Cool dense matter and neutron star phenomenology - INSPIRE

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Cool dense matter and neutron star phenomenology

S. Reddy
(
- Los Alamos
)
,
A.W. Steiner
(
- Los Alamos
)

2007

12 pages

Part of Proceedings, 7th International Conference on Strong and electroweak matter (SEWM 2006) : Brookhaven, Upton, USA, May 10-13, 2006

Published in:

Nucl.Phys.A 785 (2007) 24-35

Contribution to:

- SEWM 2006

DOI:

10.1016/j.nuclphysa.2006.11.130

View in:

Nuclear Science References

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Abstract: (Elsevier)

Neutron star observations offer a novel approach to exploring Quantum Chromodynamics (QCD) at high densities and low temperatures. We discuss how the physics of QCD affects the structure and evolution of neutron stars, paying particular attention to heterogeneous phases, quark matter, and neutrino transport. Afterwards, we discuss the status of several types of neutron star observations and what they mean for the physics of dense matter.

References(43)

Figures(0)

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