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Hydrodynamization in hybrid Bjorken flow attractors
ID
Mitra, Toshali
(
Avtor
),
ID
Mondkar, Sukrut
(
Avtor
),
ID
Mukhopadhyay, Ayan
(
Avtor
),
ID
Rebhan, Anton
(
Avtor
),
ID
Soloviev, Alexander
(
Avtor
)
PDF - Predstavitvena datoteka,
prenos
(1,90 MB)
MD5: 513E90EE21BFD2F118A3F83683C33069
PDF - Predstavitvena datoteka,
prenos
(1,90 MB)
MD5: 513E90EE21BFD2F118A3F83683C33069
Galerija slik
Izvleček
Hybrid fluid models, consisting of two sectors with more weakly and more strongly self-interacting degrees of freedom coupled consistently as in the semi-holographic framework, have been shown to exhibit an attractor surface for Bjorken flow. Retaining only the simple viscid fluid descriptions of both sectors, we find that, on the attractor surface, the hydrodynamization times of both subsectors decrease with increasing total energy density at the respective point of hydrodynamization following a conformal scaling, reach their minimum values, and subsequently rise rapidly. The minimum values are obtained when the respective energy densities are of the order of the inverse of the dimensionful inter-system coupling. Restricting to attractor curves which can be matched to glasma models at a time set by the saturation scale for both p-p and Pb-Pb collisions, we find that the more weakly coupled sector hydrodynamizes much later, and the strongly coupled sector hydrodynamizes earlier in p-p collisions, since the total energy densities at the respective hydrodynamization times of these sectors fall inside and outside of the conformal window. This holds true also for phenomenologically relevant solutions that are significantly away from the attractor surface at the time we match to glasma models.
Jezik:
Angleški jezik
Ključne besede:
relativistic hydrodynamics
,
field theory hydrodynamics
,
non-equilibrium field theory
,
Quark-Gluon plasma
Vrsta gradiva:
Članek v reviji
Tipologija:
1.01 - Izvirni znanstveni članek
Organizacija:
FMF - Fakulteta za matematiko in fiziko
Status publikacije:
Objavljeno
Različica publikacije:
Objavljena publikacija
Datum objave:
01.04.2024
Leto izida:
2024
Št. strani:
47 str.
Številčenje:
Vol. 2024, art. no. ǂ41
PID:
20.500.12556/RUL-169020
UDK:
532.5
ISSN pri članku:
1029-8479
DOI:
10.1007/JHEP04(2024)041
COBISS.SI-ID:
235095043
Datum objave v RUL:
07.05.2025
Število ogledov:
292
Število prenosov:
116
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Objavi na:
Gradivo je del revije
Naslov:
The journal of high energy physics
Skrajšan naslov:
J. high energy phys.
Založnik:
SISSA
ISSN:
1029-8479
COBISS.SI-ID:
1314148
Licence
Licenca:
CC BY 4.0, Creative Commons Priznanje avtorstva 4.0 Mednarodna
Povezava:
http://creativecommons.org/licenses/by/4.0/deed.sl
Opis:
To je standardna licenca Creative Commons, ki daje uporabnikom največ možnosti za nadaljnjo uporabo dela, pri čemer morajo navesti avtorja.
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