Pregled bibliografske jedinice broj: 992065
Noncommutative Scalar Quasinormal Modes of the Reissner Nordström Black Hole
Noncommutative Scalar Quasinormal Modes of the Reissner Nordström Black Hole // Classical and quantum gravity, 35 (2018), 17; 175005, 30 doi:10.1088/1361-6382/aad201 (međunarodna recenzija, članak, znanstveni)
CROSBI ID: 992065 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Noncommutative Scalar Quasinormal Modes of the Reissner Nordström Black Hole
Autori
Dimitrijević Ćirić, Marija ; Konjik, Nikola ; Samsarov, Anđelo
Izvornik
Classical and quantum gravity (0264-9381) 35
(2018), 17;
175005, 30
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
noncommutative scalar field ; noncommutative gauge theory, Reissner–Nordström black hole ; black hole quasinormal modes
(noncommutative scalar field, noncommutative gauge theory, Reissner–Nordström black hole, black hole quasinormal modes)
Sažetak
Aiming to search for a signal of space-time noncommutativity, we study a quasinormal mode spectrum of the Reissner Nordström black hole in the presence of a deformed space-time structure. In this context we study a noncommutative (NC) deformation of a scalar field, minimally coupled to a classical Reissner Nordström background. Our model is thus semiclassical from the beginning and scalar field is in addition minimally coupled to U(1) gauge field. The deformation is performed via particularly chosen Killing twist to yield a geometrical form of the action, which maintains the diffeomorphism invariance manifest, as well as the invariance under a deformed gauge symmetry group. We find the quasinormal mode solutions of the equations of motion governing the matter content of the model in some particular range of system parameters which corresponds to a near extremal limit. In addition, we obtain a well defined analytical condition which allows for a detailed numerical analysis. Moreover, there exists a parameter range, rather restrictive though, which allows for obtaining a QNM spectrum in a closed analytic form. We also argue within a semiclassical approach that NC deformation does not affect the Hawking temperature of thermal radiation.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Projekti:
ICTP-SEENET-MTP Project PRJ09 ‘Cosmology and Strings
HRZZ-IP-2014-09-9582 - Prema kvantnoj gravitaciji: nekomutativna geometrija, teorija polja i kozmologija (Meljanac, Stjepan, HRZZ - 2014-09) ( CroRIS)
EK-H2020-692194 - Institut Ruđer Bošković Twinning projekt: korak dalje za Zavod za teorijsku fiziku (RBI-T-WINNING) (Nesti, Fabrizio, EK ) ( CroRIS)
EK-EFRR-KK.01.1.1.06.0006 - Sinergijom do uspjeha: RBI-T-WINNING i ESIF udruženi u jačanju izvrsnosti Zavoda za teorijsku fiziku Instituta Ruđer Bošković (RBI-TWINN-SIN) (Melić, Blaženka, EK ) ( CroRIS)
Ustanove:
Institut "Ruđer Bošković", Zagreb
Profili:
Anđelo Samsarov
(autor)
Citiraj ovu publikaciju:
Časopis indeksira:
- Current Contents Connect (CCC)
- Web of Science Core Collection (WoSCC)
- Science Citation Index Expanded (SCI-EXP)
- SCI-EXP, SSCI i/ili A&HCI
- Scopus