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
Full text: Unavailable
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.