Guardado en:
Detalles Bibliográficos
Autores principales: Eissa, Nada, Ordóñez, Carlos R., Valdivia-Mera, Gustavo
Formato: Preprint
Publicado: 2025
Materias:
Acceso en línea:https://arxiv.org/abs/2508.16880
Etiquetas: Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
_version_ 1866909940895973376
author Eissa, Nada
Ordóñez, Carlos R.
Valdivia-Mera, Gustavo
author_facet Eissa, Nada
Ordóñez, Carlos R.
Valdivia-Mera, Gustavo
contents Inspired by the novel idea proposed by T.~Padmanabhan in \textit{Phys.\ Rev.\ D 100, 045024 (2019)}, we develop a method to uncover the hidden thermal properties of the inertial Feynman propagator in Minkowski spacetime in a causally consistent manner. This, in turn, enables a coherent interpretation based on future-directed propagation. In our approach, the Fourier transform is implemented following the convention used in the analysis of vacuum fluctuations. As a result, future-directed propagation across causal horizons can be consistently interpreted, from the perspective of an observer confined to a causally disconnected region, as the emission of scalar quanta at the past horizon and their absorption at the future horizon. Moreover, we find that the ratio between emission and absorption processes reproduces the characteristic Boltzmann factor of a thermal ensemble. We first apply this analysis to a causal diamond of length $2α$, performing a detailed study of the near-horizon geometry and thereby obtaining the temperature associated with the thermal behavior of the Minkowski vacuum as perceived by an observer with finite lifetime $2α$. For completeness, we also apply the method to the right Rindler wedge, recovering the well-known Unruh temperature, $T = a/(2π)$. Our results demonstrate that thermality can emerge directly from causal structure, independently of acceleration or gravity, with causal diamonds encoding intrinsic thermodynamic behavior in quantum field theory.
format Preprint
id arxiv_https___arxiv_org_abs_2508_16880
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Thermal nature of the causal diamond horizon: A hidden property of the inertial propagator
Eissa, Nada
Ordóñez, Carlos R.
Valdivia-Mera, Gustavo
High Energy Physics - Theory
General Relativity and Quantum Cosmology
Quantum Physics
Inspired by the novel idea proposed by T.~Padmanabhan in \textit{Phys.\ Rev.\ D 100, 045024 (2019)}, we develop a method to uncover the hidden thermal properties of the inertial Feynman propagator in Minkowski spacetime in a causally consistent manner. This, in turn, enables a coherent interpretation based on future-directed propagation. In our approach, the Fourier transform is implemented following the convention used in the analysis of vacuum fluctuations. As a result, future-directed propagation across causal horizons can be consistently interpreted, from the perspective of an observer confined to a causally disconnected region, as the emission of scalar quanta at the past horizon and their absorption at the future horizon. Moreover, we find that the ratio between emission and absorption processes reproduces the characteristic Boltzmann factor of a thermal ensemble. We first apply this analysis to a causal diamond of length $2α$, performing a detailed study of the near-horizon geometry and thereby obtaining the temperature associated with the thermal behavior of the Minkowski vacuum as perceived by an observer with finite lifetime $2α$. For completeness, we also apply the method to the right Rindler wedge, recovering the well-known Unruh temperature, $T = a/(2π)$. Our results demonstrate that thermality can emerge directly from causal structure, independently of acceleration or gravity, with causal diamonds encoding intrinsic thermodynamic behavior in quantum field theory.
title Thermal nature of the causal diamond horizon: A hidden property of the inertial propagator
topic High Energy Physics - Theory
General Relativity and Quantum Cosmology
Quantum Physics
url https://arxiv.org/abs/2508.16880