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| 001 | 59365 | ||
| 005 | 20240610121225.0 | ||
| 024 | 7 | _ | |a 10.1140/epja/i2007-10390-9 |2 DOI |
| 024 | 7 | _ | |a WOS:000247244600007 |2 WOS |
| 024 | 7 | _ | |a arXiv:0705.1603 |c nucl-th |2 arXiv |
| 024 | 7 | _ | |a arXiv:oai:arXiv.org:0705.1603 |2 arXiv |
| 024 | 7 | _ | |a 2128/10517 |2 Handle |
| 035 | _ | _ | |a arXiv:0705.1603 |9 arXiv |c nucl-th |
| 035 | _ | _ | |a FZJ-IKP-TH-2007-17 |
| 035 | _ | _ | |a oai:arXiv.org:0705.1603 |9 arXiv |z oai:arXiv.org:0705.1603 |
| 035 | _ | _ | |9 DESY |z D07-09150 |
| 035 | _ | _ | |9 SPIRESTeX |z Meissner:2007ya |
| 037 | _ | _ | |a PreJuSER-59365 |
| 041 | _ | _ | |a eng |
| 082 | _ | _ | |a 530 |
| 084 | _ | _ | |a Physics, Nuclear |2 WoS |
| 084 | _ | _ | |a Physics, Particles & Fields |2 WoS |
| 084 | _ | _ | |a 12.39.Fe |2 PACS |
| 084 | _ | _ | |a 13.40.Gp |2 PACS |
| 084 | _ | _ | |a 21.65.+f |2 PACS |
| 100 | 1 | _ | |a Meissner, U.G. |b 0 |u FZJ |0 P:(DE-Juel1)131252 |
| 245 | _ | _ | |a Neutron-proton mass difference in isospin-asymmetric nuclear matter |
| 260 | _ | _ | |a Berlin |b Springer |c 2007 |
| 300 | _ | _ | |a 299 - 309 |
| 336 | 7 | _ | |a Journal Article |0 PUB:(DE-HGF)16 |2 PUB:(DE-HGF) |
| 336 | 7 | _ | |a Output Types/Journal article |2 DataCite |
| 336 | 7 | _ | |a Journal Article |0 0 |2 EndNote |
| 336 | 7 | _ | |a ARTICLE |2 BibTeX |
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| 336 | 7 | _ | |a article |2 DRIVER |
| 440 | _ | 0 | |a European Physical Journal A |x 1434-6001 |0 1981 |v 32 |
| 500 | _ | _ | |a Record converted from VDB: 12.11.2012 |
| 520 | _ | _ | |a Isospin-breaking effects in the baryonic sector are studied in the framework of a medium-modified Skyrme model. The neutron-proton mass difference in infinite, asymmetric nuclear matter is discussed. In order to describe the influence of the nuclear environment on the skyrmions, we include energy-dependent charged and neutral pion optical potentials in the s- and p-wave channels. The present approach predicts that the neutron-proton mass difference is mainly dictated by its strong part and that it strongly decreases in neutron matter. |
| 536 | _ | _ | |a Physik der Hadronen und Kerne |c P53 |2 G:(DE-HGF) |0 G:(DE-Juel1)FUEK413 |x 0 |
| 588 | _ | _ | |a Dataset connected to Web of Science |
| 650 | _ | 7 | |a nuclear matter |2 INSPIRE |
| 650 | _ | 7 | |a isospin: asymmetry |2 INSPIRE |
| 650 | _ | 7 | |a p n: mass difference |2 INSPIRE |
| 650 | _ | 7 | |a Skyrme model |2 INSPIRE |
| 650 | _ | 7 | |a potential: optical |2 INSPIRE |
| 650 | _ | 7 | |a effective Lagrangian |2 INSPIRE |
| 650 | _ | 7 | |a soliton |2 INSPIRE |
| 650 | _ | 7 | |a form factor: electromagnetic |2 INSPIRE |
| 650 | _ | 7 | |a numerical calculations |2 INSPIRE |
| 700 | 1 | _ | |a Rakhimov, A. M. |b 1 |0 P:(DE-HGF)0 |
| 700 | 1 | _ | |a Wirzba, A. |b 2 |u FZJ |0 P:(DE-Juel1)131377 |
| 700 | 1 | _ | |a Yakhshiev, U. T. |b 3 |u FZJ |0 P:(DE-Juel1)VDB6964 |
| 773 | _ | _ | |a 10.1140/epja/i2007-10390-9 |g Vol. 32, p. 299 - 309 |p 299 - 309 |q 32<299 - 309 |0 PERI:(DE-600)1459066-9 |t The @European physical journal / A |v 32 |y 2007 |x 1434-6001 |
| 856 | 7 | _ | |u http://dx.doi.org/10.1140/epja/i2007-10390-9 |
| 856 | 4 | _ | |u https://juser.fz-juelich.de/record/59365/files/0705.1603v2.pdf |y OpenAccess |
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| 856 | 4 | _ | |u https://juser.fz-juelich.de/record/59365/files/0705.1603v2.pdf?subformat=pdfa |x pdfa |y OpenAccess |
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| 913 | 1 | _ | |k P53 |v Physik der Hadronen und Kerne |l Physik der Hadronen und Kerne |b Struktur der Materie |0 G:(DE-Juel1)FUEK413 |x 0 |
| 914 | 1 | _ | |y 2007 |
| 915 | _ | _ | |a OpenAccess |0 StatID:(DE-HGF)0510 |2 StatID |
| 915 | _ | _ | |a JCR/ISI refereed |0 StatID:(DE-HGF)0010 |
| 920 | 1 | _ | |k IKP-3 |l Institut 3 (Theoretische Kernphysik) |d 31.12.2001 |g IKP |0 I:(DE-Juel1)VDB25 |x 1 |
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