Finite temperature Z( N) phase transition with Kaluza–Klein gauge fields
If SU( N) gauge fields live in a world with a circular extra dimension, coupling there only to adjointly charged matter, the system possesses a global Z( N) symmetry. If the radius is small enough such that dimensional reduction takes place, this symmetry is spontaneously broken. It turns out that i...
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Veröffentlicht in: | Nuclear physics. B 2003-04, Vol.655 (1), p.170-184 |
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container_title | Nuclear physics. B |
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creator | Farakos, K. de Forcrand, P. Korthals Altes, C.P. Laine, M. Vettorazzo, M. |
description | If SU(
N) gauge fields live in a world with a circular extra dimension, coupling there only to adjointly charged matter, the system possesses a global Z(
N) symmetry. If the radius is small enough such that dimensional reduction takes place, this symmetry is spontaneously broken. It turns out that its fate at high temperatures is not easily decided with straightforward perturbation theory. Utilising non-perturbative lattice simulations, we demonstrate here that the symmetry does get restored at a certain temperature
T
c
, both for a (3+1)- and a (4+1)-dimensional world (the latter with a finite cutoff). To avoid a cosmological domain wall problem, such models would thus be allowed only if the reheating temperature after inflation is below
T
c
. We also comment on the robustness of this phenomenon with respect to small modifications of the model. |
doi_str_mv | 10.1016/S0550-3213(03)00067-1 |
format | Article |
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N) gauge fields live in a world with a circular extra dimension, coupling there only to adjointly charged matter, the system possesses a global Z(
N) symmetry. If the radius is small enough such that dimensional reduction takes place, this symmetry is spontaneously broken. It turns out that its fate at high temperatures is not easily decided with straightforward perturbation theory. Utilising non-perturbative lattice simulations, we demonstrate here that the symmetry does get restored at a certain temperature
T
c
, both for a (3+1)- and a (4+1)-dimensional world (the latter with a finite cutoff). To avoid a cosmological domain wall problem, such models would thus be allowed only if the reheating temperature after inflation is below
T
c
. We also comment on the robustness of this phenomenon with respect to small modifications of the model.</description><identifier>ISSN: 0550-3213</identifier><identifier>EISSN: 1873-1562</identifier><identifier>DOI: 10.1016/S0550-3213(03)00067-1</identifier><language>eng</language><publisher>Elsevier B.V</publisher><subject>High Energy Physics - Phenomenology ; Physics</subject><ispartof>Nuclear physics. B, 2003-04, Vol.655 (1), p.170-184</ispartof><rights>2003 Elsevier Science B.V.</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c423t-4a1c80d23f56a0ef7ecde32cf1cf014303c1415004e12630d2328ca109b560f3</citedby><cites>FETCH-LOGICAL-c423t-4a1c80d23f56a0ef7ecde32cf1cf014303c1415004e12630d2328ca109b560f3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://dx.doi.org/10.1016/S0550-3213(03)00067-1$$EHTML$$P50$$Gelsevier$$H</linktohtml><link.rule.ids>230,314,778,782,883,3539,27907,27908,45978</link.rule.ids><backlink>$$Uhttps://hal.science/hal-00008374$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Farakos, K.</creatorcontrib><creatorcontrib>de Forcrand, P.</creatorcontrib><creatorcontrib>Korthals Altes, C.P.</creatorcontrib><creatorcontrib>Laine, M.</creatorcontrib><creatorcontrib>Vettorazzo, M.</creatorcontrib><title>Finite temperature Z( N) phase transition with Kaluza–Klein gauge fields</title><title>Nuclear physics. B</title><description>If SU(
N) gauge fields live in a world with a circular extra dimension, coupling there only to adjointly charged matter, the system possesses a global Z(
N) symmetry. If the radius is small enough such that dimensional reduction takes place, this symmetry is spontaneously broken. It turns out that its fate at high temperatures is not easily decided with straightforward perturbation theory. Utilising non-perturbative lattice simulations, we demonstrate here that the symmetry does get restored at a certain temperature
