Quantum fluctuations of energy in subsystems of a hot relativistic gas

dc.contributor.authorDas, Arpan
dc.date.accessioned2025-11-27T09:08:11Z
dc.date.available2025-11-27T09:08:11Z
dc.date.issued2020-12
dc.description.abstractWe derive a formula that defines quantum fluctuations of energy in subsystems of a hot relativistic gas. For small subsystem sizes we find substantial increase of fluctuations compared to those known from standard thermodynamic considerations. However, if the size of the subsystem is sufficiently large, we reproduce the result for energy fluctuations in the canonical ensemble. Our results are subsequently used in the context of relativistic heavy-ion collisions to introduce limitations of the concepts such as classical energy density or fluid element. In the straightforward way, our formula can be applied in other fields of physics, wherever one deals with hot and relativistic matter.en_US
dc.identifier.urihttps://arxiv.org/abs/2012.05662
dc.identifier.urihttp://dspace.bits-pilani.ac.in:8080/jspui/handle/123456789/20249
dc.language.isoenen_US
dc.subjectPhysicsen_US
dc.subjectQuantum energy fluctuationsen_US
dc.subjectSmall subsystem limiten_US
dc.subjectCanonical ensemble recoveryen_US
dc.subjectHeavy-ion collision applicationsen_US
dc.titleQuantum fluctuations of energy in subsystems of a hot relativistic gasen_US
dc.typePreprinten_US

Files