Gravitational antiscreening in stellar interiors
A new class of relativistic stellar structure equations which include the effects of an energy-dependent Newton coupling is presented. Significant modifications in the mass-radius relation for neutron stars are possible only if the running of the Newton coupling due to quantum gravity occurs at low...
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| Main Authors: | , , |
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| Format: | Article (Journal) |
| Language: | English |
| Published: |
January 2020
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| In: |
Journal of cosmology and astroparticle physics
Year: 2020, Issue: 1 |
| ISSN: | 1475-7516 |
| DOI: | 10.1088/1475-7516/2020/01/022 |
| Online Access: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1088/1475-7516/2020/01/022
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| Author Notes: | A. Bonanno, R. Casadio and A. Platania |
| Summary: | A new class of relativistic stellar structure equations which include the effects of an energy-dependent Newton coupling is presented. Significant modifications in the mass-radius relation for neutron stars are possible only if the running of the Newton coupling due to quantum gravity occurs at low energies. A new Buchdahl limit is derived and its physical implications are discussed. In particular, sub-Planckian self-gravitating objects with arbitrarily small radii are possible. |
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| Item Description: | Gesehen am 14.05.2020 |
| Physical Description: | Online Resource |
| ISSN: | 1475-7516 |
| DOI: | 10.1088/1475-7516/2020/01/022 |