2019
DOI: 10.1007/s10714-019-2644-9
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Energy balance of a Bose gas in a curved space-time

Abstract: We derive a general energy balance equation for a self-interacting boson gas at vanishing temperature in a curved spacetime. This represents a first step towards a formulation of the first law of thermodynamics for a scalar field in general relativity. By using a 3 + 1 foliation of the spacetime and performing a Madelung transformation, we rewrite the Klein-Gordon-Maxwell equations in a general curved spacetime into its hydrodynamic version where we can identify the different energy contributions of the system… Show more

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Cited by 11 publications
(26 citation statements)
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“…The main difference between the hydrodynamic representation of bosons [1] [2] and fermions concerns the form of the Bernoulli equation. For bosons, after making the Madelung transformation, we can separate the KG equation into real and imaginary parts.…”
Section: Discussionmentioning
confidence: 99%
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“…The main difference between the hydrodynamic representation of bosons [1] [2] and fermions concerns the form of the Bernoulli equation. For bosons, after making the Madelung transformation, we can separate the KG equation into real and imaginary parts.…”
Section: Discussionmentioning
confidence: 99%
“…The problem of the Energy Balance for boson particles in a curved spacetime is studied in [1], where the conserved 4-current associated with the KG equation describing the evolution of a complex scalar field Φ(x µ ) is defined. We can generalize this idea by defining a new 4-current J KG µ , changing the scalar field by a spinor and the complex conjugate scalar field by the conjugate transpose of the spinor.…”
Section: Field Equationsmentioning
confidence: 99%
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