Neutron star cooling
DG Yakovlev, CJ Pethick - Annu. Rev. Astron. Astrophys., 2004 - annualreviews.org
▪ Abstract Observation of cooling neutron stars can potentially provide information about the
states of matter at supernuclear densities. We review physical properties important for …
states of matter at supernuclear densities. We review physical properties important for …
Strange quark matter and compact stars
F Weber - Progress in Particle and Nuclear Physics, 2005 - Elsevier
Astrophysicists distinguish between three different kinds of compact stars. These are white
dwarfs, neutron stars, and black holes. The former contain matter in one of the densest forms …
dwarfs, neutron stars, and black holes. The former contain matter in one of the densest forms …
The physics of neutron stars
JM Lattimer, M Prakash - Science, 2004 - science.org
Neutron stars are some of the densest manifestations of massive objects in the universe.
They are ideal astrophysical laboratories for testing theories of dense matter physics and …
They are ideal astrophysical laboratories for testing theories of dense matter physics and …
Equation of state of a dense and magnetized fermion system
The equation of state of a system of fermions in a uniform magnetic field is obtained in terms
of the thermodynamic quantities of the theory by using functional methods. It is shown that …
of the thermodynamic quantities of the theory by using functional methods. It is shown that …
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JM Lattimer - science, 2004 - academia.edu
Neutron stars are some of the densest manifestations of massive objects in the universe.
They are ideal astrophysical laboratories for testing theories of dense matter physics and …
They are ideal astrophysical laboratories for testing theories of dense matter physics and …
Electric fields at the quark surface of strange stars in the color-flavor locked phase
VV Usov - Physical Review D—Particles, Fields, Gravitation, and …, 2004 - APS
Electric fields at the quark surface of strange stars in the color-flavor locked phase Page 1
Electric fields at the quark surface of strange stars in the color-flavor locked phase Vladimir V …
Electric fields at the quark surface of strange stars in the color-flavor locked phase Vladimir V …
Dense matter in compact stars: theoretical developments and observational constraints
Dense Matter in Compact Stars: Theoretical Developments and Observational Constraints |
Annual Reviews Menu Publications AZ Journal Information About Subscribe Give Personal …
Annual Reviews Menu Publications AZ Journal Information About Subscribe Give Personal …
Strange star surface: A crust with nuggets
We reexamine the surface composition of strange stars. Strange quark stars are hypothetical
compact stars which could exist if strange quark matter was absolutely stable. It is widely …
compact stars which could exist if strange quark matter was absolutely stable. It is widely …
Constraining the physics of the r-mode instability in neutron stars with X-ray and ultraviolet observations
B Haskell, N Degenaar, WCG Ho - Monthly Notices of the Royal …, 2012 - academic.oup.com
Rapidly rotating neutron stars in low-mass X-ray binaries may be an interesting source of
gravitational waves (GWs). In particular, several modes of stellar oscillation may be driven …
gravitational waves (GWs). In particular, several modes of stellar oscillation may be driven …
Holographic proof of the averaged null energy condition
The averaged null energy conditions (ANEC) states that, along a complete null curve, the
negative energy fluctuations of a quantum field must be balanced by positive energy …
negative energy fluctuations of a quantum field must be balanced by positive energy …