Loading…

Circular geodesics and accretion disks in the Janis-Newman-Winicour and gamma metric spacetimes

We study here circular timelike geodesics in the Janis-Newman-Winicour and Gamma metric spacetimes which contain a strong curvature naked singularity and reduce to the Schwarzschild metric for a specific value of one of the parameters. We show that for both the metrics the range of allowed parameter...

Full description

Saved in:
Bibliographic Details
Published in:Physical review. D, Particles, fields, gravitation, and cosmology Particles, fields, gravitation, and cosmology, 2012-05, Vol.85 (10), Article 104031
Main Authors: Chowdhury, Anirban N., Patil, Mandar, Malafarina, Daniele, Joshi, Pankaj S.
Format: Article
Language:English
Subjects:
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-c346t-ddd883b1395dc60db8df472c4fca83765edf5326dbd2aa482f4a64b4f9f6edb03
cites cdi_FETCH-LOGICAL-c346t-ddd883b1395dc60db8df472c4fca83765edf5326dbd2aa482f4a64b4f9f6edb03
container_end_page
container_issue 10
container_start_page
container_title Physical review. D, Particles, fields, gravitation, and cosmology
container_volume 85
creator Chowdhury, Anirban N.
Patil, Mandar
Malafarina, Daniele
Joshi, Pankaj S.
description We study here circular timelike geodesics in the Janis-Newman-Winicour and Gamma metric spacetimes which contain a strong curvature naked singularity and reduce to the Schwarzschild metric for a specific value of one of the parameters. We show that for both the metrics the range of allowed parameters can be divided into three regimes where structure of the circular geodesics is qualitatively different. It follows that the properties of the accretion disks around such naked singularities can be significantly different from those of disks around black holes. This adds to previous studies showing that if naked singularities exist in nature, their observational signature would be significantly different from that of the black hole.
doi_str_mv 10.1103/PhysRevD.85.104031
format article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_1701114954</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1701114954</sourcerecordid><originalsourceid>FETCH-LOGICAL-c346t-ddd883b1395dc60db8df472c4fca83765edf5326dbd2aa482f4a64b4f9f6edb03</originalsourceid><addsrcrecordid>eNo1kD1PwzAYhC0EEqXwB5g8sqTYsZ04IyrfqgAhEKPl2K9bQ5MUvwmo_55Cy3Q33J1ODyGnnE04Z-L8abHGZ_i6nGg14UwywffIiCvFslwUen_ny6rSh-QI8Z0xkRdlOSJmGpMbljbROXQeMDqktvXUOpegj11LfcQPpLGl_QLovW0jZg_w3dg2e4ttdN2Q_gpz2zSWNtCn6CiurNu0G8BjchDsEuFkp2Pyen31Mr3NZo83d9OLWeaELPrMe6-1qLmolHcF87X2QZa5k8FZLcpCgQ9qc9nXPrdW6jxIW8hahioU4GsmxuRsu7tK3ecA2JsmooPl0rbQDWh4yTjnslJyE823UZc6xATBrFJsbFobzswvTfNP02hltjTFDx3Sa_g</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1701114954</pqid></control><display><type>article</type><title>Circular geodesics and accretion disks in the Janis-Newman-Winicour and gamma metric spacetimes</title><source>American Physical Society:Jisc Collections:APS Read and Publish 2023-2025 (reading list)</source><creator>Chowdhury, Anirban N. ; Patil, Mandar ; Malafarina, Daniele ; Joshi, Pankaj S.</creator><creatorcontrib>Chowdhury, Anirban N. ; Patil, Mandar ; Malafarina, Daniele ; Joshi, Pankaj S.</creatorcontrib><description>We study here circular timelike geodesics in the Janis-Newman-Winicour and Gamma metric spacetimes which contain a strong curvature naked singularity and reduce to the Schwarzschild metric for a specific value of one of the parameters. We show that for both the metrics the range of allowed parameters can be divided into three regimes where structure of the circular geodesics is qualitatively different. It follows that the properties of the accretion disks around such naked singularities can be significantly different from those of disks around black holes. This adds to previous studies showing that if naked singularities exist in nature, their observational signature would be significantly different from that of the black hole.</description><identifier>ISSN: 1550-7998</identifier><identifier>EISSN: 1550-2368</identifier><identifier>DOI: 10.1103/PhysRevD.85.104031</identifier><language>eng</language><subject>Accretion disks ; Circularity ; Cosmology ; Curvature ; Gravitation ; Mathematical analysis ; Naked singularities ; Schwarzschild metric ; Signatures</subject><ispartof>Physical review. D, Particles, fields, gravitation, and cosmology, 2012-05, Vol.85 (10), Article 104031</ispartof><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c346t-ddd883b1395dc60db8df472c4fca83765edf5326dbd2aa482f4a64b4f9f6edb03</citedby><cites>FETCH-LOGICAL-c346t-ddd883b1395dc60db8df472c4fca83765edf5326dbd2aa482f4a64b4f9f6edb03</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Chowdhury, Anirban N.</creatorcontrib><creatorcontrib>Patil, Mandar</creatorcontrib><creatorcontrib>Malafarina, Daniele</creatorcontrib><creatorcontrib>Joshi, Pankaj S.