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Cosmic censorship, massless fermionic test fields, and absorption probabilities

İsim Cosmic censorship, massless fermionic test fields, and absorption probabilities
Yazar Düztaş, Koray
Basım Tarihi: 2021-12-24
Basım Yeri - Springer
Tür Süreli Yayın
Dil İngilizce
Dijital Evet
Yazma Hayır
Kütüphane: Özyeğin Üniversitesi
Demirbaş Numarası 1434-6044
Kayıt Numarası 915de062-da10-458d-8255-f17c3d898085
Lokasyon Natural and Mathematical Sciences
Tarih 2021-12-24
Örnek Metin In the conventional approach, fermionic test fields lead to a generic overspinning of black holes resulting in the formation of naked singularities. The absorption of the fermionic test fields with arbitrarily low frequencies is allowed for which the contribution to the angular momentum parameter of the space-time diverges. Recently we have suggested a more subtle treatment of the problem considering the fact that only the fraction of the test fields that is absorbed by the black hole contributes to the space-time parameters. Here, we re-consider the interaction of massless spin (1/2) fields with Kerr and Kerr-Newman black holes, adapting this new approach. We show that the drastic divergence problem disappears when one incorporates the absorption probabilities. Still, there exists a range of parameters for the test fields that can lead to overspinning. We employ backreaction effects due to the self-energy of the test fields which fixes the overspinning problem for fields with relatively large amplitudes, and renders it non-generic for smaller amplitudes. This non-generic overspinning appears likely to be fixed by alternative semi-classical and quantum effects.
DOI 10.1140/epjc/s10052-021-09937-5
Cilt 81
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Cosmic censorship, massless fermionic test fields, and absorption probabilities

Yazar Düztaş, Koray
Basım Tarihi 2021-12-24
Basım Yeri - Springer
Tür Süreli Yayın
Dil İngilizce
Dijital Evet
Yazma Hayır
Kütüphane Özyeğin Üniversitesi
Demirbaş Numarası 1434-6044
Kayıt Numarası 915de062-da10-458d-8255-f17c3d898085
Lokasyon Natural and Mathematical Sciences
Tarih 2021-12-24
Örnek Metin In the conventional approach, fermionic test fields lead to a generic overspinning of black holes resulting in the formation of naked singularities. The absorption of the fermionic test fields with arbitrarily low frequencies is allowed for which the contribution to the angular momentum parameter of the space-time diverges. Recently we have suggested a more subtle treatment of the problem considering the fact that only the fraction of the test fields that is absorbed by the black hole contributes to the space-time parameters. Here, we re-consider the interaction of massless spin (1/2) fields with Kerr and Kerr-Newman black holes, adapting this new approach. We show that the drastic divergence problem disappears when one incorporates the absorption probabilities. Still, there exists a range of parameters for the test fields that can lead to overspinning. We employ backreaction effects due to the self-energy of the test fields which fixes the overspinning problem for fields with relatively large amplitudes, and renders it non-generic for smaller amplitudes. This non-generic overspinning appears likely to be fixed by alternative semi-classical and quantum effects.
DOI 10.1140/epjc/s10052-021-09937-5
Cilt 81
Özyeğin Üniversitesi
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