Analytic study of the effect of dark energy-dark matter interaction on the growth of structures

Large-scale structure has been shown as a promising cosmic probe for distinguishing and constraining dark energy models. Using the growth index parametrization, we obtain an analytic formula for the growth rate of structures in a coupled dark energy model in which the exchange of energy-momentum is...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:arXiv.org 2016-10
Hauptverfasser: Marcondes, Rafael J F, Landim, Ricardo C G, Costa, André A, Wang, Bin, Abdalla, Elcio
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page
container_issue
container_start_page
container_title arXiv.org
container_volume
creator Marcondes, Rafael J F
Landim, Ricardo C G
Costa, André A
Wang, Bin
Abdalla, Elcio
description Large-scale structure has been shown as a promising cosmic probe for distinguishing and constraining dark energy models. Using the growth index parametrization, we obtain an analytic formula for the growth rate of structures in a coupled dark energy model in which the exchange of energy-momentum is proportional to the dark energy density. We find that the evolution of \(f \sigma_8\) can be determined analytically once we know the coupling, the dark energy equation of state, the present value of the dark energy density parameter and the current mean amplitude of dark matter fluctuations. After correcting the growth function for the correspondence with the velocity field through the continuity equation in the interacting model, we use our analytic result to compare the model's predictions with large-scale structure observations.
doi_str_mv 10.48550/arxiv.1605.05264
format Article
fullrecord <record><control><sourceid>proquest_arxiv</sourceid><recordid>TN_cdi_arxiv_primary_1605_05264</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2080878452</sourcerecordid><originalsourceid>FETCH-LOGICAL-a522-57624b5adb4e6360d9e58257991486fb1255a70457a1c16b535d9037d174236a3</originalsourceid><addsrcrecordid>eNotUMtqwzAQFIVCQ5oP6KmCnu1KK60kH0PoIxDoJXcj23LiNLFTSW7rv6-dFJZ9wMywM4Q8cJZKg8ierf9tvlOuGKYMQckbMgMheGIkwB1ZhHBgjIHSgChmJF-29jjEpqQh9tVAu5rGvaOurl0Zp6uy_pO61vndkFz2k43Redq0Y7dlbLqWjjWRdr77ifuJFKLvy9h7F-7JbW2PwS3-55xsX1-2q_dk8_G2Xi03iUWABLUCWaCtCumUUKzKHBpAnWVcGlUXfHzWaiZRW15yVaDAKmNCV1xLEMqKOXm8yl7c52ffnKwf8imF_JLCiHi6Is6---pdiPmh6_1oPuTADDPaSATxB1j0Xug</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2080878452</pqid></control><display><type>article</type><title>Analytic study of the effect of dark energy-dark matter interaction on the growth of structures</title><source>arXiv.org</source><source>Free E- Journals</source><creator>Marcondes, Rafael J F ; Landim, Ricardo C G ; Costa, André A ; Wang, Bin ; Abdalla, Elcio</creator><creatorcontrib>Marcondes, Rafael J F ; Landim, Ricardo C G ; Costa, André A ; Wang, Bin ; Abdalla, Elcio</creatorcontrib><description>Large-scale structure has been shown as a promising cosmic probe for distinguishing and constraining dark energy models. Using the growth index parametrization, we obtain an analytic formula for the growth rate of structures in a coupled dark energy model in which the exchange of energy-momentum is proportional to the dark energy density. We find that the evolution of \(f \sigma_8\) can be determined analytically once we know the coupling, the dark energy equation of state, the present value of the dark energy density parameter and the current mean amplitude of dark matter fluctuations. After correcting the growth function for the correspondence with the velocity field through the continuity equation in the interacting model, we use our analytic result to compare the model's predictions with large-scale structure observations.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.1605.05264</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Continuity equation ; Dark energy ; Dark matter ; Equations of state ; Flux density ; Large scale structure of the universe ; Parameterization ; Physics - Cosmology and Nongalactic Astrophysics ; Physics - General Relativity and Quantum Cosmology ; Variation ; Velocity distribution</subject><ispartof>arXiv.org, 2016-10</ispartof><rights>2016. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,780,881,27902</link.rule.ids><backlink>$$Uhttps://doi.org/10.48550/arXiv.1605.05264$$DView paper in arXiv$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.1088/1475-7516/2016/12/009$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink></links><search><creatorcontrib>Marcondes, Rafael J F</creatorcontrib><creatorcontrib>Landim, Ricardo C G</creatorcontrib><creatorcontrib>Costa, André A</creatorcontrib><creatorcontrib>Wang, Bin</creatorcontrib><creatorcontrib>Abdalla, Elcio</creatorcontrib><title>Analytic study of the effect of dark energy-dark matter interaction on the growth of structures</title><title>arXiv.org</title><description>Large-scale structure has been shown as a promising cosmic probe for distinguishing and constraining dark energy models. Using the growth index parametrization, we obtain an analytic formula for the growth rate of structures in a coupled dark energy model in which the exchange of energy-momentum is proportional to the dark energy density. We find that the evolution of \(f \sigma_8\) can be determined analytically once we know the coupling, the dark energy equation of state, the present value of the dark energy density parameter and the current mean amplitude of dark matter fluctuations. After correcting the growth function for the correspondence with the velocity field through the continuity equation in the interacting model, we use our analytic result to compare the model's predictions with large-scale structure observations.