</creatorcontrib><title>Circular geodesics and accretion disks in the Janis-Newman-Winicour and gamma metric spacetimes</title><title>Physical review. D, Particles, fields, gravitation, and cosmology</title><description>We study here circular timelike geodesics in the Janis-Newman-Winicour and Gamma metric spacetimes which contain a strong curvature naked singularity and reduce to the Schwarzschild metric for a specific value of one of the parameters. We show that for both the metrics the range of allowed parameters can be divided into three regimes where structure of the circular geodesics is qualitatively different. It follows that the properties of the accretion disks around such naked singularities can be significantly different from those of disks around black holes. This adds to previous studies showing that if naked singularities exist in nature, their observational signature would be significantly different from that of the black hole.</description><subject>Accretion disks</subject><subject>Circularity</subject><subject>Cosmology</subject><subject>Curvature</subject><subject>Gravitation</subject><subject>Mathematical analysis</subject><subject>Naked singularities</subject><subject>Schwarzschild metric</subject><subject>Signatures</subject><issn>1550-7998</issn><issn>1550-2368</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2012</creationdate><recordtype>article</recordtype><recordid>eNo1kD1PwzAYhC0EEqXwB5g8sqTYsZ04IyrfqgAhEKPl2K9bQ5MUvwmo_55Cy3Q33J1ODyGnnE04Z-L8abHGZ_i6nGg14UwywffIiCvFslwUen_ny6rSh-QI8Z0xkRdlOSJmGpMbljbROXQeMDqktvXUOpegj11LfcQPpLGl_QLovW0jZg_w3dg2e4ttdN2Q_gpz2zSWNtCn6CiurNu0G8BjchDsEuFkp2Pyen31Mr3NZo83d9OLWeaELPrMe6-1qLmolHcF87X2QZa5k8FZLcpCgQ9qc9nXPrdW6jxIW8hahioU4GsmxuRsu7tK3ecA2JsmooPl0rbQDWh4yTjnslJyE823UZc6xATBrFJsbFobzswvTfNP02hltjTFDx3Sa_g</recordid><startdate>20120521</startdate><enddate>20120521</enddate><creator>Chowdhury, Anirban N.</creator><creator>Patil, Mandar</creator><creator>Malafarina, Daniele</creator><creator>Joshi, Pankaj S.</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20120521</creationdate><title>Circular geodesics and accretion disks in the Janis-Newman-Winicour and gamma metric spacetimes</title><author>Chowdhury, Anirban N. ; Patil, Mandar ; Malafarina, Daniele ; Joshi, Pankaj S.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c346t-ddd883b1395dc60db8df472c4fca83765edf5326dbd2aa482f4a64b4f9f6edb03</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2012</creationdate><topic>Accretion disks</topic><topic>Circularity</topic><topic>Cosmology</topic><topic>Curvature</topic><topic>Gravitation</topic><topic>Mathematical analysis</topic><topic>Naked singularities</topic><topic>Schwarzschild metric</topic><topic>Signatures</topic><toplevel>online_resources</toplevel><creatorcontrib>Chowdhury, Anirban N.</creatorcontrib><creatorcontrib>Patil, Mandar</creatorcontrib><creatorcontrib>Malafarina, Daniele</creatorcontrib><creatorcontrib>Joshi, Pankaj S.</creatorcontrib><collection>CrossRef</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Physical review. D, Particles, fields, gravitation, and cosmology</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Chowdhury, Anirban N.</au><au>Patil, Mandar</au><au>Malafarina, Daniele</au><au>Joshi, Pankaj S.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Circular geodesics and accretion disks in the Janis-Newman-Winicour and gamma metric spacetimes</atitle><jtitle>Physical review. D, Particles, fields, gravitation, and cosmology</jtitle><date>2012-05-21</date><risdate>2012</risdate><volume>85</volume><issue>10</issue><artnum>104031</artnum><issn>1550-7998</issn><eissn>1550-2368</eissn><abstract>We study here circular timelike geodesics in the Janis-Newman-Winicour and Gamma metric spacetimes which contain a strong curvature naked singularity and reduce to the Schwarzschild metric for a specific value of one of the parameters. We show that for both the metrics the range of allowed parameters can be divided into three regimes where structure of the circular geodesics is qualitatively different. It follows that the properties of the accretion disks around such naked singularities can be significantly different from those of disks around black holes. This adds to previous studies showing that if naked singularities exist in nature, their observational signature would be significantly different from that of the black hole.</abstract><doi>10.1103/PhysRevD.85.104031</doi></addata></record>
fulltext fulltext
identifier ISSN: 1550-7998
ispartof Physical review. D, Particles, fields, gravitation, and cosmology, 2012-05, Vol.85 (10), Article 104031
issn 1550-7998
1550-2368
language eng
recordid cdi_proquest_miscellaneous_1701114954
source American Physical Society:Jisc Collections:APS Read and Publish 2023-2025 (reading list)
subjects Accretion disks
Circularity
Cosmology
Curvature
Gravitation
Mathematical analysis
Naked singularities
Schwarzschild metric
Signatures
title Circular geodesics and accretion disks in the Janis-Newman-Winicour and gamma metric spacetimes
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-02T21%3A12%3A23IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Circular%20geodesics%20and%20accretion%20disks%20in%20the%20Janis-Newman-Winicour%20and%20gamma%20metric%20spacetimes&rft.jtitle=Physical%20review.%20D,%20Particles,%20fields,%20gravitation,%20and%20cosmology&rft.au=Chowdhury,%20Anirban%20N.&rft.date=2012-05-21&rft.volume=85&rft.issue=10&rft.artnum=104031&rft.issn=1550-7998&rft.eissn=1550-2368&rft_id=info:doi/10.1103/PhysRevD.85.104031&rft_dat=%3Cproquest_cross%3E1701114954%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c346t-ddd883b1395dc60db8df472c4fca83765edf5326dbd2aa482f4a64b4f9f6edb03%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=1701114954&rft_id=info:pmid/&rfr_iscdi=true