Toshali Mitra (Avtor), Sukrut Mondkar (Avtor), Ayan Mukhopadhyay (Avtor), Alexander Soloviev (Avtor)

Povzetek

Gubser flow is an evolution with cylindrical and boost symmetries, which can be best studied by mapping the future wedge of Minkowski space (R$^{3,1}$) to dS$_3$ × ℝ in a conformal relativistic theory. Here, we sharpen our previous analytic results and validate them via the first numerical exploration of the Gubser flow in a holographic conformal field theory. Remarkably, the leading generic behavior at large de Sitter time is free-streaming in transverse directions and the sub-leading behavior is that of a color glass condensate. We also show that Gubser flow can be smoothly glued to the vacuum outside the future Minkowski wedge generically given that the energy density vanishes faster than any power when extrapolated to early proper time or to large distances from the central axis. We find that at intermediate times the ratio of both the transverse and longitudinal pressures to the energy density converge approximately to a fixed point which is hydrodynamic only for large initial energy densities. We argue that our results suggest that the Gubser flow is better applied to collective behavior in jets rather than the full medium in the phenomenology of heavy ion collisions and can reveal new clues to the mechanism of confinement.

Ključne besede

relativistična hidrodinamika;Gubserjev tok;relativistic hydrodynamics;Gubser flow;

Podatki

Jezik: Angleški jezik
Leto izida:
Tipologija: 1.01 - Izvirni znanstveni članek
Organizacija: UL FMF - Fakulteta za matematiko in fiziko
UDK: 532.5
COBISS: 225221379 Povezava se bo odprla v novem oknu
ISSN: 1029-8479
Št. ogledov: 25
Št. prenosov: 6
Ocena: 0 (0 glasov)
Metapodatki: JSON JSON-RDF JSON-LD TURTLE N-TRIPLES XML RDFA MICRODATA DC-XML DC-RDF RDF

Ostali podatki

Sekundarni jezik: Slovenski jezik
Sekundarne ključne besede: relativistična hidrodinamika;Gubserjev tok;
Vrsta dela (COBISS): Članek v reviji
Strani: 58 str.
Letnik: ǂVol. ǂ2024
Zvezek: ǂart. no. ǂ226
Čas izdaje: Oct. 2024
DOI: 10.1007/JHEP10(2024)226
ID: 25847401