• No results found

wake cycle

600

The results reported in the previous sections show a remarkable coexistence of

scale-601

invariant power-law structure for the durations of θ-bursts and a Weibull functional

602

form with a characteristic time scale for δ-burst durations (Figs. 2,3). This evidence

603

draws a strong parallel with far-from-equilibrium phenomena that are characterized

604

by bursting dynamics and abrupt transitions between active and quiet states, such

605

as avalanches and earthquakes (Munoz, 2018; Corral, 2004; Boffetta et al., 1999;

606

Paczuski et al., 2005). For instance, the intensity of avalanches and earthquakes

(ac-607

tive states) is also described by power-law distributions, while time intervals between

608

consecutive avalanches/earthquakes (quiet states) follow a generalized Gamma

distri-609

bution with a characteristic time scale (exponential tail). In this context Gamma is a

610

universal scaling function that is independent of spatial scales and minimum

magni-611

tude thresholds, and is consistently observed for a broad range of conditions despite

612

the large variability associated with phenomena such as avalanches and earthquakes

613

(Corral, 2004; Ribeiro et al., 2010; de Arcangelis et al., 2016).

614

In sleep dynamics, wake and brief arousals during sleep can be considered as

615

active states that, in rodents, are characterized by bursts in θ rhythms. Hence, we

616

hypothesize that a hierarchical structure, invariant across time scales, may underlie

617

the occurrence of θ-bursts, in analogy with non-equilibrium critical phenomena, and

618

investigate the relationship between the duration of θ-bursts and their temporal

619

occurrence (Fig. 10). To this end, we consider the time sequence of θ-bursts, and

620

we study the statistical features of the quiet times Δt separating consecutive bursts,

621

taking into account the duration dθ of each θ-burst (Fig. 10a). Since θ-bursts vary

622

in duration, we impose a threshold D0 representing the time scale of analysis, and

623

we define the quiet time Δtias the period from the end of θi-burst to the beginning

624

θi+1-burst. Thus, the statistical characteristics of Δtidepend on the threshold value

625

D0. We then obtain the probability distribution P (Δt; D0) of quiet times Δti for

626

different values of D0 (insets in Fig. 6c,d). With increasing threshold (scale of

627

observation) D0, the probability of longer Δti increases, while the probability of

628

short Δti decreases, leading to different curves for the distributions P (Δt; D0).

629

Visual inspection of the complex profile formed by the time sequence of θ-bursts

630

and their respective durations shows an apparent similarity when comparing short

631

segments of the profile with the entire sequence above a given threshold D0 (Fig.

632

6b). Presence of statistical self-similarity, observed after effective coarse-graining of

633

the profile, indicates a hierarchical structure across time scales D0 that

character-634

izes θ-bursts occurrence times and durations, and the associated quiet times. To

635

demonstrate statistical self-similarity in the quiet times, we systematically analyze

636

the functional form of the probability distributions P (Δt; D0) for different thresholds

637

D0 by rescaling each distribution by the average quiet timeΔtD0. Remarkably, we

638

find that all distribution curves collapse onto a single function G (Fig. 6c,d), defined

639

by the following scaling relation

640

P (Δt) =Δt−1· G(Δt/Δt). (10)

The scaling relation in Eq. 10 represents a mathematical expression of the statistical

641

self-similarity in the profile formed by the quiet times and θ-burst durations shown

642

in Fig. 6b. We find that the scaling function G(Δt/Δt) is well described by the

643

generalized Gamma distribution G(Δt/Δt; b, ν, p) =

644

p/bν(Δt/Δt)ν−1e−(Δt/bΔt)p/Γ(ν/p) (Stacy et al., 1962), where in our analysis Δt/Δt

645

is a dimensionless quiet time. The Gamma functional form is homogeneous (Ivanov et al.,

646

1996), i.e. rescaling the variable leaves the functional form unchanged. Such scaling

647

function indicates a hierarchical structure in the quiet times between consecutive

θ-648

bursts, independent of the scale of observation D0. In the limit of D0= 0, the quiet

649

time distribution P (Δt; D0) coincides with the distribution of δ-burst durations Pδ

650

(Figs. 2b and 3b,d) — a Weibull functional form that belongs to the same class of

651

homogeneous functions as the generalized Gamma.

652

Our analysis shows that the scaling relation in Eq. 10 and the associated Gamma

653

functional form for the quiet times are robust: (i) we find them in the 24 h period

654

(Fig. 10) as well as separately during light and dark periods, and (ii) they do not

655

significantly change with lesion in the VLPO (compare Fig. 10c and Fig. 10d).

656

Further, the presence of such hierarchical structure in quiet times indicates specific

657

temporal order in the occurrence of θ-bursts. To explicitly verify this, we randomly

658

reshuffle the sequence of θ-burst durations, while preserving the δ-burst durations

659

corresponding to quiet times at D0= 0, and we perform the analysis on the reshuffled

660

sequence to obtain quiet time distributions Prand(Δt; D0) for different thresholds D0.

661

In this case, after rescaling the distributions Prand(Δt; D0) by the average quiet

662

time ΔtD0, their curves collapse onto an exponential distribution (dashed lines in

663

Fig. 10c,d) — a hallmark of temporal independence between consecutive events

664

(Daley and Vere-Jones, 1988). This clearly demonstrates that temporal correlations

665

are intimately related to the existence of non-exponential scaling functions (Eq. 10)

666

(Corral, 2004; Daley and Vere-Jones, 1988).

667

Notably, a similar temporal organization characterized by coexistence of

power-668

law and generalized Gamma distribution has been reported for active states and quiet

669

times in a range of non-equilibrium systems self-tuning at criticality (earthquakes,

670

avalanches) (Munoz, 2018; Pruessner, 2012; Corral, 2004). Thus, our findings of

671

power-law distribution for θ-burst durations (Figs. 2,3) combined with a generalized

672

Gamma distribution for the quiet times between consecutive θ-bursts at different

673

scales of observation D0(Fig. 10) are a strong evidence in support of our hypothesis

674

that bursting activity of fundamental brain rhythms and the associated sleep

micro-675

architecture exhibit critical non-equilibrium behavior.

676

3.5 Long-range power-law correlations in the durations of θ

677

Related documents