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
Create successful ePaper yourself
Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.
Maximum m<strong>as</strong>ses <strong>of</strong> neutron stars with hyperons<br />
– p.8<br />
Brueckner-Hartree-Fock<br />
calculation with most recent s<strong>of</strong>t<br />
core Nijmegen potential ESC08<br />
includes repulsive three-body<br />
<strong>for</strong>ces (TBF, UIX’)<br />
overall findings: M < 1.4M ⊙<br />
when hyperons are included<br />
higher m<strong>as</strong>ses possible within<br />
RMF model <strong>and</strong> SU(3)<br />
symmetry (Weissenborn,<br />
Chatterjee, JSB, in preparation)<br />
(Schulze <strong>and</strong> Rijken 2011)<br />
o<strong>the</strong>r possible solution:<br />
<strong>quark</strong> <strong>matter</strong> core<br />
a stiff
Change language