An upper limit to the secular variation of the gravitational constant from white dwarf stars

A variation of the gravitational constant over cosmological ages modifies the main sequence lifetimes and white dwarf cooling ages. Using an state-of-the-art stellar evolutionary code we compute the effects of a secularly varying G on the main sequence ages and, employing white dwarf cooling ages co...

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Autores principales: García Berro, Enrique, Lorén Aguilar, Pablo, Torres, Santiago, Althaus, Leandro Gabriel, Isern, Jordi
Formato: Articulo Preprint
Lenguaje:Inglés
Publicado: 2011
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/93935
http://iopscience.iop.org/article/10.1088/1475-7516/2011/05/021/meta
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