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 …

2.3. Old Population 2.4. Magnetic Fields of Neutron Stars 2.5. Z and Atoll Classification 3.
Type I X-ray Bursts 3.1. Introduction 3.2. Burst Profiles 3.3. Burst Spectral Analysis 3.4 …

NEUTRON-STAR collisions occur inevitably when binary neutron stars spiral into each other
as a result of damping of gravitational radiation. Such collisions will produce a characteristic …

The 2015 centenary of the publication of Einstein's general theory of relativity, and the first
detection of gravitational waves have focused renewed attention on the question of whether …

We map the general relativistic two-body problem onto that of a test particle moving in an
effective external metric. This effective-one-body approach defines, in a non-perturbative …

A generic class of theories where gravity is mediated by one tensor field together with an
arbitrary number of scalar fields is considered. The predictions of these theories are worked …

It is shown that a wide class of tensor-scalar theories can pass the present weak-field
gravitational tests and exhibit nonperturbative strong-field deviations away from general …

Supernova 1987A ADS Classic is now deprecated. It will be completely retired in October
2019. This page will automatically redirect to the new ADS interface at that point. SAO/NASA …

We report microscopic calculations of the equation of state for dense nuclear and neutron
matter. The calculations are performed for five Hamiltonians: the Argonne v 14 and Urbana v …

An incomparable reference for astrophysicists studying pulsars and other kinds of neutron
stars, Theory of Neutron Star Magnetospheres sums up two decades of astrophysical …