2021
DOI: 10.1140/epjb/s10051-021-00214-8
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Heat distribution of relativistic Brownian motion

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Cited by 8 publications
(18 citation statements)
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“…For equation (30), much like in the previous case, let us proceed in a term-by-term fashion. Firstly, the term…”
Section: Lorentz Covariancementioning
confidence: 99%
See 3 more Smart Citations
“…For equation (30), much like in the previous case, let us proceed in a term-by-term fashion. Firstly, the term…”
Section: Lorentz Covariancementioning
confidence: 99%
“…Thus, we showed that all terms appearing in equation ( 30) are Lorentz-covariant fourvectors. This allows us to rewrite our relativistic Langevin equation (30) in explicitly Lorentzcovariant form:…”
Section: Lorentz Covariancementioning
confidence: 99%
See 2 more Smart Citations
“…Other effects on the heat distribution for Brownian particles, e.g. nonlinear potentials [44][45][46], inertia [47][48][49][50][51], relativistic motion [52], and non-isothermal transformations [53], have also been addressed theoretically. Furthermore, heat fluctuations have been studied for active matter systems, such as active chains in viscous heat baths [54], Brownian particles embedded in active media [55,56], and activity-driven harmonic chains [57].…”
Section: Introductionmentioning
confidence: 99%