The Newton constant and gravitational waves in some vector field adjusting mechanisms
- Autores
- Santillán, Osvaldo Pablo; Scornavacche, Marina Andrea
- Año de publicación
- 2017
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- At the present, there exist some Lorentz breaking scenarios which explain the smallness of the cosmological constant at the present era [1]-[2]. An important aspect to analyze is the propagation of gravitational waves and the screening or enhancement of the Newton constant G N in these models. The problem is that the Lorentz symmetry breaking terms may induce an unacceptable value of the Newton constant G N or introduce longitudinal modes in the gravitational wave propagation. Furthermore this breaking may spoil the standard dispersion relation ω=ck. In [3] the authors have presented a model suggesting that the behavior of the gravitational constant is correct for asymptotic times. In the present work, an explicit checking is made and we finally agree with these claims. Furthermore, it is suggested that the gravitational waves are also well behaved for large times. In the process, some new models with the same behavior are obtained, thus enlarging the list of possible adjustment mechanisms.
Fil: Santillán, Osvaldo Pablo. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Investigaciones Matemáticas "Luis A. Santaló". Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Investigaciones Matemáticas "Luis A. Santaló"; Argentina
Fil: Scornavacche, Marina Andrea. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina - Materia
-
COSMOLOGICAL PERTURBATION THEORY
DARK ENERGY THEORY
GRAVITATIONAL WAVES / THEORY - 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:11336/212524
Ver los metadatos del registro completo
id |
CONICETDig_a56ea8b4103d89cc316e89756af0f33c |
---|---|
oai_identifier_str |
oai:ri.conicet.gov.ar:11336/212524 |
network_acronym_str |
CONICETDig |
repository_id_str |
3498 |
network_name_str |
CONICET Digital (CONICET) |
spelling |
The Newton constant and gravitational waves in some vector field adjusting mechanismsSantillán, Osvaldo PabloScornavacche, Marina AndreaCOSMOLOGICAL PERTURBATION THEORYDARK ENERGY THEORYGRAVITATIONAL WAVES / THEORYhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1At the present, there exist some Lorentz breaking scenarios which explain the smallness of the cosmological constant at the present era [1]-[2]. An important aspect to analyze is the propagation of gravitational waves and the screening or enhancement of the Newton constant G N in these models. The problem is that the Lorentz symmetry breaking terms may induce an unacceptable value of the Newton constant G N or introduce longitudinal modes in the gravitational wave propagation. Furthermore this breaking may spoil the standard dispersion relation ω=ck. In [3] the authors have presented a model suggesting that the behavior of the gravitational constant is correct for asymptotic times. In the present work, an explicit checking is made and we finally agree with these claims. Furthermore, it is suggested that the gravitational waves are also well behaved for large times. In the process, some new models with the same behavior are obtained, thus enlarging the list of possible adjustment mechanisms.Fil: Santillán, Osvaldo Pablo. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Investigaciones Matemáticas "Luis A. Santaló". Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Investigaciones Matemáticas "Luis A. Santaló"; ArgentinaFil: Scornavacche, Marina Andrea. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; ArgentinaIOP Publishing2017-10info: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/11336/212524Santillán, Osvaldo Pablo; Scornavacche, Marina Andrea; The Newton constant and gravitational waves in some vector field adjusting mechanisms; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 10; 10-2017; 48-681475-7516CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/1475-7516/2017/10/048/pdfinfo:eu-repo/semantics/altIdentifier/doi/10.1088/1475-7516/2017/10/048info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-03T09:58:19Zoai:ri.conicet.gov.ar:11336/212524instacron: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:34982025-09-03 09:58:19.338CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
The Newton constant and gravitational waves in some vector field adjusting mechanisms |
title |
The Newton constant and gravitational waves in some vector field adjusting mechanisms |
spellingShingle |
