Repulsive gravity effects in horizon formation: Horizon
remnants in naked singularities

J 2021

Repulsive gravity effects in horizon formation: Horizon remnants in naked singularities

PUGLIESE, Daniela a Hernando QUEVEDO

Základní údaje

Originální název

Repulsive gravity effects in horizon formation: Horizon remnants in naked singularities

Autoři

PUGLIESE, Daniela (380 Itálie, domácí) a Hernando QUEVEDO

Vydání

General Relativity and Gravitation, US - Spojené státy americké, 2021, 0001-7701

Další údaje

Jazyk

angličtina

Typ výsledku

Článek v odborném periodiku

Obor

10308 Astronomy

Stát vydavatele

Spojené státy

Utajení

není předmětem státního či obchodního tajemství

Odkazy

URL

Impakt faktor

Impact factor: 2.840

Kód RIV

RIV/47813059:19630/21:A0000152

Organizační jednotka

Fyzikální ústav v Opavě

DOI

https://doi.org/10.1007/s10714-021-02858-4

UT WoS

000700395400001

EID Scopus

2-s2.0-85115741467

Klíčová slova anglicky

Black holes;Naked singularities;Killing horizons;Light surfaces;Photon orbits

Štítky

2022, FÚ, RIV22

Příznaky

Mezinárodní význam, Recenzováno

Změněno: 17. 2. 2022 14:55, Mgr. Pavlína Jalůvková

Anotace

V originále

Repulsive gravity is a well known characteristic of naked singularities. In this work, we explore light surfaces and find new effects of repulsive gravity. We compare Kerr naked singularities with the corresponding black hole counterparts and find certain structures that are identified as horizon remnants. We argue that these features might be significant for the comprehension of processes that lead to the formation or eventually destruction of black hole Killing horizons. These features can be detected by observing photon orbits, particularly close to the rotation axis, which can be used to distinguish naked singularities from black holes.

Citovat

PUGLIESE, Daniela a Hernando QUEVEDO. Repulsive gravity effects in horizon formation: Horizon remnants in naked singularities. General Relativity and Gravitation. US - Spojené státy americké, 2021, roč. 53, č. 10, s. "89-1"-"89-14", 14 s. ISSN 0001-7701. Dostupné z: https://doi.org/10.1007/s10714-021-02858-4.

@article{58081,
   author = {Pugliese, Daniela and Quevedo, Hernando},
   article_location = {US - Spojené státy americké},
   article_number = {10},
   doi = {https://doi.org/10.1007/s10714-021-02858-4},
   keywords = {Black holes;Naked singularities;Killing horizons;Light surfaces;Photon orbits},
   language = {eng},
   issn = {0001-7701},
   journal = {General Relativity and Gravitation},
   title = {Repulsive gravity effects in horizon formation: Horizon remnants in naked singularities},
   url = {https://link.springer.com/article/10.1007/s10714-021-02858-4},
   volume = {53},
   year = {2021}
}

TY  - JOUR
ID  - 58081
AU  - Pugliese, Daniela - Quevedo, Hernando
PY  - 2021
TI  - Repulsive gravity effects in horizon formation: Horizon remnants in naked singularities
JF  - General Relativity and Gravitation
VL  - 53
IS  - 10
SP  - "89-1"-"89-14"
EP  - "89-1"-"89-14"
SN  - 00017701
KW  - Black holes;Naked singularities;Killing horizons;Light surfaces;Photon orbits
UR  - https://link.springer.com/article/10.1007/s10714-021-02858-4
N2  - Repulsive gravity is a well known characteristic of naked singularities. In this work, we explore light surfaces and find new effects of repulsive gravity. We compare Kerr naked singularities with the corresponding black hole counterparts and find certain structures that are identified as horizon remnants. We argue that these features might be significant for the comprehension of processes that lead to the formation or eventually destruction of black hole Killing horizons. These features can be detected by observing photon orbits, particularly close to the rotation axis, which can be used to distinguish naked singularities from black holes.
ER  -

PUGLIESE, Daniela a Hernando QUEVEDO. Repulsive gravity effects in horizon formation: Horizon remnants in naked singularities. \textit{General Relativity and Gravitation}. US - Spojené státy americké, 2021, roč.~53, č.~10, s.~''89-1''-''89-14'', 14 s. ISSN~0001-7701. Dostupné z: https://doi.org/10.1007/s10714-021-02858-4.

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