Such a distribution implies that the neurons
in the network have a continuous range of resting membrane potentials,
and, if there are endogenously active cells, the active neurons have a continuous range of firing rates. Different distributions, especially multimodal ones, can lead to different nullclines and thus different network behavior (Wilson and Cowan 1972
). We thus
considered a bimodal distribution in which the normalized applied
current, Îa, at each neuron was either 0 mV (resting membrane potential 15 mV below threshold) or 5 mV
(endogenously active). For the two bimodal distributions we looked at,
30 and 50% of the cells endogenously active, the firing rates changed
by <5%. Thus, at least for these parameters, changing the
distribution of applied currents had little effect on firing rate.
The effect of changing the axonal spread depended on whether we
changed the spread for the inhibitory or the excitatory neurons. Increasing the normalized radius of the inhibitory axonal spread,
I, from 0.12 to 0.25 and then to 0.50 increased the firing rate by 50 and 132%, respectively. (Recall that
the normalized radius of the network is 1.) These results are
consistent with the view that inhibition is acting to control local hot
spots of excitatory activity, so overly diffuse inhibition is not so effective. Increasing the excitatory axonal spread,
E, on the other hand, led to a decrease in
firing rate that was fairly small: increasing
E from 0.12 to 0.25 and 0.50 dropped the
firing rate by 4 and 13%, respectively. Our interpretation here is
that longer range excitation allows the recruitment of additional
inhibitory neurons, thus lowering firing rates.
In all cases, the above parameter changes produce changes in firing rate consistent with our model. This is indicative that the model is relatively robust. This should not be surprising, in view of Fig. 4E, which guarantees an equilibrium at reasonably low firing rate.
We end with a simulation closer to cortical parameters than we have
been using: Network A with IPSP and EPSP amplitudes of
1
and 0.2 mV, respectively, 20,000 neurons of which 15% were inhibitory,
a threshold voltage of
40 mV, corresponding to a nominal gap between
resting and threshold of 25 mV, and a maximum for the boxcar
distribution, Îmax, equal to 10 mV. The
network with these parameters fired steadily with a mean rate of 0.9 Hz.
| |
APPENDIX B: ESTIMATE OF THE MINIMUM OF THE EXCITATORY NULLCLINE |
|---|
|
|
|---|
In this appendix we estimate the size of
*E, the average excitatory
firing rate at the minimum of the excitatory nullcline. To do this we
derive a differential equation for
E(
E,
I) valid when
E is small, solve it to determine the
shape of the excitatory gain function, and then find the tangential intersection with the line
E(
E,
I) =
E. We start with the relation
|
(B1) |
|
(B2) |
|
(B3) |
V(t) is the change in membrane
potential caused by the arrival of an EPSP,
Rcell is the cell membrane resistance, VEPSP is the amplitude of a typical EPSP, and
t is the characteristic width of an EPSP. This last
quantity,
t, is defined by the second equality in
Eq. B3.
When the response to an EPSP is linear, it is not hard to show that
t
cell. We will assume that EPSPs
are small enough that the linear approximation holds, in which case
Eq. B2 can be replaced with the inequality
|
(B4) |

E/
Isyn,E,
is the rate of change of the average firing rate of a network of neurons with respect to the synaptic drive. This can be estimated as
follows. For a single cell, the slope of the frequency-current (F-I) curve is small below some threshold current
and approximately linear above it. [For the type I neurons used here,
spike initiation occurs via a saddle-node bifurcation, which leads to a
square-root F-I curve with respect to
constant injected current (Rinzel and Ermentrout
1998
E/
Isyn,E
is the slope above threshold, denoted F', times the fraction
of cells above threshold, denoted
. We thus have
|
|
(B5) |
|
(B6) |
E(
E,
I) as a function of
E, we need to know how
depends on
the firing rates,
I and
E. We can estimate this dependence as
follows. Let
Isyn,E be the minimum
current that will make almost all cells in the network fire. Then, the excitatory firing rate that will make almost every cell fire is
Isyn,E/(
Isyn,E/
E).
Defining
|
(B7) |
E increases from
0 to 
, the fraction of active cells increases from its value at
E = 0 Hz, which we denote
0(
I), to 1. For clarity,
in the remainder of this analysis we will drop the dependence of
0 on
I. Assuming that
the fraction of active cells increases linearly for
E < 
, we can write
=
0 + (1
0)
E/
. Then,
Eq. B5 becomes, for small values of
E
|
(B8) |
|
(B9) |
E =
E.
It is straightforward to show that the value of the average excitatory
firing rate at that tangential intersection,
*E, is given by
|
(B10) |
> 1, the right hand side of
Eq. B10 is maximum when
0 = 0. Consequently, we can bound
*E by
|
(B11) |

