activity
20062010
most citedBulk viscosity of strange quark matter: Urca versus non-leptonic processes

52 citations · 136 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2010★ 3 cited

Strangeness in Astrophysics and Cosmology

Tillmann Boeckel, Matthias Hempel, Irina Sagert +3

Some recent developments concerning the role of strange quark matter for astrophysical systems and the QCD phase transition in the early universe are addressed. Causality constrain…

astro-ph.SR2009★ 3 cited

Dissipation of radial oscillations in compact stars

Basil A. Sa'd, Jürgen Schaffner-Bielich

We demonstrate that there exists a new mechanism for dissipating the energy of stellar oscillations. For neutron stars, in particular, we show that the mechanical energy of density…

hep-ph2008★ 33 cited

Mutual friction in a cold color flavor locked superfluid and r-mode instabilities in compact stars

Massimo Mannarelli, Cristina Manuel, Basil A. Sa'd

Dissipative processes acting in rotating neutron stars are essential in preventing the growth of the r-mode instability. We estimate the damping time of r-modes of an hypothetical…

astro-ph2008

Quark contribution to r-mode instabilities for several phases of deconfined quark matter

Basil A. Sa'd

R-mode instabilities lead to specific signatures in the evolution of rotating pulsars, and may provide a unique signature which can identify the phase of matter that exists in the…

astro-ph2007★ 52 cited

Bulk viscosity of strange quark matter: Urca versus non-leptonic processes

Basil A. Sa'd, Igor A. Shovkovy, Dirk H. Rischke

A general formalism for calculating the bulk viscosity of strange quark matter is developed. Contrary to the common belief that the non-leptonic processes alone give the dominant c…

astro-ph2006★ 45 cited

Bulk viscosity of spin-one color superconductors with two quark flavors

Basil A. Sa'd, Igor A. Shovkovy, Dirk H. Rischke

We consider the contribution of the Urca-type processes to the bulk viscosity of several spin-one color-superconducting phases of dense two-flavor quark matter. In the so-called tr…