2021
			
	    
	
	
    Repulsive gravity effects in horizon formation: Horizon remnants in naked singularities
PUGLIESE, Daniela and Hernando QUEVEDOBasic information
Original name
Repulsive gravity effects in horizon formation: Horizon remnants in naked singularities
	Authors
PUGLIESE, Daniela (380 Italy, belonging to the institution) and Hernando QUEVEDO
			Edition
 General Relativity and Gravitation, US - Spojené státy americké, 2021, 0001-7701
			Other information
Language
English
		Type of outcome
Article in a journal
		Field of Study
10308 Astronomy
		Country of publisher
United States of America
		Confidentiality degree
is not subject to a state or trade secret
		References:
Impact factor
Impact factor: 2.840
			RIV identification code
RIV/47813059:19630/21:A0000152
		Organization unit
Institute of physics in Opava
			UT WoS
000700395400001
		EID Scopus
2-s2.0-85115741467
		Keywords in English
Black holes;Naked singularities;Killing horizons;Light surfaces;Photon orbits
		Tags
International impact, Reviewed
		
				
				Changed: 17/2/2022 14:55, Mgr. Pavlína Jalůvková
				
		Abstract
In the original language
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.