Transition in the Equilibrium Distribution Function of Relativistic Particles

Verfasser / Beitragende:
[Miller Mendoza, Nuno A.M. Araújo, Sauro Succi, Hans J. Herrmann]
Ort, Verlag, Jahr:
2012
Enthalten in:
Scientific Reports, 2, p. 611
Format:
Artikel (online)
ID: 528785559
LEADER caa a22 4500
001 528785559
005 20181217030312.0
007 cr unu---uuuuu
008 180924e201208 xx s 000 0 eng
024 7 0 |a 10.3929/ethz-b-000055258  |2 doi 
024 7 0 |a 10.1038/srep00611  |2 doi 
035 |a (ETHRESEARCH)oai:www.research-collecti.ethz.ch:20.500.11850/55258 
245 0 0 |a Transition in the Equilibrium Distribution Function of Relativistic Particles  |h [Elektronische Daten]  |c [Miller Mendoza, Nuno A.M. Araújo, Sauro Succi, Hans J. Herrmann] 
246 0 |a Sci Rep 
506 |a Open access  |2 ethresearch 
520 3 |a We analyze a transition from single peaked to bimodal velocity distribution in a relativistic fluid under increasing temperature, in contrast with a non-relativistic gas, where only a monotonic broadening of the bell-shaped distribution is observed. Such transition results from the interplay between the raise in thermal energy and the constraint of maximum velocity imposed by the speed of light. We study the Bose-Einstein, the Fermi-Dirac, and the Maxwell-Jüttner distributions, and show that they all exhibit the same qualitative behavior. We characterize the nature of the transition in the framework of critical phenomena and show that it is either continuous or discontinuous, depending on the group velocity. We analyze the transition in one, two, and three dimensions, with special emphasis on twodimensions, for which a possible experiment in graphene, based on the measurement of the Johnson-Nyquist noise, is proposed. 
540 |a Creative Commons Attribution-NonCommercial-NoDerivs 3.0 Unported  |u http://creativecommons.org/licenses/by-nc-nd/3.0  |2 ethresearch 
690 7 |a Statistical physics, thermodynamics and nonlinear dynamics  |2 ethresearch 
690 7 |a Plasma physics  |2 ethresearch 
690 7 |a Carbon nanotubes and fullerenes  |2 ethresearch 
690 7 |a Astronomy and astrophysics  |2 ethresearch 
700 1 |a Mendoza  |D Miller  |e joint author 
700 1 |a Araújo  |D Nuno A.M.  |e joint author 
700 1 |a Succi  |D Sauro  |e joint author 
700 1 |a Herrmann  |D Hans J.  |e joint author 
773 0 |t Scientific Reports  |d London : Nature Publishing Group  |g 2, p. 611  |x 2045-2322 
856 4 0 |u http://hdl.handle.net/20.500.11850/55258  |q text/html  |z WWW-Backlink auf das Repository (Open access) 
908 |D 1  |a Journal Article  |2 ethresearch 
950 |B ETHRESEARCH  |P 856  |E 40  |u http://hdl.handle.net/20.500.11850/55258  |q text/html  |z WWW-Backlink auf das Repository (Open access) 
950 |B ETHRESEARCH  |P 700  |E 1-  |a Mendoza  |D Miller  |e joint author 
950 |B ETHRESEARCH  |P 700  |E 1-  |a Araújo  |D Nuno A.M.  |e joint author 
950 |B ETHRESEARCH  |P 700  |E 1-  |a Succi  |D Sauro  |e joint author 
950 |B ETHRESEARCH  |P 700  |E 1-  |a Herrmann  |D Hans J.  |e joint author 
950 |B ETHRESEARCH  |P 773  |E 0-  |t Scientific Reports  |d London : Nature Publishing Group  |g 2, p. 611  |x 2045-2322 
898 |a BK010053  |b XK010053  |c XK010000 
949 |B ETHRESEARCH  |F ETHRESEARCH  |b ETHRESEARCH  |j Journal Article  |c Open access