| dc.contributor | Universidade Estadual Paulista (UNESP) | |
| dc.creator | Krein, G. | |
| dc.date | 2014-05-20T14:07:44Z | |
| dc.date | 2016-10-25T17:12:59Z | |
| dc.date | 2014-05-20T14:07:44Z | |
| dc.date | 2016-10-25T17:12:59Z | |
| dc.date | 2003-11-01 | |
| dc.date.accessioned | 2017-04-05T21:42:36Z | |
| dc.date.available | 2017-04-05T21:42:36Z | |
| dc.identifier | European Physical Journal A. New York: Springer-verlag, v. 18, n. 2-3, p. 511-513, 2003. | |
| dc.identifier | 1434-6001 | |
| dc.identifier | http://hdl.handle.net/11449/23788 | |
| dc.identifier | http://acervodigital.unesp.br/handle/11449/23788 | |
| dc.identifier | 10.1140/epja/i2002-10272-8 | |
| dc.identifier | WOS:000186890000089 | |
| dc.identifier | http://dx.doi.org/10.1140/epja/i2002-10272-8 | |
| dc.identifier.uri | http://repositorioslatinoamericanos.uchile.cl/handle/2250/868831 | |
| dc.description | Chiral-symmetry restoration is usually discussed in the context of quark matter, a system of deconfined quarks. However, many systems like stable nuclei and neutron stars have quarks confined within nucleons. In the present paper we use a Fermi sea of three-quark clusters instead of a Fermi sea of deconfined quarks to investigate the in-medium quark condensate. We find that an enhancement of the chiral breaking in clustered matter as claimed in the literature is not a consequence of the clustering but rather dependent on the microscopic model dynamics. | |
| dc.language | eng | |
| dc.publisher | Springer | |
| dc.relation | European Physical Journal A | |
| dc.rights | info:eu-repo/semantics/closedAccess | |
| dc.title | Chiral-symmetry restoration in clustered hadronic matter | |
| dc.type | Otro | |
