String analog of Reissner–Nordström black holes cannot be overcharged

Name: String analog of Reissner–Nordström black holes cannot be overcharged
Author: Düztaş, Koray, Jamil, M.

İsim	String analog of Reissner–Nordström black holes cannot be overcharged
Yazar	Düztaş, Koray, Jamil, M.
Basım Tarihi:	2019-09-28
Basım Yeri	- World Scientific Publishing Co Pte Lt
Konu	Black holes in string theory, Cosmic censorship, Black hole thermodynamics
Tür	Süreli Yayın
Dil	İngilizce
Dijital	Evet
Yazma	Hayır
Kütüphane:	Özyeğin Üniversitesi
Demirbaş Numarası	0217-7323
Kayıt Numarası	61e03947-b0aa-4f4b-a119-c86eed0ad61f
Lokasyon	Natural and Mathematical Sciences
Tarih	2019-09-28
Örnek Metin	In this work, we attempt to overcharge extremal and nearly extremal charged black holes in string theory, known as the Garfinkle-Horowitz-Strominger solution. We first show that extremal black holes cannot be overcharged analogous to the case of Reissner-Nordstrom (RN) black holes. Contrary to their analog in general relativity, nearly extremal black holes can neither be overcharged beyond extremality, nor can they be driven to extremality by the interaction with test particles. Therefore, the analysis in this work also implies that the third law of black hole thermodynamics holds for the relevant charged black holes in string theory perturbed by test particles. This can be interpreted as a stronger version of the third law since one can drop out the continuity proviso for the relevant process.
DOI	10.1142/S0217732319502481
Cilt	34

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String analog of Reissner–Nordström black holes cannot be overcharged

Yazar Düztaş, Koray, Jamil, M.

Basım Tarihi 2019-09-28

Basım Yeri - World Scientific Publishing Co Pte Lt

Konu Black holes in string theory, Cosmic censorship, Black hole thermodynamics

Tür Süreli Yayın

Dil İngilizce

Dijital Evet

Yazma Hayır

Kütüphane Özyeğin Üniversitesi

Demirbaş Numarası 0217-7323

Kayıt Numarası 61e03947-b0aa-4f4b-a119-c86eed0ad61f

Lokasyon Natural and Mathematical Sciences

Tarih 2019-09-28

Örnek Metin In this work, we attempt to overcharge extremal and nearly extremal charged black holes in string theory, known as the Garfinkle-Horowitz-Strominger solution. We first show that extremal black holes cannot be overcharged analogous to the case of Reissner-Nordstrom (RN) black holes. Contrary to their analog in general relativity, nearly extremal black holes can neither be overcharged beyond extremality, nor can they be driven to extremality by the interaction with test particles. Therefore, the analysis in this work also implies that the third law of black hole thermodynamics holds for the relevant charged black holes in string theory perturbed by test particles. This can be interpreted as a stronger version of the third law since one can drop out the continuity proviso for the relevant process.

DOI 10.1142/S0217732319502481

Cilt 34