An independent constraint on the secular rate of variation of the gravitational constant from pulsating white dwarfs
A secular variation of the gravitational constant modifies the structure and evolutionary time scales of white dwarfs. Using an state-of-the-art stellar evolutionary code and an up-to-date pulsational code we compute the effects of a secularly varying G on the pulsational properties of variable whit...
Autores principales: | , , , |
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Formato: | Articulo Preprint |
Lenguaje: | Inglés |
Publicado: |
2013
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Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/93932 http://iopscience.iop.org/article/10.1088/1475-7516/2013/06/032 |
Aporte de: |
id |
I19-R120-10915-93932 |
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record_format |
dspace |
institution |
Universidad Nacional de La Plata |
institution_str |
I-19 |
repository_str |
R-120 |
collection |
SEDICI (UNLP) |
language |
Inglés |
topic |
Ciencias Astronómicas Gravity White dwarfs Brown dwarfs |
spellingShingle |
Ciencias Astronómicas Gravity White dwarfs Brown dwarfs Córsico, Alejandro Hugo Althaus, Leandro Gabriel García Berro, Enrique Romero, Alejandra Daniela An independent constraint on the secular rate of variation of the gravitational constant from pulsating white dwarfs |
topic_facet |
Ciencias Astronómicas Gravity White dwarfs Brown dwarfs |
description |
A secular variation of the gravitational constant modifies the structure and evolutionary time scales of white dwarfs. Using an state-of-the-art stellar evolutionary code and an up-to-date pulsational code we compute the effects of a secularly varying G on the pulsational properties of variable white dwarfs. Comparing the the theoretical results obtained taking into account the effects of a running G with the observed periods and measured rates of change of the periods of two well studied pulsating white dwarfs, G117-B15A and R548, we place constraints on the rate of variation of Newton's constant. We derive an upper bound Ġ/G ~ −1.8 × 10−10 yr−1 using the variable white dwarf G117-B15A, and Ġ/G ~ −1.3 × 10−10 yr−1 using R548. Although these upper limits are currently less restrictive than those obtained using other techniques, they can be improved in a future measuring the rate of change of the period of massive white dwarfs.
Export citation and abstract |
format |
Articulo Preprint |
author |
Córsico, Alejandro Hugo Althaus, Leandro Gabriel García Berro, Enrique Romero, Alejandra Daniela |
author_facet |
Córsico, Alejandro Hugo Althaus, Leandro Gabriel García Berro, Enrique Romero, Alejandra Daniela |
author_sort |
Córsico, Alejandro Hugo |
title |
An independent constraint on the secular rate of variation of the gravitational constant from pulsating white dwarfs |
title_short |
An independent constraint on the secular rate of variation of the gravitational constant from pulsating white dwarfs |
title_full |
An independent constraint on the secular rate of variation of the gravitational constant from pulsating white dwarfs |
title_fullStr |
An independent constraint on the secular rate of variation of the gravitational constant from pulsating white dwarfs |
title_full_unstemmed |
An independent constraint on the secular rate of variation of the gravitational constant from pulsating white dwarfs |
title_sort |
independent constraint on the secular rate of variation of the gravitational constant from pulsating white dwarfs |
publishDate |
2013 |
url |
http://sedici.unlp.edu.ar/handle/10915/93932 http://iopscience.iop.org/article/10.1088/1475-7516/2013/06/032 |
work_keys_str_mv |
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bdutipo_str |
Repositorios |
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1764820491991777282 |