Loading…
Self-accelerating universe in modified gravity with dynamical torsion
We consider a model belonging to the class of gravities with dynamical torsion. The model is free of ghosts and gradient instabilities about Minkowski and torsionless Einstein backgrounds. We find that at zero cosmological constant, the model admits a self-accelerating solution with a non-Riemannian...
Saved in:
Published in: | Physical review. D 2017-01, Vol.95 (2), Article 024013 |
---|---|
Main Authors: | , , |
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-c324t-fc67c3b364c1c2dbdb4375c806ba566a6b02c5c59e1555d86c1d2d9eda9f9b303 |
---|---|
cites | cdi_FETCH-LOGICAL-c324t-fc67c3b364c1c2dbdb4375c806ba566a6b02c5c59e1555d86c1d2d9eda9f9b303 |
container_end_page | |
container_issue | 2 |
container_start_page | |
container_title | Physical review. D |
container_volume | 95 |
creator | Nikiforova, V. Randjbar-Daemi, S. Rubakov, V. |
description | We consider a model belonging to the class of gravities with dynamical torsion. The model is free of ghosts and gradient instabilities about Minkowski and torsionless Einstein backgrounds. We find that at zero cosmological constant, the model admits a self-accelerating solution with a non-Riemannian connection. Small value of the effective cosmological constant is obtained at the expense of the hierarchy between the dimensionless couplings. |
doi_str_mv | 10.1103/PhysRevD.95.024013 |
format | article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_journals_2125314998</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2125314998</sourcerecordid><originalsourceid>FETCH-LOGICAL-c324t-fc67c3b364c1c2dbdb4375c806ba566a6b02c5c59e1555d86c1d2d9eda9f9b303</originalsourceid><addsrcrecordid>eNo9kF1LwzAYhYMoOOb-gFcBrzvfJE26XMqcThgoflyH9E26ZXTtTLpK_72TqVfnuTicAw8h1wymjIG4fdkM6dX391Mtp8BzYOKMjHheQAbA9fk_M7gkk5S2cEQFumBsRBZvvq4yi-hrH20XmjU9NKH3MXkaGrprXaiCd3QdbR-6gX6FbkPd0NhdQFvTro0ptM0VuahsnfzkN8fk42HxPl9mq-fHp_ndKkPB8y6rUBUoSqFyZMhd6cpcFBJnoEorlbKqBI4SpfZMSulmCpnjTntndaVLAWJMbk67-9h-HnzqzLY9xOZ4aTjjUrBc69mxxU8tjG1K0VdmH8POxsEwMD_GzJ8xo6U5GRPf_C5g2g</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2125314998</pqid></control><display><type>article</type><title>Self-accelerating universe in modified gravity with dynamical torsion</title><source>American Physical Society:Jisc Collections:APS Read and Publish 2023-2025 (reading list)</source><creator>Nikiforova, V. ; Randjbar-Daemi, S. ; Rubakov, V.</creator><creatorcontrib>Nikiforova, V. ; Randjbar-Daemi, S. ; Rubakov, V.</creatorcontrib><description>We consider a model belonging to the class of gravities with dynamical torsion. The model is free of ghosts and gradient instabilities about Minkowski and torsionless Einstein backgrounds. We find that at zero cosmological constant, the model admits a self-accelerating solution with a non-Riemannian connection. Small value of the effective cosmological constant is obtained at the expense of the hierarchy between the dimensionless couplings.</description><identifier>ISSN: 2470-0010</identifier><identifier>EISSN: 2470-0029</identifier><identifier>DOI: 10.1103/PhysRevD.95.024013</identifier><language>eng</language><publisher>College Park: American Physical Society</publisher><subject>Cosmological constant ; Couplings ; Ghosts ; Torsion ; Universe</subject><ispartof>Physical review. D, 2017-01, Vol.95 (2), Article 024013</ispartof><rights>Copyright American Physical Society Jan 15, 2017</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c324t-fc67c3b364c1c2dbdb4375c806ba566a6b02c5c59e1555d86c1d2d9eda9f9b303</citedby><cites>FETCH-LOGICAL-c324t-fc67c3b364c1c2dbdb4375c806ba566a6b02c5c59e1555d86c1d2d9eda9f9b303</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>Nikiforova, V.</creatorcontrib><creatorcontrib>Randjbar-Daemi, S.</creatorcontrib><creatorcontrib>Rubakov, V.