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Probing neutron-star superfluidity with gravitational-wave data.
| Content Provider | Semantic Scholar |
|---|---|
| Author | Andersson, Nils Comer, Gregory L. |
| Copyright Year | 2001 |
| Abstract | We discuss the possibility that future gravitational-wave detectors may be able to detect various modes of oscillation of old, cold neutron stars. We argue that such detections would provide unique insights into the superfluid nature of neutron-star cores, and could also lead to a much improved understanding of pulsar glitches. Our estimates are based on a detector configuration with several narrow-band (cryogenic) interferometers operating as a "xylophone" which could lead to high sensitivity at high frequencies. We also draw on recent advances in our understanding of the dynamics of pulsating superfluid neutron-star cores. |
| Starting Page | 241101 |
| Ending Page | 241101 |
| Page Count | 1 |
| File Format | PDF HTM / HTML |
| Alternate Webpage(s) | https://arxiv.org/pdf/gr-qc/0110112.pdf |
| PubMed reference number | 11736491v1 |
| Volume Number | 87 |
| Issue Number | 24 |
| Journal | Physical review letters |
| Language | English |
| Access Restriction | Open |
| Subject Keyword | Detectors Estimated GUCY2C protein, human Neutrons Pulsar Stars, Celestial |
| Content Type | Text |
| Resource Type | Article |
