Modified inertial mass from information loss

A modification of inertia (called MiHsC or quantized inertia) has been proposed that assumes that inertia is caused by Unruh radiation, and that this radiation is made inhomogeneous in space by either Rindler horizons caused by acceleration or the distant Hubble horizon. The former predicts the stan...

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Detalles Bibliográficos
Autores: McCulloch, M. E., Giné, Jaume
Tipo de recurso: artículo
Estado:Versión enviada para evaluación y publicación
Fecha de publicación:2017
País:España
Institución:Universitat de Lleida (UdL)
Repositorio:Repositori Obert UdL
OAI Identifier:oai:repositori.udl.cat:10459.1/69875
Acceso en línea:https://doi.org/10.1142/S0217732317501486
http://hdl.handle.net/10459.1/69875
Access Level:acceso abierto
Palabra clave:Inertial mass
Unruh radiation
Information
Landauer’s principle
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spelling Modified inertial mass from information lossMcCulloch, M. E.Giné, JaumeInertial massUnruh radiationInformationLandauer’s principleA modification of inertia (called MiHsC or quantized inertia) has been proposed that assumes that inertia is caused by Unruh radiation, and that this radiation is made inhomogeneous in space by either Rindler horizons caused by acceleration or the distant Hubble horizon. The former predicts the standard inertial mass, and the latter predicts galaxy rotation without dark matter and cosmic acceleration without dark energy. It is proposed here that this model can be derived in an alternative way by assuming that the sum of mass (M), energy (E) and the information content of horizons (I) is conserved (EMI) so that mass–energy is released in a discrete manner when the area of a Rindler horizon reduces. This model could be tested by looking for the quantization of inertial mass and acceleration at very high accelerations, and may provide an explanation for the cosmological constant problem.The second author is partially supported by a MINECO/ FEDER grant number MTM2014-53703-P and an AGAUR (Generalitat de Catalunya) grant number 2014SGR 1204.World Scientific Publishing2017info:eu-repo/semantics/articleinfo:eu-repo/semantics/submittedVersionhttps://doi.org/10.1142/S0217732317501486http://hdl.handle.net/10459.1/69875reponame:Repositori Obert UdL instname:Universitat de Lleida (UdL)Inglésinfo:eu-repo/grantAgreement/MINECO//MTM2014-53703-PVersió preprint del document publicat a https://doi.org/10.1142/S0217732317501486Modern Physics Letters A, 2017, vol. 32, núm. 28, a1750148(c) World Scientific Publishing, 2017info:eu-repo/semantics/openAccessoai:repositori.udl.cat:10459.1/698752026-06-24T12:42:17Z
dc.title.none.fl_str_mv Modified inertial mass from information loss
title Modified inertial mass from information loss
spellingShingle Modified inertial mass from information loss
McCulloch, M. E.
Inertial mass
Unruh radiation
Information
Landauer’s principle
title_short Modified inertial mass from information loss
title_full Modified inertial mass from information loss
title_fullStr Modified inertial mass from information loss
title_full_unstemmed Modified inertial mass from information loss
title_sort Modified inertial mass from information loss
dc.creator.none.fl_str_mv McCulloch, M. E.
Giné, Jaume
author McCulloch, M. E.
author_facet McCulloch, M. E.
Giné, Jaume
author_role author
author2 Giné, Jaume
author2_role author
dc.subject.none.fl_str_mv Inertial mass
Unruh radiation
Information
Landauer’s principle
topic Inertial mass
Unruh radiation
Information
Landauer’s principle
description A modification of inertia (called MiHsC or quantized inertia) has been proposed that assumes that inertia is caused by Unruh radiation, and that this radiation is made inhomogeneous in space by either Rindler horizons caused by acceleration or the distant Hubble horizon. The former predicts the standard inertial mass, and the latter predicts galaxy rotation without dark matter and cosmic acceleration without dark energy. It is proposed here that this model can be derived in an alternative way by assuming that the sum of mass (M), energy (E) and the information content of horizons (I) is conserved (EMI) so that mass–energy is released in a discrete manner when the area of a Rindler horizon reduces. This model could be tested by looking for the quantization of inertial mass and acceleration at very high accelerations, and may provide an explanation for the cosmological constant problem.
publishDate 2017
dc.date.none.fl_str_mv 2017
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/submittedVersion
format article
status_str submittedVersion
dc.identifier.none.fl_str_mv https://doi.org/10.1142/S0217732317501486
http://hdl.handle.net/10459.1/69875
url https://doi.org/10.1142/S0217732317501486
http://hdl.handle.net/10459.1/69875
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv info:eu-repo/grantAgreement/MINECO//MTM2014-53703-P
Versió preprint del document publicat a https://doi.org/10.1142/S0217732317501486
Modern Physics Letters A, 2017, vol. 32, núm. 28, a1750148
dc.rights.none.fl_str_mv (c) World Scientific Publishing, 2017
info:eu-repo/semantics/openAccess
rights_invalid_str_mv (c) World Scientific Publishing, 2017
eu_rights_str_mv openAccess
dc.publisher.none.fl_str_mv World Scientific Publishing
publisher.none.fl_str_mv World Scientific Publishing
dc.source.none.fl_str_mv reponame:Repositori Obert UdL
instname:Universitat de Lleida (UdL)
instname_str Universitat de Lleida (UdL)
reponame_str Repositori Obert UdL
collection Repositori Obert UdL
repository.name.fl_str_mv
repository.mail.fl_str_mv
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