Impact of Pycnonuclear Fusion Uncertainties on the Cooling of Accreting Neutron Star Crusts

The observation of X-rays during quiescence from transiently accreting neutron stars provides unique clues about the nature of dense matter. This, however, requires extensive modeling of the crusts and matching the results to observations. The pycnonuclear fusion reaction rates implemented in these...

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Bibliografiske detaljer

Principais autores:	R. Jain, E. F. Brown, H. Schatz, A. V. Afanasjev, M. Beard, L. R. Gasques, S. S. Gupta, G. W. Hitt, W. R. Hix, R. Lau, P. Möller, W. J. Ong, M. Wiescher, Y. Xu
Format:	Artigo
Sprog:	Inglês
Udgivet:	IOP Publishing 2023-01-01
Serier:	The Astrophysical Journal
Fag:	Nuclear astrophysics Neutron stars Degenerate matter X-ray transient sources
Online adgang:	https://doi.org/10.3847/1538-4357/acebc4
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