Pulsars as a probe for the nuclear and quark matter equation of state
Pulsars as a probe for the nuclear and quark matter equation of state
Pulsars as a probe for the nuclear and quark matter equation of state
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– p.7<br />
Structure <strong>of</strong> a Neutron Star (Fridolin Weber)<br />
<strong>quark</strong>−hybrid<br />
star<br />
N+e<br />
N+e+n<br />
traditional neutron star<br />
n,p,e, µ<br />
n superfluid<br />
hyperon<br />
star<br />
s u<br />
p<br />
e<br />
r<br />
c<br />
o<br />
n d<br />
u<br />
c<br />
t<br />
i<br />
n<br />
g<br />
p<br />
neutron star with<br />
pion condensate<br />
absolutely stable<br />
strange <strong>quark</strong><br />
<strong>matter</strong><br />
µ<br />
u d s<br />
Σ,Λ,Ξ,∆<br />
u,d,s<br />
<strong>quark</strong>s<br />
H<br />
n,p,e, µ<br />
K −<br />
π −<br />
r o<br />
t<br />
n o s<br />
crust<br />
Fe<br />
10 6 g/cm 3<br />
10 11 g/cm 3<br />
10 14 g/cm 3<br />
m s<br />
strange star<br />
R ~ 10 km<br />
M ~ 1.4 M<br />
nucleon star
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