Models of pulsar glitches

B Haskell, A Melatos - International Journal of Modern Physics D, 2015 - World Scientific
Radio pulsars provide us with some of the most stable clocks in the universe. Nevertheless
several pulsars exhibit sudden spin-up events, known as glitches. More than forty years after …

Color superconductivity in dense quark matter

MG Alford, A Schmitt, K Rajagopal, T Schäfer - Reviews of Modern Physics, 2008 - APS
Matter at high density and low temperature is expected to be a color superconductor, which
is a degenerate Fermi gas of quarks with a condensate of Cooper pairs near the Fermi …

[HTML][HTML] Physics of neutron star crusts

N Chamel, P Haensel - Living Reviews in relativity, 2008 - Springer
The physics of neutron star crusts is vast, involving many different research fields, from
nuclear and condensed matter physics to general relativity. This review summarizes the …

Pulsar constraints on neutron star structure and equation of state

B Link, RI Epstein, JM Lattimer - Physical Review Letters, 1999 - APS
With the aim of constraining the structural properties of neutron stars and the equation of
state of dense matter, we study sudden spin-ups, glitches, occurring in the Vela pulsar and …

Pulsar glitches: A review

S Zhou, E Gügercinoğlu, J Yuan, M Ge, C Yu - Universe, 2022 - mdpi.com
∼ 6% of all known pulsars have been observed to exhibit sudden spin-up events, known as
glitches. For more than fifty years, these phenomena have played an important role in …

Avalanche dynamics of radio pulsar glitches

A Melatos, C Peralta, JSB Wyithe - The Astrophysical Journal, 2008 - iopscience.iop.org
We test statistically the hypothesis that radio pulsar glitches result from an avalanche
process, in which angular momentum is transferred erratically from the flywheel-like …

Pairing gaps in nucleonic superfluids

JMC Chen, JW Clark, RD Davé, VV Khodel - Nuclear Physics A, 1993 - Elsevier
Singlet S-wave nucleonic superfluids are studied within a microscopic many-body theory
that incorporates explicit spatial correlations due to strong short-range repulsive forces as …

Predicting the starquakes in PSR J0537–6910

J Middleditch, FE Marshall, QD Wang… - The Astrophysical …, 2006 - iopscience.iop.org
We report on more than 7 yr of monitoring of PSR J0537-6910, the 16 ms pulsar in the LMC,
using data acquired with RXTE. During this campaign the pulsar experienced 23 sudden …

Thermal properties and detectability of neutron stars. II. Thermal evolution of rotation-powered neutron stars

S Tsuruta - Physics Reports, 1998 - Elsevier
After a brief introduction we present a progress report on the recent works carried out during
the last ten years or so, on the thermal evolution of neutron stars and related problems. The …

Physical mechanisms for the variable spin-down and light curve of SGR 1900+ 14

C Thompson, RC Duncan, PM Woods… - The Astrophysical …, 2000 - iopscience.iop.org
We consider the physical implications of the rapid spin-down of soft gamma repeater SGR
1900+ 14 reported by Woods and colleagues in 1999. During an 80 day interval between …