Some results on interspike interval statistics in conductance-based models for neuron action potentials

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Some results on interspike interval statistics in conductance-based models for neuron action potentials Nils Berglund MAPMO, Université d Orléans CNRS, UMR 7349 et Fédération Denis Poisson www.univ-orleans.fr/mapmo/membres/berglund nils.berglund@math.cnrs.fr Collaborators: Barbara Gentz (Bielefeld) Christian Kuehn (Vienne), Damien Landon (Orléans) Projet ANR MANDy, Mathematical Analysis of Neuronal Dynamics Random Models in Neuroscience UPMC, Paris, July 5, 2012

The Poisson hypothesis Action potential [Dickson 00] Interspike interval (ISI) statistics (under random stimulation) 1

The Poisson hypothesis Action potential [Dickson 00] Interspike interval (ISI) statistics (under random stimulation) Poisson hypothesis: ISI has exponential distribution Consequence: Markov property 1-a

The Poisson hypothesis Action potential [Dickson 00] Interspike interval (ISI) statistics (under random stimulation) Poisson hypothesis: ISI has exponential distribution Consequence: Markov property For which models is it a good approximation? What ISI can we expect for other (stochastic, conductance-based) models? 1-b

The stochastic exit problem Stochastic differential equation (SDE) dx t = f(x t ) dt + σg(x t ) dw t x R n Exit problem: Given D R n, characterise First-exit time (and location) τ D = inf{t > 0: x t D} D x τd 2

The stochastic exit problem Stochastic differential equation (SDE) dx t = f(x t ) dt + σg(x t ) dw t x R n Exit problem: Given D R n, characterise First-exit time (and location) τ D = inf{t > 0: x t D} D x τd When do we have lim σ 0 P { τ D > se[τ D ] } = e s? 2-a

The stochastic exit problem Stochastic differential equation (SDE) dx t = f(x t ) dt + σg(x t ) dw t x R n Exit problem: Given D R n, characterise First-exit time (and location) τ D = inf{t > 0: x t D} D x τd When do we have lim σ 0 P { τ D > se[τ D ] } = e s? True if n = 1 true for integrate-and-fire models True if D basin of attraction [Day 83] True if f(x) = U(x) and g(x) = 1l [Bovier et al 04] 2-b

The stochastic exit problem Stochastic differential equation (SDE) dx t = f(x t ) dt + σg(x t ) dw t x R n Exit problem: Given D R n, characterise First-exit time (and location) τ D = inf{t > 0: x t D} D x τd When do we have lim σ 0 P { τ D > se[τ D ] } = e s? True if n = 1 true for integrate-and-fire models True if D basin of attraction [Day 83] True if f(x) = U(x) and g(x) = 1l [Bovier et al 04] Not necessarily true if n 2, curl f 0 and D det orbit 2-c

Deterministic FitzHugh Nagumo (FHN) equations Consider the FHN equations in the form εẋ = x x 3 + y ẏ = a x by x membrane potential of neuron y proportion of open ion channels (recovery variable) ε 1 fast slow system b = 0 in the following for simplicity 3

Deterministic FitzHugh Nagumo (FHN) equations Consider the FHN equations in the form εẋ = x x 3 + y ẏ = a x by x membrane potential of neuron y proportion of open ion channels (recovery variable) ε 1 fast slow system b = 0 in the following for simplicity Stationary point P = (a, a 3 a) Linearisation has eigenvalues δ± δ 2 ε ε where δ = 3a2 1 2 δ > 0: stable node (δ > ε ) or focus (0 < δ < ε ) δ = 0: singular Hopf bifurcation [Erneux & Mandel 86] δ < 0: unstable focus ( ε < δ < 0) or node (δ < ε ) 3-a

Deterministic FitzHugh Nagumo (FHN) equations δ > 0: P is asymptotically stable the system is excitable one can define a separatrix 4

Deterministic FitzHugh Nagumo (FHN) equations δ > 0: P is asymptotically stable the system is excitable one can define a separatrix δ < 0: P is unstable asympt. stable periodic orbit sensitive dependence on δ: canard (duck) phenomenon [Callot, Diener, Diener 78, Benoît 81,... ] 4-a

Deterministic FitzHugh Nagumo (FHN) equations δ > 0: P is asymptotically stable the system is excitable one can define a separatrix δ < 0: P is unstable asympt. stable periodic orbit sensitive dependence on δ: canard (duck) phenomenon [Callot, Diener, Diener 78, Benoît 81,... ] 4-b

