White dwarf constraints on a varying G
- Autores
- García Berro, E.; Torres, S.; Althaus, Leandro Gabriel; Corsico, Alejandro H.; Loren Aguilar, P.; Romero, A. D.; Isern, J.
- Año de publicación
- 2014
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- A secular variation of G modifies the structure and evolutionary time scales of white dwarfs. Using an state-of-the-art stellar evolutionary code, an up-to-date pulsational code, and a detailed population synthesis code we demonstrate that the effects of a running G are obvious both in the properties of individual white dwarfs, and in those of the white dwarf populations in clusters. Specifically, we show that the white dwarf evolutionary sequences depend on both the value of dot G/G, and on the value of G when the white dwarf was born. We show as well that the pulsational properties of variable white dwarfs can be used to constrain dot G/G. Finally, we also show that the ensemble properties of of white dwarfs in clusters can also be used to set upper bounds to dot G/G. Precisely, the tightest bound -- dot G/G ˜ -1.8 10-12 yr-1 -- is obtained studying the population of the old, metal-rich, well populated, open cluster NGC 6791. Less stringent upper limits can be obtained comparing the theoretical results obtained taking into account the effects of a running G with the measured rates of change of the periods of two well studied pulsating white dwarfs, G117-B15A and R548. Using these white dwarfs we obtain dot G/G˜ -1.8× 10-10 yr-1, and dot G/G˜ -1.3× 10-10 yr-1, respectively, which although less restrictive than the previous bound, can be improved measuring the rate of change of the period of massive white dwarfs.
Fil: García Berro, E.. Universidad Politecnica de Catalunya; España. Institute for Space Studies of Catalonia; España
Fil: Torres, S.. Universidad Politecnica de Catalunya; España. Institute for Space Studies of Catalonia; España
Fil: Althaus, Leandro Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Corsico, Alejandro H.. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina
Fil: Loren Aguilar, P.. University of Exeter. School of Physics; Reino Unido
Fil: Romero, A. D.. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Isern, J.. Institute for Space Studies of Catalonia; España. Institut de Ciències de l’Espai; España - Materia
-
White Dwarfs
Secular Variation - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/10920
Ver los metadatos del registro completo
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oai:ri.conicet.gov.ar:11336/10920 |
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3498 |
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CONICET Digital (CONICET) |
spelling |
White dwarf constraints on a varying GGarcía Berro, E.Torres, S.Althaus, Leandro GabrielCorsico, Alejandro H.Loren Aguilar, P.Romero, A. D.Isern, J.White DwarfsSecular Variationhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1A secular variation of G modifies the structure and evolutionary time scales of white dwarfs. Using an state-of-the-art stellar evolutionary code, an up-to-date pulsational code, and a detailed population synthesis code we demonstrate that the effects of a running G are obvious both in the properties of individual white dwarfs, and in those of the white dwarf populations in clusters. Specifically, we show that the white dwarf evolutionary sequences depend on both the value of dot G/G, and on the value of G when the white dwarf was born. We show as well that the pulsational properties of variable white dwarfs can be used to constrain dot G/G. Finally, we also show that the ensemble properties of of white dwarfs in clusters can also be used to set upper bounds to dot G/G. Precisely, the tightest bound -- dot G/G ˜ -1.8 10-12 yr-1 -- is obtained studying the population of the old, metal-rich, well populated, open cluster NGC 6791. Less stringent upper limits can be obtained comparing the theoretical results obtained taking into account the effects of a running G with the measured rates of change of the periods of two well studied pulsating white dwarfs, G117-B15A and R548. Using these white dwarfs we obtain dot G/G˜ -1.8× 10-10 yr-1, and dot G/G˜ -1.3× 10-10 yr-1, respectively, which although less restrictive than the previous bound, can be improved measuring the rate of change of the period of massive white dwarfs.Fil: García Berro, E.. Universidad Politecnica de Catalunya; España. Institute for Space Studies of Catalonia; EspañaFil: Torres, S.. Universidad Politecnica de Catalunya; España. Institute for Space Studies of Catalonia; EspañaFil: Althaus, Leandro Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Corsico, Alejandro H.. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; ArgentinaFil: Loren Aguilar, P.. University of Exeter. School of Physics; Reino UnidoFil: Romero, A. D.. Universidade Federal do Rio Grande do Sul; BrasilFil: Isern, J.. Institute for Space Studies of Catalonia; España. Institut de Ciències de l’Espai; EspañaIstituto Nazionale di Astrofisica2014-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/10920García Berro, E.; Torres, S.; Althaus, Leandro Gabriel; Corsico, Alejandro H.; Loren Aguilar, P.; et al.; White dwarf constraints on a varying G; Istituto Nazionale di Astrofisica; Memorie della Societa Astronomica Italiana; 85; 1-2014; 118-1231824-016Xenginfo:eu-repo/semantics/altIdentifier/url/http://sait.oat.ts.astro.it/MmSAI/85/PDF/118.pdfinfo:eu-repo/semantics/altIdentifier/url/http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1308.5414info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:42:01Zoai:ri.conicet.gov.ar:11336/10920instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 09:42:01.678CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
White dwarf constraints on a varying G |
title |
