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dc.date.accessioned 2020-06-26T14:01:49Z
dc.date.available 2020-06-26T14:01:49Z
dc.date.issued 2017-12
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/99235
dc.description.abstract We study the behavior of strongly interacting matter under a uniform intense external magnetic field in the context of nonlocal extensions of the Polyakov-Nambu-Jona-Lasinio model. A detailed description of the formalism is presented, considering the cases of zero and finite temperature. In particular, we analyze the effect of the magnetic field on the chiral restoration and deconfinement transitions, which are found to occur at approximately the same critical temperatures. Our results show that these models offer a natural framework to account for the phenomenon of inverse magnetic catalysis found in lattice QCD calculations.
dc.language en es
dc.subject Quantum chromodynamics es
dc.subject Relativistic quark model es
dc.subject Chiral symmetry es
dc.title Strong magnetic fields in nonlocal chiral quark models en
dc.type Articulo es
sedici.identifier.uri https://ri.conicet.gov.ar/11336/50047 es
sedici.identifier.other http://dx.doi.org/10.1103/PhysRevD.96.114012 es
sedici.identifier.other hdl:11336/50047 es
sedici.identifier.issn 2470-0029 es
sedici.creator.person Gómez Dumm, Daniel Alberto es
sedici.creator.person Izzo Villafañe, María Florencia es
sedici.creator.person Noguera, S. es
sedici.creator.person Pagura, Valeria Paula es
sedici.creator.person Scoccola, Norberto Nerio es
sedici.subject.materias Física es
sedici.description.fulltext true es
mods.originInfo.place Instituto de Física La Plata es
mods.originInfo.place Consejo Nacional de Investigaciones Científicas y Técnicas es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Physical Review D es
sedici.relation.journalVolumeAndIssue vol. 96, no. 11 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)