</creatorcontrib><title>Self-accelerating universe in modified gravity with dynamical torsion</title><title>Physical review. D</title><description>We consider a model belonging to the class of gravities with dynamical torsion. The model is free of ghosts and gradient instabilities about Minkowski and torsionless Einstein backgrounds. We find that at zero cosmological constant, the model admits a self-accelerating solution with a non-Riemannian connection. Small value of the effective cosmological constant is obtained at the expense of the hierarchy between the dimensionless couplings.</description><subject>Cosmological constant</subject><subject>Couplings</subject><subject>Ghosts</subject><subject>Torsion</subject><subject>Universe</subject><issn>2470-0010</issn><issn>2470-0029</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><recordid>eNo9kF1LwzAYhYMoOOb-gFcBrzvfJE26XMqcThgoflyH9E26ZXTtTLpK_72TqVfnuTicAw8h1wymjIG4fdkM6dX391Mtp8BzYOKMjHheQAbA9fk_M7gkk5S2cEQFumBsRBZvvq4yi-hrH20XmjU9NKH3MXkaGrprXaiCd3QdbR-6gX6FbkPd0NhdQFvTro0ptM0VuahsnfzkN8fk42HxPl9mq-fHp_ndKkPB8y6rUBUoSqFyZMhd6cpcFBJnoEorlbKqBI4SpfZMSulmCpnjTntndaVLAWJMbk67-9h-HnzqzLY9xOZ4aTjjUrBc69mxxU8tjG1K0VdmH8POxsEwMD_GzJ8xo6U5GRPf_C5g2g</recordid><startdate>20170111</startdate><enddate>20170111</enddate><creator>Nikiforova, V.</creator><creator>Randjbar-Daemi, S.</creator><creator>Rubakov, V.</creator><general>American Physical Society</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20170111</creationdate><title>Self-accelerating universe in modified gravity with dynamical torsion</title><author>Nikiforova, V. ; Randjbar-Daemi, S. ; Rubakov, V.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c324t-fc67c3b364c1c2dbdb4375c806ba566a6b02c5c59e1555d86c1d2d9eda9f9b303</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>Cosmological constant</topic><topic>Couplings</topic><topic>Ghosts</topic><topic>Torsion</topic><topic>Universe</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Nikiforova, V.</creatorcontrib><creatorcontrib>Randjbar-Daemi, S.</creatorcontrib><creatorcontrib>Rubakov, V.</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</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Nikiforova, V.</au><au>Randjbar-Daemi, S.</au><au>Rubakov, V.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Self-accelerating universe in modified gravity with dynamical torsion</atitle><jtitle>Physical review. D</jtitle><date>2017-01-11</date><risdate>2017</risdate><volume>95</volume><issue>2</issue><artnum>024013</artnum><issn>2470-0010</issn><eissn>2470-0029</eissn><abstract>We consider a model belonging to the class of gravities with dynamical torsion. The model is free of ghosts and gradient instabilities about Minkowski and torsionless Einstein backgrounds. We find that at zero cosmological constant, the model admits a self-accelerating solution with a non-Riemannian connection. Small value of the effective cosmological constant is obtained at the expense of the hierarchy between the dimensionless couplings.</abstract><cop>College Park</cop><pub>American Physical Society</pub><doi>10.1103/PhysRevD.95.024013</doi></addata></record> |
fulltext | fulltext |
identifier | ISSN: 2470-0010 |
ispartof | Physical review. D, 2017-01, Vol.95 (2), Article 024013 |
issn | 2470-0010 2470-0029 |
language | eng |
recordid | cdi_proquest_journals_2125314998 |
source | American Physical Society:Jisc Collections:APS Read and Publish 2023-2025 (reading list) |
subjects | Cosmological constant Couplings Ghosts Torsion Universe |
title | Self-accelerating universe in modified gravity with dynamical torsion |
url | http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-28T03%3A49%3A32IST&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=Self-accelerating%20universe%20in%20modified%20gravity%20with%20dynamical%20torsion&rft.jtitle=Physical%20review.%20D&rft.au=Nikiforova,%20V.&rft.date=2017-01-11&rft.volume=95&rft.issue=2&rft.artnum=024013&rft.issn=2470-0010&rft.eissn=2470-0029&rft_id=info:doi/10.1103/PhysRevD.95.024013&rft_dat=%3Cproquest_cross%3E2125314998%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c324t-fc67c3b364c1c2dbdb4375c806ba566a6b02c5c59e1555d86c1d2d9eda9f9b303%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2125314998&rft_id=info:pmid/&rfr_iscdi=true |