T
c
, both for a (3+1)- and a (4+1)-dimensional world (the latter with a finite cutoff). To avoid a cosmological domain wall problem, such models would thus be allowed only if the reheating temperature after inflation is below
T
c
. We also comment on the robustness of this phenomenon with respect to small modifications of the model.</description><subject>High Energy Physics - Phenomenology</subject><subject>Physics</subject><issn>0550-3213</issn><issn>1873-1562</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2003</creationdate><recordtype>article</recordtype><recordid>eNqFkM1KAzEUhYMoWKuPIGTZLkbvncyfKylirbbowq7chJi5aSPTmZJMK7ryHXxDn8SmlW5dXTh858D9GDtHuEDA7PIZ0hQiEaPogegDQJZHeMA6WOQiwjSLD1lnjxyzE-_fIFCi6LCHoa1tS7ylxZKcaleO-EuPP_b5cq78Jneq9ra1Tc3fbTvnY1WtPtXP1_e4IlvzmVrNiBtLVelP2ZFRlaezv9tl0-Ht9GYUTZ7u7m8Gk0gnsWijRKEuoIyFSTMFZHLSJYlYG9QGMBEgNCaYAiSEcSYCGRdaIVy9phkY0WX93excVXLp7EK5D9koK0eDiQxZ-K0QebLGDZvuWO0a7x2ZfQFBBndy604GMRKE3LqToXe969Hmj7UlJ722VGsqrSPdyrKx_yz8AmK6dQo</recordid><startdate>20030407</startdate><enddate>20030407</enddate><creator>Farakos, K.</creator><creator>de Forcrand, P.</creator><creator>Korthals Altes, C.P.</creator><creator>Laine, M.</creator><creator>Vettorazzo, M.</creator><general>Elsevier B.V</general><general>North-Holland ; Elsevier [1967-....]</general><scope>AAYXX</scope><scope>CITATION</scope><scope>1XC</scope></search><sort><creationdate>20030407</creationdate><title>Finite temperature Z( N) phase transition with Kaluza–Klein gauge fields</title><author>Farakos, K. ; de Forcrand, P. ; Korthals Altes, C.P. ; Laine, M. ; Vettorazzo, M.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c423t-4a1c80d23f56a0ef7ecde32cf1cf014303c1415004e12630d2328ca109b560f3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2003</creationdate><topic>High Energy Physics - Phenomenology</topic><topic>Physics</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Farakos, K.</creatorcontrib><creatorcontrib>de Forcrand, P.</creatorcontrib><creatorcontrib>Korthals Altes, C.P.</creatorcontrib><creatorcontrib>Laine, M.</creatorcontrib><creatorcontrib>Vettorazzo, M.</creatorcontrib><collection>CrossRef</collection><collection>Hyper Article en Ligne (HAL)</collection><jtitle>Nuclear physics. B</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Farakos, K.</au><au>de Forcrand, P.</au><au>Korthals Altes, C.P.</au><au>Laine, M.</au><au>Vettorazzo, M.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Finite temperature Z( N) phase transition with Kaluza–Klein gauge fields</atitle><jtitle>Nuclear physics. B</jtitle><date>2003-04-07</date><risdate>2003</risdate><volume>655</volume><issue>1</issue><spage>170</spage><epage>184</epage><pages>170-184</pages><issn>0550-3213</issn><eissn>1873-1562</eissn><abstract>If SU(
N) gauge fields live in a world with a circular extra dimension, coupling there only to adjointly charged matter, the system possesses a global Z(
N) symmetry. If the radius is small enough such that dimensional reduction takes place, this symmetry is spontaneously broken. It turns out that its fate at high temperatures is not easily decided with straightforward perturbation theory. Utilising non-perturbative lattice simulations, we demonstrate here that the symmetry does get restored at a certain temperature
T
c
, both for a (3+1)- and a (4+1)-dimensional world (the latter with a finite cutoff). To avoid a cosmological domain wall problem, such models would thus be allowed only if the reheating temperature after inflation is below
T
c
. We also comment on the robustness of this phenomenon with respect to small modifications of the model.</abstract><pub>Elsevier B.V</pub><doi>10.1016/S0550-3213(03)00067-1</doi><tpages>15</tpages><oa>free_for_read</oa></addata></record> |
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source | Elsevier ScienceDirect Journals Complete - AutoHoldings |
subjects | High Energy Physics - Phenomenology Physics |
title | Finite temperature Z( N) phase transition with Kaluza–Klein gauge fields |
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