Interpreting cosmological tensions from the effective field theory of torsional gravity
Cosmological tensions can arise within the Lamda cold dark matter scenario amongst different observational windows, which may indicate new physics beyond the standard paradigm if confirmed by measurements. In this article, we report how to alleviate both the H-0 and sigma(8) tensions simultaneously...
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Veröffentlicht in: | Physical review. D 2020-06, Vol.101 (12), p.1, Article 121301 |
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description | Cosmological tensions can arise within the Lamda cold dark matter scenario amongst different observational windows, which may indicate new physics beyond the standard paradigm if confirmed by measurements. In this article, we report how to alleviate both the H-0 and sigma(8) tensions simultaneously within torsional gravity from the perspective of effective field theory. Following these observations, we construct concrete models of Lagrangians of torsional gravity. Specifically, we consider the parametrization f(T) = -T - 2 Lambda/M-P(2) + alpha T-beta, where two out of the three parameters are independent. This model can efficiently fit observations solving the two tensions. To our knowledge, this is the first time where a modified gravity theory can alleviate both H-0 and sigma(8) tensions simultaneously, hence, offering an additional argument in favor of gravitational modification. |
doi_str_mv | 10.1103/PhysRevD.101.121301 |
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To our knowledge, this is the first time where a modified gravity theory can alleviate both H-0 and sigma(8) tensions simultaneously, hence, offering an additional argument in favor of gravitational modification.</description><subject>Astronomy & Astrophysics</subject><subject>Cold dark matter</subject><subject>Concrete construction</subject><subject>Field theory</subject><subject>Gravitation</subject><subject>Gravity</subject><subject>Parameterization</subject><subject>Physical Sciences</subject><subject>Physics</subject><subject>Physics, Particles & Fields</subject><subject>Science & Technology</subject><issn>1550-7998</issn><issn>2470-0010</issn><issn>1550-2368</issn><issn>2470-0029</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><sourceid>AOWDO</sourceid><recordid>eNqNkF1LwzAUhosoOKe_wJuAl7J5TtL041Lq10BQRPGytGmyZXTNTLJJ_70pnV6bm4ST5zmc80bRJcIcEdjN66p3b3J_N0fAOVJkgEfRBDmHGWVJdnx4p3menUZnzq0BGE3SdBJ9Ljov7dZKr7slEcZtTGuWWlQt8bJz2nSOKGs2xK8kkUpJ4fVeEqVl2ww1Y3tiFPHGDmywlrbaa9-fRyeqap28ONzT6OPh_r14mj2_PC6K2-eZYDnzM1XVPKmz0BeaMBBS3uSoVJpD0sSUNnWacWC5SOO4phzzAKiY5pwziMMXsml0NfbdWvO1k86Xa7OzYRBX0gCGjYFBoNhICWucs1KVW6s3le1LhHJIsPxNMBSwHBMMVjZa37I2ygktOyH_TADgMcaYwHCw0L7yIYLC7Dof1Ov_q-wHsv6GmQ</recordid><startdate>20200619</startdate><enddate>20200619</enddate><creator>Yan, Sheng-Feng</creator><creator>Zhang, Pierre</creator><creator>Chen, Jie-Wen</creator><creator>Zhang, Xin-Zhe</creator><creator>Cai, Yi-Fu</creator><creator>Saridakis, Emmanuel N.</creator><general>Amer Physical Soc</general><general>American Physical Society</general><scope>AOWDO</scope><scope>BLEPL</scope><scope>DTL</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0003-0706-8465</orcidid><orcidid>https://orcid.org/0000-0003-1500-0874</orcidid><orcidid>https://orcid.org/0000-0002-8037-543X</orcidid></search><sort><creationdate>20200619</creationdate><title>Interpreting cosmological tensions from the effective field theory of torsional gravity</title><author>Yan, Sheng-Feng ; Zhang, Pierre ; Chen, Jie-Wen ; Zhang, Xin-Zhe ; Cai, Yi-Fu ; Saridakis, Emmanuel N.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c393t-fab56b8ffe0d267125d91ff7906d422db785039c744b2519125f4295530478513</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>Astronomy & Astrophysics</topic><topic>Cold dark matter</topic><topic>Concrete construction</topic><topic>Field theory</topic><topic>Gravitation</topic><topic>Gravity</topic><topic>Parameterization</topic><topic>Physical Sciences</topic><topic>Physics</topic><topic>Physics, Particles & Fields</topic><topic>Science & Technology</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Yan, Sheng-Feng</creatorcontrib><creatorcontrib>Zhang, Pierre</creatorcontrib><creatorcontrib>Chen, Jie-Wen</creatorcontrib><creatorcontrib>Zhang, Xin-Zhe</creatorcontrib><creatorcontrib>Cai, Yi-Fu</creatorcontrib><creatorcontrib>Saridakis, Emmanuel N.</creatorcontrib><collection>Web of Science - Science Citation Index Expanded - 2020</collection><collection>Web of Science Core Collection</collection><collection>Science Citation Index Expanded</collection><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>Yan, Sheng-Feng</au><au>Zhang, Pierre</au><au>Chen, Jie-Wen</au><au>Zhang, Xin-Zhe</au><au>Cai, Yi-Fu</au><au>Saridakis, Emmanuel N.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Interpreting cosmological tensions from the effective field theory of torsional gravity</atitle><jtitle>Physical review. D</jtitle><stitle>PHYS REV D</stitle><date>2020-06-19</date><risdate>2020</risdate><volume>101</volume><issue>12</issue><spage>1</spage><pages>1-</pages><artnum>121301</artnum><issn>1550-7998</issn><issn>2470-0010</issn><eissn>1550-2368</eissn><eissn>2470-0029</eissn><abstract>Cosmological tensions can arise within the Lamda cold dark matter scenario amongst different observational windows, which may indicate new physics beyond the standard paradigm if confirmed by measurements. In this article, we report how to alleviate both the H-0 and sigma(8) tensions simultaneously within torsional gravity from the perspective of effective field theory. Following these observations, we construct concrete models of Lagrangians of torsional gravity. Specifically, we consider the parametrization f(T) = -T - 2 Lambda/M-P(2) + alpha T-beta, where two out of the three parameters are independent. This model can efficiently fit observations solving the two tensions. To our knowledge, this is the first time where a modified gravity theory can alleviate both H-0 and sigma(8) tensions simultaneously, hence, offering an additional argument in favor of gravitational modification.</abstract><cop>COLLEGE PK</cop><pub>Amer Physical Soc</pub><doi>10.1103/PhysRevD.101.121301</doi><tpages>7</tpages><orcidid>https://orcid.org/0000-0003-0706-8465</orcidid><orcidid>https://orcid.org/0000-0003-1500-0874</orcidid><orcidid>https://orcid.org/0000-0002-8037-543X</orcidid></addata></record> |
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subjects | Astronomy & Astrophysics Cold dark matter Concrete construction Field theory Gravitation Gravity Parameterization Physical Sciences Physics Physics, Particles & Fields Science & Technology |
title | Interpreting cosmological tensions from the effective field theory of torsional gravity |
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