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Title: Large and massive neutron stars: Implications for the sound speed within QCD of dense matter

Journal Article · · Physical Review. C

Here, the NASA telescope NICER has recently measured x-ray emissions from the heaviest of the precisely known two-solar mass neutron stars, PSR J0740 + 6620. Analysis of the data suggests that PSR J0740 + 6620 has a radius in the range of R2.0 ≈ (11.4 – 16.1) km at the 68% credibility level. In this article, we study the implications of this analysis for the sound speed in the high-density inner cores by using recent chiral effective field theory (χEFT) calculations of the equation of state at next-to-next-to-next-to-leading order to describe outer regions of the star at modest density. We find that the lower bound on the maximum speed of sound in the inner core, min {c$$^{2}_{s,max}$$}, increases rapidly with the radius of massive neutron stars. If χ EFT remains an efficient expansion for nuclear interactions up to about twice the nuclear saturation density, R2.0 ≥ 13 km requires min {c$$^{2}_{s,max}$$} ≥ 0.562 and 0.442 at the 68% and 95% credibility level, respectively.

Research Organization:
Univ. of Washington, Seattle, WA (United States)
Sponsoring Organization:
USDOE Office of Science (SC), Nuclear Physics (NP); National Science Foundation (NSF); Heising-Simons Foundation
Grant/Contract Number:
FG02-00ER41132; PHY-1630782; 2017-228; SC0013617
OSTI ID:
1922115
Journal Information:
Physical Review. C, Vol. 105, Issue 3; ISSN 2469-9985
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English

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