Stochastic FHN equations dx t = 1 ε [x t x 3 t + y t ] dt + σ 1 ε dw (1) t dy t = [a x t ] dt + σ 2 dw (2) t W t (1), W t (2) : independent Wiener processes 0 < σ 1, σ 2 1, σ = σ1 2 + σ2 2 5

Stochastic FHN equations dx t = 1 ε [x t x 3 t + y t ] dt + σ 1 ε dw (1) t dy t = [a x t ] dt + σ 2 dw (2) t W t (1), W t (2) : independent Wiener processes 0 < σ 1, σ 2 1, σ = σ1 2 + σ2 2 ε = 0.1 δ = 0.02 σ 1 = σ 2 = 0.03 5-a

Some previous work Numerical: Kosmidis & Pakdaman 03,..., Borowski et al 11 Moment methods: Tanabe & Pakdaman 01 Approx. of Fokker Planck equ: Lindner et al 99, Simpson & Kuske 11 Large deviations: Muratov & Vanden Eijnden 05, Doss & Thieullen 09 Sample paths near canards: Sowers 08 6

Some previous work Numerical: Kosmidis & Pakdaman 03,..., Borowski et al 11 Moment methods: Tanabe & Pakdaman 01 Approx. of Fokker Planck equ: Lindner et al 99, Simpson & Kuske 11 Large deviations: Muratov & Vanden Eijnden 05, Doss & Thieullen 09 Sample paths near canards: Sowers 08 Proposed phase diagram [Muratov & Vanden Eijnden 08] σ σ = δ 3/2 ε 3/4 σ = (δε) 1/2 σ = δε 1/4 ε 1/2 δ 6-a

Intermediate regime: mixed-mode oscillations (MMOs) Time series t x t for ε = 0.01, δ = 3 10 3, σ = 1.46 10 4,..., 3.65 10 4 7

Precise analysis of sample paths 8

Precise analysis of sample paths Dynamics near stable branch, unstable branch and saddle node bifurcation: already done in [B & Gentz 05] Dynamics near singular Hopf bifurcation: To do 8-a

Precise analysis of sample paths Dynamics near stable branch, unstable branch and saddle node bifurcation: already done in [B & Gentz 05] Dynamics near singular Hopf bifurcation: To do 8-b

Small-amplitude oscillations (SAOs) Definition of random number of SAOs N: nullcline y = x 3 x D P separatrix F, parametrised by R [0, 1] 9

Small-amplitude oscillations (SAOs) Definition of random number of SAOs N: nullcline y = x 3 x D P separatrix F, parametrised by R [0, 1] (R 0, R 1,..., R N 1 ) substochastic Markov chain with kernel K(R 0, A) = P R 0{R τ A} R F, A F, τ = first-hitting time of F (after turning around P ) N = number of turns around P until leaving D 9-a

General results on distribution of SAOs General theory of continuous-space Markov chains: [Orey 71, Nummelin 84] Principal eigenvalue: eigenvalue λ 0 of K of largest module. λ 0 R Quasistationary distribution: prob. measure π 0 s.t. π 0 K = λ 0 π 0 10

General results on distribution of SAOs General theory of continuous-space Markov chains: [Orey 71, Nummelin 84] Principal eigenvalue: eigenvalue λ 0 of K of largest module. λ 0 R Quasistationary distribution: prob. measure π 0 s.t. π 0 K = λ 0 π 0 Theorem 1: [B & Landon, 2011] Assume σ 1, σ 2 > 0 λ 0 < 1 K admits quasistationary distribution π 0 N is almost surely finite N is asymptotically geometric: lim n P{N = n + 1 N > n} = 1 λ 0 E[r N ] < for r < 1/λ 0, so all moments of N are finite 10-a

General results on distribution of SAOs General theory of continuous-space Markov chains: [Orey 71, Nummelin 84] Principal eigenvalue: eigenvalue λ 0 of K of largest module. λ 0 R Quasistationary distribution: prob. measure π 0 s.t. π 0 K = λ 0 π 0 Theorem 1: [B & Landon, 2011] Assume σ 1, σ 2 > 0 λ 0 < 1 K admits quasistationary distribution π 0 N is almost surely finite N is asymptotically geometric: lim n P{N = n + 1 N > n} = 1 λ 0 E[r N ] < for r < 1/λ 0, so all moments of N are finite Proof: uses Frobenius Perron Jentzsch Krein Rutman Birkhoff theorem [Ben Arous, Kusuoka, Stroock 84] implies uniform positivity of K which implies spectral gap 10-b

