Published 2009
| Version v1
Miscellaneous
R-modes, gravitational waves and neutron star exotica
Description
Full text: In this talk our current understanding of the gravitational-wave driven r-mode instability is summarized. It is explained how the neutron star composition enters the problem, and describes progress towards understanding how the instability works in superfluid stars. Recent results for hyperon and color superconducting cores are discussed. (author)
Additional details
Identifiers
Publishing Information
- Imprint Place
- Darmstadt (Germany)
- Imprint Title
- Nuclear matter at high density. Electronic proceedings of the international workshop 37 on gross properties of nuclei and nuclear excitations
- Imprint Pagination
- [200 p.]
- Journal Page Range
- [1 p.]
Conference
- Title
- International workshop 37 on gross properties of nuclei and nuclear excitations
- Acronym
- Nuclear matter at high density
- Dates
- 18-24 Jan 2009
- Place
- Hirschegg (Austria)
INIS
- Country of Publication
- Germany
- Country of Input or Organization
- Austria
- INIS RN
- 41095221
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference, Non-conventional Literature
- Descriptors DEI
- COLOR MODEL; GRAVITATIONAL WAVES; HYPERONS; NEUTRON STARS; SUPERFLUIDITY
- Descriptors DEC
- BARYONS; COMPOSITE MODELS; ELEMENTARY PARTICLES; FERMIONS; HADRONS; MATHEMATICAL MODELS; PARTICLE MODELS; QUARK MODEL; STARS; STRANGE PARTICLES