White dwarf constraints on a varying G |
spellingShingle |
White dwarf constraints on a varying G García Berro, E. White Dwarfs Secular Variation |
title_short |
White dwarf constraints on a varying G |
title_full |
White dwarf constraints on a varying G |
title_fullStr |
White dwarf constraints on a varying G |
title_full_unstemmed |
White dwarf constraints on a varying G |
title_sort |
White dwarf constraints on a varying G |
dc.creator.none.fl_str_mv |
García Berro, E. Torres, S. Althaus, Leandro Gabriel Corsico, Alejandro H. Loren Aguilar, P. Romero, A. D. Isern, J. |
author |
García Berro, E. |
author_facet |
García Berro, E. Torres, S. Althaus, Leandro Gabriel Corsico, Alejandro H. Loren Aguilar, P. Romero, A. D. Isern, J. |
author_role |
author |
author2 |
Torres, S. Althaus, Leandro Gabriel Corsico, Alejandro H. Loren Aguilar, P. Romero, A. D. Isern, J. |
author2_role |
author author author author author author |
dc.subject.none.fl_str_mv |
White Dwarfs Secular Variation |
topic |
White Dwarfs Secular Variation |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
A secular variation of G modifies the structure and evolutionary time scales of white dwarfs. Using an state-of-the-art stellar evolutionary code, an up-to-date pulsational code, and a detailed population synthesis code we demonstrate that the effects of a running G are obvious both in the properties of individual white dwarfs, and in those of the white dwarf populations in clusters. Specifically, we show that the white dwarf evolutionary sequences depend on both the value of dot G/G, and on the value of G when the white dwarf was born. We show as well that the pulsational properties of variable white dwarfs can be used to constrain dot G/G. Finally, we also show that the ensemble properties of of white dwarfs in clusters can also be used to set upper bounds to dot G/G. Precisely, the tightest bound -- dot G/G ˜ -1.8 10-12 yr-1 -- is obtained studying the population of the old, metal-rich, well populated, open cluster NGC 6791. Less stringent upper limits can be obtained comparing the theoretical results obtained taking into account the effects of a running G with the measured rates of change of the periods of two well studied pulsating white dwarfs, G117-B15A and R548. Using these white dwarfs we obtain dot G/G˜ -1.8× 10-10 yr-1, and dot G/G˜ -1.3× 10-10 yr-1, respectively, which although less restrictive than the previous bound, can be improved measuring the rate of change of the period of massive white dwarfs. Fil: García Berro, E.. Universidad Politecnica de Catalunya; España. Institute for Space Studies of Catalonia; España Fil: Torres, S.. Universidad Politecnica de Catalunya; España. Institute for Space Studies of Catalonia; España Fil: Althaus, Leandro Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Corsico, Alejandro H.. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina Fil: Loren Aguilar, P.. University of Exeter. School of Physics; Reino Unido Fil: Romero, A. D.. Universidade Federal do Rio Grande do Sul; Brasil Fil: Isern, J.. Institute for Space Studies of Catalonia; España. Institut de Ciències de l’Espai; España |
description |
A secular variation of G modifies the structure and evolutionary time scales of white dwarfs. Using an state-of-the-art stellar evolutionary code, an up-to-date pulsational code, and a detailed population synthesis code we demonstrate that the effects of a running G are obvious both in the properties of individual white dwarfs, and in those of the white dwarf populations in clusters. Specifically, we show that the white dwarf evolutionary sequences depend on both the value of dot G/G, and on the value of G when the white dwarf was born. We show as well that the pulsational properties of variable white dwarfs can be used to constrain dot G/G. Finally, we also show that the ensemble properties of of white dwarfs in clusters can also be used to set upper bounds to dot G/G. Precisely, the tightest bound -- dot G/G ˜ -1.8 10-12 yr-1 -- is obtained studying the population of the old, metal-rich, well populated, open cluster NGC 6791. Less stringent upper limits can be obtained comparing the theoretical results obtained taking into account the effects of a running G with the measured rates of change of the periods of two well studied pulsating white dwarfs, G117-B15A and R548. Using these white dwarfs we obtain dot G/G˜ -1.8× 10-10 yr-1, and dot G/G˜ -1.3× 10-10 yr-1, respectively, which although less restrictive than the previous bound, can be improved measuring the rate of change of the period of massive white dwarfs. |
publishDate |
2014 |
dc.date.none.fl_str_mv |
2014-01 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/10920 García Berro, E.; Torres, S.; Althaus, Leandro Gabriel; Corsico, Alejandro H.; Loren Aguilar, P.; et al.; White dwarf constraints on a varying G; Istituto Nazionale di Astrofisica; Memorie della Societa Astronomica Italiana; 85; 1-2014; 118-123 1824-016X |
url |
http://hdl.handle.net/11336/10920 |
identifier_str_mv |
García Berro, E.; Torres, S.; Althaus, Leandro Gabriel; Corsico, Alejandro H.; Loren Aguilar, P.; et al.; White dwarf constraints on a varying G; Istituto Nazionale di Astrofisica; Memorie della Societa Astronomica Italiana; 85; 1-2014; 118-123 1824-016X |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/http://sait.oat.ts.astro.it/MmSAI/85/PDF/118.pdf info:eu-repo/semantics/altIdentifier/url/http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1308.5414 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
Istituto Nazionale di Astrofisica |
publisher.none.fl_str_mv |
Istituto Nazionale di Astrofisica |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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1844613324700909568 |
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13.070432 |