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American Physical Society, Physical Review Letters, 13(97), 2006

DOI: 10.1103/physrevlett.97.131102

Cambridge University Press (CUP), Proceedings of the International Astronomical Union, H15(5), p. 314-314, 2009

DOI: 10.1017/s1743921310009518

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Constraining a Possible Time Variation of the Gravitational Constant through “Gravitochemical Heating” of Neutron Stars

Journal article published in 2006 by Paula Jofré, Andreas Reisenegger ORCID, Rodrigo Fernández
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Data provided by SHERPA/RoMEO

Abstract

AbstractA hypothetical time-variation of the gravitational constant G would produce gravitochemical heating of old (≳ 107−8 yr) neutron stars. It could produce detectable thermal ultraviolet emission from such stars for changes as small as |Ġ/G|~ 10−12 yr−1, comparable to the best existing upper limits from other methods.

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