depends on
Isyn,E, the minimum current needed
to make all the cells in the network fire (Eq.
B7). The minimum current consists of two parts: the minimum
rheobase current plus the total inhibitory synaptic current delivered
to a cell. The latter quantity is
I
Isyn,I/
I. Denoting the minimum rheobase current as Irh and
using the same argument as above to express
Isyn,I/
I
in terms of physiological quantities, we arrive at
|
(B12) |

|
|
(B13) |
|
(B14a) |
|
(B14b) |
*E, we need to know the sizes
of
,
rh, and
. A bound on the first of these,
,
is found by combining Eq. B4 with the definition
of
in Eq. B6, yielding
|
(B15) |
cell with a time constant of 10 ms,
cellVEPSP/Rcell = 3.3 × 10
4 nA/Hz × VEPSP (mV). Because
KEEVEPSP (mV) is typically at least 103, the first three terms on the right hand side of
Eq. B15 should be larger than ~0.33 nA/Hz. The
remaining term in Eq. B15, the slope of a cell's
F-I curve, is typically on the order of 250 Hz/nA
(McCormick et al. 1985
, the
slope of the F-I curve was ~150 Hz/nA;
simulations not shown.) Using 250 Hz/nA for the
F-I curve, we arrive at
83.
|
The quantity
rh given in Eq.
B14a has almost the same factors as
; the only difference
is that F' is replaced by 1/Irh and the expression is inverted. For typical cells,
Irh is at most 0.2 nA (McCormick et al.
1985
). Combining this value with the above estimate for
cellVEPSPKEE/Rcell,
we find that
rh ~ 0.6 Hz.
Finally if excitatory and inhibitory neurons have similar PSP sizes and
connectivities,
~ 1. Thus Eq. B13 can
be written
|
(B16) |
*I. Unless
*I is very large,
*E will be small, almost
certainly below 0.1 Hz.
Testing the validity of the above analysis requires that we construct the excitatory nullcline. This can be done in our simulations by slowly increasing the value of Îmax for the inhibitory neurons only, which shifts the inhibitory nullcline up without affecting the excitatory one. By recording the equilibrium firing rates as we shift the inhibitory nullcline, we can sweep out the excitatory nullcline. An excitatory nullcline constructed in this manner is shown in Fig. 12B. Consistent with the bound given in Eq. B16, the minimum of the inhibitory nullcline occurs at an excitatory firing rate of 0.014 Hz.
| |
ACKNOWLEDGMENTS |
|---|
We thank E. Neale for providing Epon-embedded cultures containing the HRP-injected neurons used to measure axonal arborization and C. Del Negro, J. Rinzel, and M. Wiener for insightful discussions and comments on this manuscript.
| |
FOOTNOTES |
|---|
Address for reprint requests: P. E. Latham, Dept. of Neurobiology, UCLA, Box 95-1763, Los Angeles, CA 90095-1763.
The costs of publication of this article were defrayed in part by the payment of page charges. The article must therefore be hereby marked "advertisement" in accordance with 18 U.S.C. Section 1734 solely to indicate this fact.
Received 5 March 1999; accepted in final form 30 September 1999.
| |
REFERENCES |
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