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Neutron stars: a cosmic hadron physics laboratory
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Pines, David |
| Copyright Year | 1989 |
| Description | A progress report is given on neutron stars as a cosmic hadron physics laboratory. Particular attention is paid to the crustal neutron superfluid, and to the information concerning its properties which may be deduced from observations of pulsar glitches and postglitch behavior. Current observational evidence concerning the softness or stiffness of the high density neutron matter equation of state is reviewed briefly, and the (revolutionary) implications of a confirmation of the existence of a 0.5 ms pulsar at the core of (Supernova) SN1987A are discussed. |
| File Size | 988952 |
| Page Count | 23 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19890016406 |
| Archival Resource Key | ark:/13960/t80k78n5r |
| Language | English |
| Publisher Date | 1989-01-01 |
| Access Restriction | Open |
| Subject Keyword | Astrophysics Hadrons Extraterrestrial Matter Neutron Stars Equations of State Particle Interactions Pulsars Neutrons Stellar Physics Supernova 1987a Degenerate Matter Superfluidity Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
