• Nenhum resultado encontrado

[PENDING] Elementary excitations in homogeneous superfluid neutron star matter: Role of the proton component

N/A
N/A
Info
Descarregar agora
Protected

Academic year: 2024

Share "Elementary excitations in homogeneous superfluid neutron star matter: Role of the proton component"

Copied!
23
0
0

Carregando.... (Ver texto completo agora)

Descarregar agora ( 23 páginas )

Texto

Imagem

FIG. 1: Proton excitation spectrum with pairing interaction only. The proton density corresponds to the case of neutron-star matter at nuclear saturation density, with a proton fraction fixed by β equilibrium, which means a proton Fermi momentum k Fp = 0.5
FIG. 2: Proton excitation spectrum with pairing and Coulomb interactions, ignoring the electron component
FIG. 3: Proton excitation spectrum with pairing and Coulomb interactions, including the electron component
FIG. 4: Velocity of the Goldstone mode as a function of proton density. v G : velocity of the Goldstone mode in the pure pairing case (purepair)
+6

Referências

Descarregar agora ( PDF - 23 páginas - 496.77 KB )

Documentos relacionados