Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100310954> ?p ?o ?g. }
- W3100310954 abstract "We study correlations, transport, and chaos in a Heisenberg magnet as a classical model many-body system. By varying temperature and dimensionality, we can tune between settings with and without symmetry breaking and accompanying collective modes or quasiparticles (spin waves) which in the limit of low temperatures become increasingly long-lived. Changing the sign of the exchange interaction from a ferro- to an antiferromagnetic one varies the spin-wave spectrum, and hence the low-energy spectral density. We analyze both conventional and out-of-time-ordered spin correlators (decorrelators) to track the spreading of a spatiotemporally localized perturbation---the wing beat of the butterfly---as well as transport coefficients and Lyapunov exponents. We identify a number of qualitatively different regimes. Trivially, at $T=0$, there is no dynamics at all. In the limit of low temperature, $T={0}^{+}$, integrability emerges, with infinitely long-lived magnons; here the wave packet created by the perturbation propagates ballistically, yielding a light cone at the spin-wave velocity which thus subsumes the butterfly velocity; inside the light cone, a pattern characteristic of the free spin-wave spectrum is visible at short times. On top of this, residual interactions (nonlinearities in the equations of motion) lead to spin-wave lifetimes which, while divergent in this limit, remain finite at any nonzero $T$. At the longest times, this leads to a standard chaotic regime; for this regime, we show that the Lyapunov exponent is simply proportional to the (inverse) spin-wave lifetime. Visibly strikingly, between this and the short-time integrable regimes, a scarred regime emerges: Here, the decorrelator is spatiotemporally highly nonuniform, being dominated by rare and random scattering events seeding secondary light cones. As the spin correlation length decreases with increasing $T$, the distinction between these regimes disappears and at high temperature the previously studied chaotic paramagnetic regime emerges. For this, we elucidate how, somewhat counterintuitively, the ballistic butterfly velocity arises from a diffusive spin dynamics." @default.
- W3100310954 created "2020-11-23" @default.
- W3100310954 creator A5043804822 @default.
- W3100310954 creator A5048643855 @default.
- W3100310954 creator A5077211376 @default.
- W3100310954 date "2021-05-07" @default.
- W3100310954 modified "2023-10-18" @default.
- W3100310954 title "Classical many-body chaos with and without quasiparticles" @default.
- W3100310954 cites W1574188317 @default.
- W3100310954 cites W1583746591 @default.
- W3100310954 cites W1603380880 @default.
- W3100310954 cites W1969400766 @default.
- W3100310954 cites W1970929911 @default.
- W3100310954 cites W1971185946 @default.
- W3100310954 cites W1973736387 @default.
- W3100310954 cites W1980514318 @default.
- W3100310954 cites W1990932576 @default.
- W3100310954 cites W1995489344 @default.
- W3100310954 cites W1998459108 @default.
- W3100310954 cites W2000232635 @default.
- W3100310954 cites W2006925969 @default.
- W3100310954 cites W2007656106 @default.
- W3100310954 cites W2008317504 @default.
- W3100310954 cites W2016488536 @default.
- W3100310954 cites W2024295583 @default.
- W3100310954 cites W2027714081 @default.
- W3100310954 cites W2028157391 @default.
- W3100310954 cites W2038591556 @default.
- W3100310954 cites W2054880184 @default.
- W3100310954 cites W2055714762 @default.
- W3100310954 cites W2056511881 @default.
- W3100310954 cites W2068561656 @default.
- W3100310954 cites W2079405992 @default.
- W3100310954 cites W2080086907 @default.
- W3100310954 cites W2089191553 @default.
- W3100310954 cites W2090703333 @default.
- W3100310954 cites W2118301480 @default.
- W3100310954 cites W2122639408 @default.
- W3100310954 cites W2157236990 @default.
- W3100310954 cites W2164161378 @default.
- W3100310954 cites W2201348740 @default.
- W3100310954 cites W2262619112 @default.
- W3100310954 cites W2282168229 @default.
- W3100310954 cites W2485554649 @default.
- W3100310954 cites W2522882285 @default.
- W3100310954 cites W2560130063 @default.
- W3100310954 cites W2582585316 @default.
- W3100310954 cites W2585766751 @default.
- W3100310954 cites W2587983218 @default.
- W3100310954 cites W2611206484 @default.
- W3100310954 cites W2618465568 @default.
- W3100310954 cites W2620407091 @default.
- W3100310954 cites W2620844540 @default.
- W3100310954 cites W2738879091 @default.
- W3100310954 cites W2766333524 @default.
- W3100310954 cites W2770030665 @default.
- W3100310954 cites W2782099770 @default.
- W3100310954 cites W2790085823 @default.
- W3100310954 cites W2805957242 @default.
- W3100310954 cites W2886992082 @default.
- W3100310954 cites W2980717710 @default.
- W3100310954 cites W3000019265 @default.
- W3100310954 cites W3033736351 @default.
- W3100310954 cites W3037042650 @default.
- W3100310954 cites W3037318174 @default.
- W3100310954 cites W3092798498 @default.
- W3100310954 cites W3099348199 @default.
- W3100310954 cites W3100755341 @default.
- W3100310954 cites W3101241776 @default.
- W3100310954 cites W3101645585 @default.
- W3100310954 cites W3101666819 @default.
- W3100310954 cites W3102136626 @default.
- W3100310954 cites W3102391734 @default.
- W3100310954 cites W3103634851 @default.
- W3100310954 cites W3121590353 @default.
- W3100310954 cites W3121608281 @default.
- W3100310954 doi "https://doi.org/10.1103/physrevb.103.174302" @default.
- W3100310954 hasPublicationYear "2021" @default.
- W3100310954 type Work @default.
- W3100310954 sameAs 3100310954 @default.
- W3100310954 citedByCount "13" @default.
- W3100310954 countsByYear W31003109542020 @default.
- W3100310954 countsByYear W31003109542021 @default.
- W3100310954 countsByYear W31003109542022 @default.
- W3100310954 countsByYear W31003109542023 @default.
- W3100310954 crossrefType "journal-article" @default.
- W3100310954 hasAuthorship W3100310954A5043804822 @default.
- W3100310954 hasAuthorship W3100310954A5048643855 @default.
- W3100310954 hasAuthorship W3100310954A5077211376 @default.
- W3100310954 hasBestOaLocation W31003109541 @default.
- W3100310954 hasConcept C121332964 @default.
- W3100310954 hasConcept C136479403 @default.
- W3100310954 hasConcept C158622935 @default.
- W3100310954 hasConcept C191544260 @default.
- W3100310954 hasConcept C197067312 @default.
- W3100310954 hasConcept C204382992 @default.
- W3100310954 hasConcept C26873012 @default.
- W3100310954 hasConcept C3079626 @default.
- W3100310954 hasConcept C44221107 @default.
- W3100310954 hasConcept C54101563 @default.