Unruh Effect for Mixed Neutrinos and the KMS Condition
The quantization of mixed (neutrino) fields in an accelerated background reveals a non-thermal nature for Unruh radiation, which can be fitted by a Tsallis-like distribution function. However, for relativistic flavor neutrinos, which are represented by the standard Pontecorvo states, such a correcti...
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MDPI AG
2022-05-01
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Online Access: | https://www.mdpi.com/2218-1997/8/6/306 |
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author | Massimo Blasone Gaetano Lambiase Giuseppe Gaetano Luciano Luciano Petruzziello |
author_facet | Massimo Blasone Gaetano Lambiase Giuseppe Gaetano Luciano Luciano Petruzziello |
author_sort | Massimo Blasone |
collection | DOAJ |
description | The quantization of mixed (neutrino) fields in an accelerated background reveals a non-thermal nature for Unruh radiation, which can be fitted by a Tsallis-like distribution function. However, for relativistic flavor neutrinos, which are represented by the standard Pontecorvo states, such a correction turns out to be negligible and thermality is restored. We show that the usage of Pontecorvo states for the calculation of the decay rate of an accelerated proton in the laboratory and comoving frames leads to consistent results and correctly implements the KMS thermal condition. Thus, the employment of these states in the above framework is not at odds with the principle of general covariance, in contrast to recent claims in the literature. |
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format | Article |
id | doaj.art-c37a8acaee02402cae4d60bc36f614dd |
institution | Directory Open Access Journal |
issn | 2218-1997 |
language | English |
last_indexed | 2024-03-09T22:18:32Z |
publishDate | 2022-05-01 |
publisher | MDPI AG |
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series | Universe |
spelling | doaj.art-c37a8acaee02402cae4d60bc36f614dd2023-11-23T19:19:01ZengMDPI AGUniverse2218-19972022-05-018630610.3390/universe8060306Unruh Effect for Mixed Neutrinos and the KMS ConditionMassimo Blasone0Gaetano Lambiase1Giuseppe Gaetano Luciano2Luciano Petruzziello3Dipartimento di Fisica, Università di Salerno, Via Giovanni Paolo II, 132 I-84084 Fisciano, Salerno, ItalyDipartimento di Fisica, Università di Salerno, Via Giovanni Paolo II, 132 I-84084 Fisciano, Salerno, ItalyDipartimento di Fisica, Università di Salerno, Via Giovanni Paolo II, 132 I-84084 Fisciano, Salerno, ItalyIstituto Nazionale di Fisica Nucleare, Sezione di Napoli, Gruppo Collegato di Salerno, Via Giovanni Paolo II, 132 I-84084 Fisciano, Salerno, ItalyThe quantization of mixed (neutrino) fields in an accelerated background reveals a non-thermal nature for Unruh radiation, which can be fitted by a Tsallis-like distribution function. However, for relativistic flavor neutrinos, which are represented by the standard Pontecorvo states, such a correction turns out to be negligible and thermality is restored. We show that the usage of Pontecorvo states for the calculation of the decay rate of an accelerated proton in the laboratory and comoving frames leads to consistent results and correctly implements the KMS thermal condition. Thus, the employment of these states in the above framework is not at odds with the principle of general covariance, in contrast to recent claims in the literature.https://www.mdpi.com/2218-1997/8/6/306neutrino mixingweak interactionsUnruh effectnon-extensive Tsallis statisticsquantum gravity |
spellingShingle | Massimo Blasone Gaetano Lambiase Giuseppe Gaetano Luciano Luciano Petruzziello Unruh Effect for Mixed Neutrinos and the KMS Condition Universe neutrino mixing weak interactions Unruh effect non-extensive Tsallis statistics quantum gravity |
title | Unruh Effect for Mixed Neutrinos and the KMS Condition |
title_full | Unruh Effect for Mixed Neutrinos and the KMS Condition |
title_fullStr | Unruh Effect for Mixed Neutrinos and the KMS Condition |
title_full_unstemmed | Unruh Effect for Mixed Neutrinos and the KMS Condition |
title_short | Unruh Effect for Mixed Neutrinos and the KMS Condition |
title_sort | unruh effect for mixed neutrinos and the kms condition |
topic | neutrino mixing weak interactions Unruh effect non-extensive Tsallis statistics quantum gravity |
url | https://www.mdpi.com/2218-1997/8/6/306 |
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