The Newton constant and gravitational waves in some vector field adjusting mechanisms Santillán, Osvaldo Pablo COSMOLOGICAL PERTURBATION THEORY DARK ENERGY THEORY GRAVITATIONAL WAVES / THEORY |
title_short |
The Newton constant and gravitational waves in some vector field adjusting mechanisms |
title_full |
The Newton constant and gravitational waves in some vector field adjusting mechanisms |
title_fullStr |
The Newton constant and gravitational waves in some vector field adjusting mechanisms |
title_full_unstemmed |
The Newton constant and gravitational waves in some vector field adjusting mechanisms |
title_sort |
The Newton constant and gravitational waves in some vector field adjusting mechanisms |
dc.creator.none.fl_str_mv |
Santillán, Osvaldo Pablo Scornavacche, Marina Andrea |
author |
Santillán, Osvaldo Pablo |
author_facet |
Santillán, Osvaldo Pablo Scornavacche, Marina Andrea |
author_role |
author |
author2 |
Scornavacche, Marina Andrea |
author2_role |
author |
dc.subject.none.fl_str_mv |
COSMOLOGICAL PERTURBATION THEORY DARK ENERGY THEORY GRAVITATIONAL WAVES / THEORY |
topic |
COSMOLOGICAL PERTURBATION THEORY DARK ENERGY THEORY GRAVITATIONAL WAVES / THEORY |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
At the present, there exist some Lorentz breaking scenarios which explain the smallness of the cosmological constant at the present era [1]-[2]. An important aspect to analyze is the propagation of gravitational waves and the screening or enhancement of the Newton constant G N in these models. The problem is that the Lorentz symmetry breaking terms may induce an unacceptable value of the Newton constant G N or introduce longitudinal modes in the gravitational wave propagation. Furthermore this breaking may spoil the standard dispersion relation ω=ck. In [3] the authors have presented a model suggesting that the behavior of the gravitational constant is correct for asymptotic times. In the present work, an explicit checking is made and we finally agree with these claims. Furthermore, it is suggested that the gravitational waves are also well behaved for large times. In the process, some new models with the same behavior are obtained, thus enlarging the list of possible adjustment mechanisms. Fil: Santillán, Osvaldo Pablo. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Investigaciones Matemáticas "Luis A. Santaló". Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Investigaciones Matemáticas "Luis A. Santaló"; Argentina Fil: Scornavacche, Marina Andrea. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina |
description |
At the present, there exist some Lorentz breaking scenarios which explain the smallness of the cosmological constant at the present era [1]-[2]. An important aspect to analyze is the propagation of gravitational waves and the screening or enhancement of the Newton constant G N in these models. The problem is that the Lorentz symmetry breaking terms may induce an unacceptable value of the Newton constant G N or introduce longitudinal modes in the gravitational wave propagation. Furthermore this breaking may spoil the standard dispersion relation ω=ck. In [3] the authors have presented a model suggesting that the behavior of the gravitational constant is correct for asymptotic times. In the present work, an explicit checking is made and we finally agree with these claims. Furthermore, it is suggested that the gravitational waves are also well behaved for large times. In the process, some new models with the same behavior are obtained, thus enlarging the list of possible adjustment mechanisms. |
publishDate |
2017 |
dc.date.none.fl_str_mv |
2017-10 |
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/11336/212524 Santillán, Osvaldo Pablo; Scornavacche, Marina Andrea; The Newton constant and gravitational waves in some vector field adjusting mechanisms; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 10; 10-2017; 48-68 1475-7516 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/212524 |
identifier_str_mv |
Santillán, Osvaldo Pablo; Scornavacche, Marina Andrea; The Newton constant and gravitational waves in some vector field adjusting mechanisms; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 10; 10-2017; 48-68 1475-7516 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/1475-7516/2017/10/048/pdf info:eu-repo/semantics/altIdentifier/doi/10.1088/1475-7516/2017/10/048 |
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 |
IOP Publishing |
publisher.none.fl_str_mv |
IOP Publishing |
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 |
_version_ |
1842269515617927168 |
score |
13.13397 |