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pro vyhledávání: '"Pais, H"'
In this work, we study the effect of including a resonant state of four neutrons in the low-density warm nuclear equation of state, using a relativistic mean-field formalism, where in-medium effects are considered. For that purpose, the abundances of
Externí odkaz:
http://arxiv.org/abs/2409.18232
Detailed assessments of the ability of recent theoretical approaches to modeling existing experimental data for ternary fission confirm earlier indications that the dominant mode of cluster formation in ternary fission is clusterization in very neutr
Externí odkaz:
http://arxiv.org/abs/2211.13492
Autor:
Typel, S., Oertel, M., Klähn, T., Chatterjee, D., Dexheimer, V., Ishizuka, C., Mancini, M., Novak, J., Pais, H., Providencia, C., Raduta, A., Servillat, M., Tolos, L.
CompOSE (CompStar Online Supernovae Equations of State) is an online repository of equations of state (EoS) for use in nuclear physics and astrophysics, e.g., in the description of compact stars or the simulation of core-collapse supernovae and neutr
Externí odkaz:
http://arxiv.org/abs/2203.03209
Publikováno v:
Eur. Phys. J. A (2021) 57:262
Chemical constants extracted from $^{124}$Xe+ $^{124}$Sn collisions at 32 AMeV are compared to the predictions of an extended Nuclear Statistical Equilibrium model including mean-field interactions and in-medium binding energy shifts for the light ($
Externí odkaz:
http://arxiv.org/abs/2109.02961
Publikováno v:
Phys. Rev. C 103, 061601 (2021)
Ternary fission of actinides probes the state of the nucleus at scission. Light clusters are produced in space and time very close to the scission point. Within the nonequilibrium statistical operator method, a generalized Gibbs distribution is const
Externí odkaz:
http://arxiv.org/abs/2012.14691
Publikováno v:
Phys. Rev. C 102, 064621 (2020)
Yields of equatorially emitted light isotopes, $1\le Z\le 14$, observed in ternary fission in the reaction $^{241}$Pu($n_{\rm th}$,f) are employed to determine apparent chemical equilibrium constants for low-temperature and low-density nuclear matter
Externí odkaz:
http://arxiv.org/abs/2009.05200
The yields of light elements ($Z=1,2$) obtained from spontaneous ternary fission of $^{252}$Cf are treated within a nonequilibrium approach, and the contribution of unstable nuclei and excited bound states is taken into account. These light cluster y
Externí odkaz:
http://arxiv.org/abs/2008.06321
Akademický článek
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Publikováno v:
Phys. Rev. C 95, 055808 (2017)
The spinodal instabilities in hot asymmetric nuclear matter and some important critical parameters derived thereof are studied using six different families of relativistic mean-field (RMF) models. The slopes of the symmetry energy coefficient vary ov
Externí odkaz:
http://arxiv.org/abs/1705.02096
Autor:
Alam, N., Agrawal, B. K., Fortin, M., Pais, H., Providência, C., Raduta, Ad. R., Sulaksono, A.
Publikováno v:
Phys. Rev. C 94, 052801 (2016)
We examine the correlations of neutron star radii with the nuclear matter incompressibility, symmetry energy, and their slopes, which are the key parameters of the equation of state (EoS) of asymmetric nuclear matter. The neutron star radii and the E
Externí odkaz:
http://arxiv.org/abs/1610.06344