Histograms of distribution of SAO number N (1000 spikes) σ = ε = 10 4, δ = 1.2 10 3,..., 10 4 140 160 120 140 100 80 60 40 120 100 80 60 40 20 20 0 0 500 1000 1500 2000 2500 3000 3500 4000 600 500 400 300 200 100 0 0 10 20 30 40 50 60 70 1000 0 0 50 100 150 200 250 300 900 800 700 600 500 400 300 200 100 0 0 1 2 3 4 5 6 7 8 11

Dynamics near the separatrix Change of variables: Translate to Hopf bif. point Scale space and time Straighten nullcline ẋ = 0 variables (ξ, z) where nullcline: {z = 1 2 } where dξ t = dz t = ( ) 1 ε 2 z t 3 ξ3 t ( µ + 2ξ t z t + 2 ε 3 ξ4 t dt + σ 1 dw (1) ) t dt 2 σ 1 ξ t dw t (1) + σ 2 dw t (2) µ = δ ε σ 2 1 σ 1 = 3 σ 1 ε 3/4 σ 2 = 3 σ 2 ε 3/4 12

Dynamics near the separatrix Change of variables: Translate to Hopf bif. point Scale space and time Straighten nullcline ẋ = 0 variables (ξ, z) where nullcline: {z = 1 2 } where dξ t = dz t = ( ) 1 ε 2 z t 3 ξ3 t ( µ + 2ξ t z t + 2 ε 3 ξ4 t dt + σ 1 dw (1) ) t dt 2 σ 1 ξ t dw t (1) + σ 2 dw t (2) µ = δ ε σ 2 1 σ 1 = 3 σ 1 ε 3/4 σ 2 = 3 σ 2 ε 3/4 Upward drift dominates if µ 2 σ 2 1 + σ2 2 (ε1/4 δ) 2 σ 2 1 + σ2 2 Rotation around P : use that 2z e 2z 2ξ2 +1 is constant for µ = ε = 0 12-a

Dynamics near the separatrix (a) z (b) z ξ ξ (c) z (d) z ξ ξ 13

Transition from weak to strong noise Linear approximation: dz 0 t = ( µ + tz 0 t ) dt σ1 t dw t (1) + σ 2 dw t (2) ( ) P{no SAO} Φ π 1/4 µ σ 1 2+ σ2 2 Φ(x) = x e y2 /2 2π dy 14

Transition from weak to strong noise Linear approximation: dz 0 t = ( µ + tz 0 t ) dt σ1 t dw t (1) + σ 2 dw t (2) ( ) P{no SAO} Φ π 1/4 µ σ 1 2+ σ2 2 Φ(x) = x e y2 /2 2π dy 1 0.9 0.8 0.7 0.6 0.5 0.4 series 1/E(N) P(N=1) phi : P{no SAO} +: 1/E[N] : 1 λ 0 curve: x Φ(π 1/4 x) 0.3 0.2 0.1 x = µ σ 1 2+ σ2 2 = ε1/4 (δ σ 1 2/ε) σ1 2+σ2 2 0 1.5 1 0.5 0 0.5 1 1.5 2 µ/σ 14-a

The weak-noise regime Theorem 2: [B & Landon 2011] Assume ε and δ/ ε sufficiently small There exists κ > 0 s.t. for σ 2 (ε 1/4 δ) 2 / log( ε/δ) 15

The weak-noise regime Theorem 2: [B & Landon 2011] Assume ε and δ/ ε sufficiently small There exists κ > 0 s.t. for σ 2 (ε 1/4 δ) 2 / log( ε/δ) Principal eigenvalue: 1 λ 0 exp { κ (ε1/4 δ) 2 σ 2 } 15-a

The weak-noise regime Theorem 2: [B & Landon 2011] Assume ε and δ/ ε sufficiently small There exists κ > 0 s.t. for σ 2 (ε 1/4 δ) 2 / log( ε/δ) Principal eigenvalue: 1 λ 0 exp { κ (ε1/4 δ) 2 Expected number of SAOs: E µ 0[N] C(µ 0 ) exp {κ (ε1/4 δ) 2 where C(µ 0 ) = probability of starting on F above separatrix σ 2 σ 2 } } 15-b

The weak-noise regime Theorem 2: [B & Landon 2011] Assume ε and δ/ ε sufficiently small There exists κ > 0 s.t. for σ 2 (ε 1/4 δ) 2 / log( ε/δ) Principal eigenvalue: 1 λ 0 exp { κ (ε1/4 δ) 2 Expected number of SAOs: E µ 0[N] C(µ 0 ) exp {κ (ε1/4 δ) 2 Proof: where C(µ 0 ) = probability of starting on F above separatrix Construct A F such that K(x, A) exponentially close to 1 for all x A Use two different sets of coordinates to approximate K: Near separatrix, and during SAO σ 2 σ 2 } } 15-c

