File Download
Links for fulltext
(May Require Subscription)
- Publisher Website: 10.1103/PhysRevD.78.084015
- Scopus: eid_2-s2.0-54249099673
- WOS: WOS:000260574900077
- Find via
Supplementary
- Citations:
- Appears in Collections:
Article: Thin accretion disks onto brane world black holes
Title | Thin accretion disks onto brane world black holes | ||||
---|---|---|---|---|---|
Authors | |||||
Issue Date | 2008 | ||||
Publisher | American Physical Society. The Journal's web site is located at http://prd.aps.org | ||||
Citation | Physical Review D (Particles, Fields, Gravitation and Cosmology), 2008, v. 78 n. 8, article no. 084015 How to Cite? | ||||
Abstract | The brane-world description of our universe entails a large extra dimension and a fundamental scale of gravity that might be lower by several orders of magnitude as compared to the Planck scale. An interesting consequence of the brane-world scenario is in the nature of the vacuum solutions of the brane gravitational field equations, with properties quite distinct as compared to the standard black-hole solutions of general relativity. One possibility of observationally discriminating between different types of black holes is the study of the emission properties of the accretion disks. In the present paper we obtain the energy flux, the emission spectrum and accretion efficiency from the accretion disks around several classes of static and rotating brane-world black holes, and we compare them to the general relativistic case. Particular signatures can appear in the electromagnetic spectrum, thus leading to the possibility of directly testing extra-dimensional physical models by using astrophysical observations of the emission spectra from accretion disks. © 2008 The American Physical Society. | ||||
Persistent Identifier | http://hdl.handle.net/10722/91820 | ||||
ISSN | 2014 Impact Factor: 4.643 | ||||
ISI Accession Number ID |
Funding Information: The work of T. H. is supported by an RGC grant of the government of the Hong Kong SAR. | ||||
References |
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Pun, CSJ | en_HK |
dc.contributor.author | Kovács, Z | en_HK |
dc.contributor.author | Harko, T | en_HK |
dc.date.accessioned | 2010-09-17T10:27:34Z | - |
dc.date.available | 2010-09-17T10:27:34Z | - |
dc.date.issued | 2008 | en_HK |
dc.identifier.citation | Physical Review D (Particles, Fields, Gravitation and Cosmology), 2008, v. 78 n. 8, article no. 084015 | - |
dc.identifier.issn | 1550-7998 | en_HK |
dc.identifier.uri | http://hdl.handle.net/10722/91820 | - |
dc.description.abstract | The brane-world description of our universe entails a large extra dimension and a fundamental scale of gravity that might be lower by several orders of magnitude as compared to the Planck scale. An interesting consequence of the brane-world scenario is in the nature of the vacuum solutions of the brane gravitational field equations, with properties quite distinct as compared to the standard black-hole solutions of general relativity. One possibility of observationally discriminating between different types of black holes is the study of the emission properties of the accretion disks. In the present paper we obtain the energy flux, the emission spectrum and accretion efficiency from the accretion disks around several classes of static and rotating brane-world black holes, and we compare them to the general relativistic case. Particular signatures can appear in the electromagnetic spectrum, thus leading to the possibility of directly testing extra-dimensional physical models by using astrophysical observations of the emission spectra from accretion disks. © 2008 The American Physical Society. | en_HK |
dc.language | eng | en_HK |
dc.publisher | American Physical Society. The Journal's web site is located at http://prd.aps.org | en_HK |
dc.relation.ispartof | Physical Review D (Particles, Fields, Gravitation and Cosmology) | - |
dc.rights | Copyright 2008 by The American Physical Society. This article is available online at https://doi.org/10.1103/PhysRevD.78.084015 | - |
dc.title | Thin accretion disks onto brane world black holes | en_HK |
dc.type | Article | en_HK |
dc.identifier.email | Pun, CSJ: jcspun@hkucc.hku.hk | en_HK |
dc.identifier.email | Harko, T: harko@hkucc.hku.hk | en_HK |
dc.identifier.authority | Pun, CSJ=rp00772 | en_HK |
dc.identifier.authority | Harko, T=rp01333 | en_HK |
dc.description.nature | published_or_final_version | - |
dc.identifier.doi | 10.1103/PhysRevD.78.084015 | en_HK |
dc.identifier.scopus | eid_2-s2.0-54249099673 | en_HK |
dc.identifier.hkuros | 161438 | - |
dc.relation.references | http://www.scopus.com/mlt/select.url?eid=2-s2.0-54249099673&selection=ref&src=s&origin=recordpage | en_HK |
dc.identifier.volume | 78 | en_HK |
dc.identifier.issue | 8 | en_HK |
dc.identifier.spage | article no. 084015 | - |
dc.identifier.epage | article no. 084015 | - |
dc.identifier.eissn | 1550-2368 | - |
dc.identifier.isi | WOS:000260574900077 | - |
dc.publisher.place | United States | en_HK |
dc.identifier.scopusauthorid | Pun, CSJ=7003931846 | en_HK |
dc.identifier.scopusauthorid | Kovács, Z=36483148800 | en_HK |
dc.identifier.scopusauthorid | Harko, T=7006485783 | en_HK |
dc.identifier.issnl | 1550-2368 | - |