NEUTRON STARS AND THE COHERENT NUCLEAR INTERACTION
1995 ◽
Vol 04
(04)
◽
pp. 531-548
◽
Keyword(s):
In the framework of a novel approach to the dynamics of nuclei and large collections of nucleons, which fully exploits the coherent interaction among π’s, nucleons and Δ’s, we derive a new equation of state for neutronic matter. By introducing it in the Tolman-Oppenheimer-Volkof equations we derive the masses and radii of neutron stars as a function of the central density. We obtain a maximum mass Mmax≃2.7 Mʘ and a minimum period of rotation Tmin=0.8 msec.
1971 ◽
Vol 46
◽
pp. 352-355
Keyword(s):
2020 ◽
Vol 499
(1)
◽
pp. L82-L86
◽
Keyword(s):
2007 ◽
Vol 3
(S246)
◽
pp. 291-300
◽
Keyword(s):
2016 ◽
Vol 463
(3)
◽
pp. 2667-2679
◽
Keyword(s):
2006 ◽
Vol 15
(03)
◽
pp. 405-418
◽
Keyword(s):
1994 ◽
Vol 03
(04)
◽
pp. 813-838
◽
Keyword(s):