</description><subject>Continuity equation</subject><subject>Dark energy</subject><subject>Dark matter</subject><subject>Equations of state</subject><subject>Flux density</subject><subject>Large scale structure of the universe</subject><subject>Parameterization</subject><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><subject>Physics - General Relativity and Quantum Cosmology</subject><subject>Variation</subject><subject>Velocity distribution</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><sourceid>GOX</sourceid><recordid>eNotUMtqwzAQFIVCQ5oP6KmCnu1KK60kH0PoIxDoJXcj23LiNLFTSW7rv6-dFJZ9wMywM4Q8cJZKg8ierf9tvlOuGKYMQckbMgMheGIkwB1ZhHBgjIHSgChmJF-29jjEpqQh9tVAu5rGvaOurl0Zp6uy_pO61vndkFz2k43Redq0Y7dlbLqWjjWRdr77ifuJFKLvy9h7F-7JbW2PwS3-55xsX1-2q_dk8_G2Xi03iUWABLUCWaCtCumUUKzKHBpAnWVcGlUXfHzWaiZRW15yVaDAKmNCV1xLEMqKOXm8yl7c52ffnKwf8imF_JLCiHi6Is6---pdiPmh6_1oPuTADDPaSATxB1j0Xug</recordid><startdate>20161020</startdate><enddate>20161020</enddate><creator>Marcondes, Rafael J F</creator><creator>Landim, Ricardo C G</creator><creator>Costa, André A</creator><creator>Wang, Bin</creator><creator>Abdalla, Elcio</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>GOX</scope></search><sort><creationdate>20161020</creationdate><title>Analytic study of the effect of dark energy-dark matter interaction on the growth of structures</title><author>Marcondes, Rafael J F ; Landim, Ricardo C G ; Costa, André A ; Wang, Bin ; Abdalla, Elcio</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a522-57624b5adb4e6360d9e58257991486fb1255a70457a1c16b535d9037d174236a3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2016</creationdate><topic>Continuity equation</topic><topic>Dark energy</topic><topic>Dark matter</topic><topic>Equations of state</topic><topic>Flux density</topic><topic>Large scale structure of the universe</topic><topic>Parameterization</topic><topic>Physics - Cosmology and Nongalactic Astrophysics</topic><topic>Physics - General Relativity and Quantum Cosmology</topic><topic>Variation</topic><topic>Velocity distribution</topic><toplevel>online_resources</toplevel><creatorcontrib>Marcondes, Rafael J F</creatorcontrib><creatorcontrib>Landim, Ricardo C G</creatorcontrib><creatorcontrib>Costa, André A</creatorcontrib><creatorcontrib>Wang, Bin</creatorcontrib><creatorcontrib>Abdalla, Elcio</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science &amp; Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection><collection>arXiv.org</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Marcondes, Rafael J F</au><au>Landim, Ricardo C G</au><au>Costa, André A</au><au>Wang, Bin</au><au>Abdalla, Elcio</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Analytic study of the effect of dark energy-dark matter interaction on the growth of structures</atitle><jtitle>arXiv.org</jtitle><date>2016-10-20</date><risdate>2016</risdate><eissn>2331-8422</eissn><abstract>Large-scale structure has been shown as a promising cosmic probe for distinguishing and constraining dark energy models. Using the growth index parametrization, we obtain an analytic formula for the growth rate of structures in a coupled dark energy model in which the exchange of energy-momentum is proportional to the dark energy density. We find that the evolution of \(f \sigma_8\) can be determined analytically once we know the coupling, the dark energy equation of state, the present value of the dark energy density parameter and the current mean amplitude of dark matter fluctuations. After correcting the growth function for the correspondence with the velocity field through the continuity equation in the interacting model, we use our analytic result to compare the model's predictions with large-scale structure observations.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1605.05264</doi><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier EISSN: 2331-8422
ispartof arXiv.org, 2016-10
issn 2331-8422
language eng
recordid cdi_arxiv_primary_1605_05264
source arXiv.org; Free E- Journals
subjects Continuity equation
Dark energy
Dark matter
Equations of state
Flux density
Large scale structure of the universe
Parameterization
Physics - Cosmology and Nongalactic Astrophysics
Physics - General Relativity and Quantum Cosmology
Variation
Velocity distribution
title Analytic study of the effect of dark energy-dark matter interaction on the growth of structures
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-28T11%3A51%3A14IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_arxiv&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Analytic%20study%20of%20the%20effect%20of%20dark%20energy-dark%20matter%20interaction%20on%20the%20growth%20of%20structures&rft.jtitle=arXiv.org&rft.au=Marcondes,%20Rafael%20J%20F&rft.date=2016-10-20&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.1605.05264&rft_dat=%3Cproquest_arxiv%3E2080878452%3C/proquest_arxiv%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2080878452&rft_id=info:pmid/&rfr_iscdi=true