The story so far Three regimes for δ < ε: σ ε 1/4 δ: rare isolated spikes interval Exp( ε e (ε1/4 δ) 2 /σ 2 ) σ ε 3/4 σ = (δε) 1/2 σ = δ 3/2 ε 1/4 δ σ ε 3/4 : transition asympt geometric nb of SAOs σ = (δε) 1/2 : geometric(1/2) σ = δε 1/4 σ ε 3/4 : repeated spikes ε 1/2 δ 16

The story so far Three regimes for δ < ε: σ ε 1/4 δ: rare isolated spikes interval Exp( ε e (ε1/4 δ) 2 /σ 2 ) σ ε 3/4 σ = (δε) 1/2 σ = δ 3/2 ε 1/4 δ σ ε 3/4 : transition asympt geometric nb of SAOs σ = (δε) 1/2 : geometric(1/2) σ = δε 1/4 σ ε 3/4 : repeated spikes ε 1/2 δ Perspectives interspike interval distribution periodically modulated exponential how is it modulated? transient effects are important - bias towards N = 1 relation between P{no SAO}, 1/E[N] and 1 λ 0 consequences of postspike distribution µ 0 π 0 sharper bounds on λ 0 (and π 0 ) 16-a

Higher dimensions Systems with one fast and two slow variables Fold Unstable slow manifold Stable slow manifold Stable slow manifold Folded node Fold 17

Folded node singularity Normal form [Benoît, Lobry 82, Szmolyan, Wechselberger 01]: ɛẋ = y x 2 ẏ = (µ + 1)x z (+ higher-order terms) ż = µ 2 18

Folded node singularity Normal form [Benoît, Lobry 82, Szmolyan, Wechselberger 01]: ɛẋ = y x 2 ẏ = (µ + 1)x z (+ higher-order terms) ż = µ 2 y C r 0 C a 0 x L z 18-a

Folded node singularity Theorem [Benoît, Lobry 82, Szmolyan, Wechselberger 01]: For 2k + 1 < µ 1 < 2k + 3, the system admits k canard solutions The j th canard makes (2j + 1)/2 oscillations Mixed-mode oscillations (MMOs) Picture: Mathieu Desroches 18-b

Effect of noise dx t = 1 ε (y t x 2 t ) dt + σ ε dw (1) t dy t = [ (µ + 1)x t z t ] dt + σ dw (2) t dz t = µ 2 dt + h.o.t. Noise smears out small amplitude oscillations Early transitions modify the mixed-mode pattern 19

Main results Theorem 3: [B, Gentz, Kuehn 2010] For z 0, paths stay with high probability in covariance tubes For z = 0, section of tube is close to circular with radius µ 1/4 σ Distance between k th and k + 1 st canard e (2k+1)2 µ 20

20-a

Main results Theorem 3: [B, Gentz, Kuehn 2010] For z 0, paths stay with high probability in covariance tubes For z = 0, section of tube is close to circular with radius µ 1/4 σ Distance between k th and k + 1 st canard e (2k+1)2 µ Corollary: Let σ k (µ) = µ 1/4 e (2k+1)2 µ Canards with 2k+1 4 oscillations become indistinguishable from noisy fluctuations for σ > σ k (µ) 20-b

Main results Theorem 3: [B, Gentz, Kuehn 2010] For z 0, paths stay with high probability in covariance tubes For z = 0, section of tube is close to circular with radius µ 1/4 σ Distance between k th and k + 1 st canard e (2k+1)2 µ Theorem 4: [B, Gentz, Kuehn 2010] For z > 0, paths are likely to escape after time of order µ log σ 20-c

What s next? Estimate global return map for stochastic system Analyse possible mixed-mode patterns Possible scenario: metastable transitions between regular patterns Comparison with real data 21

What s next? Estimate global return map for stochastic system Analyse possible mixed-mode patterns Possible scenario: metastable transitions between regular patterns Comparison with real data Summary ISI distributions are not always exponential Transient effects are important (QSD, metastability) Precise sample path analysis is possible, useful tools exist (in some cases): singular perturbation theory, large deviations, martingales, substochastic Markov processes,... Still many open problems: other bifurcations, better approximation of QSD, higher dimensions, other types of noise,... 21-a

