Zobrazeno 1 - 10
of 46
pro vyhledávání: '"J. C. T. Oliveira"'
Publikováno v:
Journal of Physics: Conference Series. 1291:012038
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cf24c41713c39d99a4a7829916633189
https://doi.org/10.1088/1742-6596/1291/1/012038
https://doi.org/10.1088/1742-6596/1291/1/012038
Publikováno v:
International Journal of Modern Physics D. 19:1541-1544
In the present work we study the equation of state for asymmetric hadronic matter, to be applied in neutron star structure calculation. The delta-rich hadronic stellar matter condensate is studied in the context of mean-field approximation in an exte
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dd9f39486a340c255df7cc6c547c91ab
https://doi.org/10.1142/s0218271810017585
https://doi.org/10.1142/s0218271810017585
Publikováno v:
International Journal of Modern Physics D. 19:1447-1454
This work shows results for the EXO 0748-676 neutron star structure obtained with the use of a phenomenological quark matter description by taking into account a quark interaction, and observing the asymptotic freedom and the confinement characterist
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6b4e0a8214aac321aeebb5ccd1da03b2
https://doi.org/10.1142/s0218271810017500
https://doi.org/10.1142/s0218271810017500
Publikováno v:
Nuclear Physics B - Proceedings Supplements. 199:333-336
Recently reported massive compact stars ( M ∼ 2 M ⊙ ) have provided strong constraints on the properties of the ultradense matter beyond the saturation nuclear density. Therefore, realistic quark or hybrid star models must be compatible with thes
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::15379b0a936730877acfbee25b1fcd40
https://doi.org/10.1016/j.nuclphysbps.2010.02.054
https://doi.org/10.1016/j.nuclphysbps.2010.02.054
Publikováno v:
International Journal of Modern Physics D. 17:737-746
The color–flavor locked (CFL) phase is believed to be the fundamental state of strange quark matter (SQM) at high densities. The CFL phase is a color superconductor composed of pairs of u, d and s quarks, with no electrons, forming a Bose condensat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::64bbe952bb2ac223491b09519af46e36
https://doi.org/10.1142/s021827180801253x
https://doi.org/10.1142/s021827180801253x
Publikováno v:
International Journal of Modern Physics: Conference Series. 45:1760034
In this work we have obtained the equation of state to the highly asymmetric dense stellar matter, using the nonlinear Walecka model in the mean field approximation. We discussed the implication of changes in coupling constant of the delta baryonic r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::87db61b16236d498e9dc9fd75d255055
https://doi.org/10.1142/s2010194517600345
https://doi.org/10.1142/s2010194517600345
Publikováno v:
Revista Brasileira de Ensino de Física, Vol 26, Iss 2, Pp 93-98
Neste trabalho, apresentamos quatro deduções conhecidas da equação E = mc², incluindo a original. Relacionamos os conceitos físicos e as ferramentas matemáticas utilizados em cada caso e comparamos as deduções. Após a análise, verificamos
Externí odkaz:
https://doaj.org/article/0626e131e7004812bb9e782de5cc29bc
Publikováno v:
AIP Conference Proceedings.
In the present work we determine the equation of state of delta‐resonance‐rich stellar matter and discuss the effects of the baryon‐meson coupling constants on the delta population in the stellar medium. We extended the non‐linear Walecka (NL
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::29a7d3f2c7d09650fd8153938b7e86a8
https://doi.org/10.1063/1.3608939
https://doi.org/10.1063/1.3608939
Publikováno v:
Astronomy and Relativistic Astrophysics.
The static spherically symmetric quark star structure is calculated by using an equation of state which takes into account the superconducting Color-Flavor Locked (CFL) phase of the strange quark matter. Some fundamental aspects of QCD (asymptotic fr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5ed6ff9f2cfdec78593517693f2e185e
https://doi.org/10.1142/9789814304887_0015
https://doi.org/10.1142/9789814304887_0015
Autor:
R. S. Costa, J. C. T. Oliveira, H. Rodrigues, M. Chiapparini, S. B. Duarte, A. Deppman, C. Krug, G. S. Zahn, J. L. Rios, N. Added, V. S. Timoteo
Publikováno v:
AIP Conference Proceedings.
We study the nuclear matter properties in the regime of high temperatures using a relativistic mean‐field theory. Contrasting with the usual linear Walecka model [1], we include the σ‐ω meson coupling [2] in order to investigate the role of thi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c3af701395edd7cc6861e0cd41436c31
https://doi.org/10.1063/1.3448000
https://doi.org/10.1063/1.3448000