Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/28135| Title: | Neutron Stars as Particle Accelerators | Authors: | CARAVEO, PATRIZIA | Issue Date: | 2018 | Journal: | NUCLEAR AND PARTICLE PHYSICS PROCEEDINGS | Number: | 297-299 | First Page: | 96 | Abstract: | According to standard theoretical interpretations, in neutron stars’ magnetospheres particles are accelerated along the magnetic field lines where the highly-magnetized surrounding o ers the ideal conditions to make them radiate high-energy gamma-rays (E > 100 MeV) that bear the timing signature of their parent neutron star. | URI: | http://hdl.handle.net/20.500.12386/28135 | URL: | https://www.sciencedirect.com/science/article/pii/S2405601418301020?via%3Dihub | ISSN: | 2405-6014 | DOI: | 10.1016/j.nuclphysbps.2018.07.015 | Bibcode ADS: | 2018NPPP..297...96C | Fulltext: | open |
| Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| Caraveo-rev.pdf | postprint | 134.16 kB | Adobe PDF | View/Open |
| 1-s2.0-S2405601418301020-main.pdf | [Administrators only] | 158.36 kB | Adobe PDF |
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