Further reading N.B. and Barbara Gentz, Noise-induced phenomena in slow-fast dynamical systems, A sample-paths approach, Springer, Probability and its Applications (2006) N.B. and Barbara Gentz, Stochastic dynamic bifurcations and excitability, in C. Laing and G. Lord, (Eds.), Stochastic methods in Neuroscience, p. 65-93, Oxford University Press (2009) N.B., Stochastic dynamical systems in neuroscience, Oberwolfach Reports 8:2290 2293 (2011) N.B., Barbara Gentz and Christian Kuehn, Hunting French Ducks in a Noisy Environment, J. Differential Equations 252:4786 4841 (2012) N.B. and Damien Landon, Mixed-mode oscillations and interspike interval statistics in the stochastic FitzHugh Nagumo model, Nonlinearity, at press (2012). arxiv:1105.1278 www.univ-orleans.fr/mapmo/membres/berglund 22

Additional material

Covariance tubes Linearized stochastic equation around a canard (x det, y det, z det dζ t = A(t)ζ t dt + σ dw t A(t) = t t ( 2x det t 1 (1+µ) 0 t ) t ) ζ t = U(t)ζ 0 + σ U(t, s) dw s (U(t, s) : principal solution of U = AU) 0 Gaussian process with covariance matrix Cov(ζ t ) = σ 2 V (t) V (t) = U(t)V (0)U(t) 1 + t 0 U(t, s)u(t, s)t ds 24

Covariance tubes Linearized stochastic equation around a canard (x det, y det, z det dζ t = A(t)ζ t dt + σ dw t A(t) = t t ( 2x det t 1 (1+µ) 0 t ) t ) ζ t = U(t)ζ 0 + σ U(t, s) dw s (U(t, s) : principal solution of U = AU) 0 Gaussian process with covariance matrix Cov(ζ t ) = σ 2 V (t) V (t) = U(t)V (0)U(t) 1 + Covariance tube : B(h) = { (x, y) (x det t t 0 U(t, s)u(t, s)t ds, yt det ), V (t) 1 [(x, y) (x det t, yt det )] < h 2} Theorem 3: [B, Gentz, Kuehn 2010] Probability of leaving covariance tube before time t (with z t 0) : P { τ B(h) < t } C(t) e κh2 /2σ 2 24-a

Covariance tubes Theorem 3: [B, Gentz, Kuehn 2010] Probability of leaving covariance tube before time t (with z t 0) : P { τ B(h) < t } C(t) e κh2 /2σ 2 Sketch of proof : (Sub)martingale : {M t } t 0, E{M t M s } = ( )M s for t s 0 { } Doob s submartingale inequality : P M t L 1 L E[M T ] sup 0 t T 25

Covariance tubes Theorem 3: [B, Gentz, Kuehn 2010] Probability of leaving covariance tube before time t (with z t 0) : P { τ B(h) < t } C(t) e κh2 /2σ 2 Sketch of proof : (Sub)martingale : {M t } t 0, E{M t M s } = ( )M s for t s 0 { } Doob s submartingale inequality : P M t L 1 L E[M T ] Linear equation : ζ t = σ t 0 sup 0 t T U(t, s) dw s is no martingale but can be approximated by martingale on small time intervals exp{γ ζ t, V (t) 1 ζ t } approximated by submartingale Doob s inequality yields bound on probability of leaving B(h) during small time intervals. Then sum over all time intervals 25-a

Covariance tubes Theorem 3: [B, Gentz, Kuehn 2010] Probability of leaving covariance tube before time t (with z t 0) : P { τ B(h) < t } C(t) e κh2 /2σ 2 Sketch of proof : (Sub)martingale : {M t } t 0, E{M t M s } = ( )M s for t s 0 { } Doob s submartingale inequality : P M t L 1 L E[M T ] Linear equation : ζ t = σ t 0 sup 0 t T U(t, s) dw s is no martingale but can be approximated by martingale on small time intervals exp{γ ζ t, V (t) 1 ζ t } approximated by submartingale Doob s inequality yields bound on probability of leaving B(h) during small time intervals. Then sum over all time intervals Nonlinear equation : dζ t = A(t)ζ t dt + b(ζ t, t) dt + σ dw t ζ t = σ t 0 U(t, s) dw s + t 0 U(t, s)b(ζ s, s) ds Second integral can be treated as small perturbation for t τ B(h) 25-b

Early transitions Let D be neighbourhood of size z of a canard for z > 0 (unstable) Theorem 4: [B, Gentz, Kuehn 2010] κ, C, γ 1, γ 2 > 0 such that for σ log σ γ 1 µ 3/4 probability of leaving D after z t = z satisfies Small for z Sketch of proof : P { z τd > z } C log σ γ 2 e κ(z2 µ)/(µ log σ ) µ log σ /κ Escape from neighbourhood of size σ log σ / z : compare with linearized equation on small time intervals + Markov property Escape from annulus σ log σ / z ζ z : use polar coordinates and averaging To combine the two regimes : use Laplace transforms 26