Zobrazeno 1 - 10
of 11
pro vyhledávání: '"Amrit Pattnaik"'
Publikováno v:
U.Porto Journal of Engineering, Vol 9, Iss 4, Pp 20-50 (2023)
Power quality is the manifestation of a disruption in the supply voltage, current or frequency that damages the utility equipment and has become an important issue with the introduction of more sophisticated and sensitive devices. So, the supply powe
Externí odkaz:
https://doaj.org/article/c3c175f9b30c461d87ec2815219fb884
Publikováno v:
Foundations; Volume 2; Issue 4; Pages: 898-911
The present study is focused on revealing a characteristic kink of the neutron shell closure N = 126 across the Hg-isotopic chain within the relativistic mean-field (RMF) approach with the IOPB-I, DD-ME2, DD-PC1 and NL3 parameter sets. The RMF densit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d1e6f9ba7eaf93ced861ad27c2011748
https://doi.org/10.3390/foundations2040061
https://doi.org/10.3390/foundations2040061
Publikováno v:
Canadian Journal of Physics. 100:102-111
We have systematically studied the surface properties, such as symmetry energy, neutron pressure, and symmetry energy curvature coefficient for Ne, Na, Mg, Al, and Si nuclei from the proton to neutron drip lines. The coherent density fluctuation mode
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1ed65570ec0f25f970d4351cdb5afd24
https://doi.org/10.1139/cjp-2021-0231
https://doi.org/10.1139/cjp-2021-0231
The anisotropy of pressure arises due to the various complex phenomena that happen inside the neutron star (NS). In this study, we calculate the degree of anisotropy inside the NS using the scalar pressure anisotropy model. Macroscopic properties suc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fdb119394456c0fba1c12509a5a1368c
Publikováno v:
Physical Review C. 105
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::83730ea6be6b774ce043124c8ad1579f
https://doi.org/10.1103/physrevc.105.014318
https://doi.org/10.1103/physrevc.105.014318
[Background] In our earlier work {\bf [Phys. Rev. C 104, 055804 (2021)]}, we studied the surface properties of a neutron star, assuming it as a huge finite nucleus containing protons, neutrons, electrons, and muons. For the first time, we reported th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::30515cc3299778b00a606a425755fdfd
Based on the current measurement of the neutron distribution radius ($R_n$) of $^{208}$Pb through the PREX-2 data, we re-visited the recently developed G3 and IOPB-I force parameter by fine-tuning some of the specific couplings within the relativisti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b69edbd85c3cc84ae96c2299c3323a02
Publikováno v:
Physica Scripta. 96:125319
The ground-state properties such as binding energy, root-mean-square radius, pairing energy, nucleons density distribution, symmetry energy, and single-particle energies are calculated for the isotopic chain of Ca, Sn, Pb, and Z = 120 nuclei. The rec
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a1249c35fd56bc14f626528ba09aa583
https://doi.org/10.1088/1402-4896/ac3a4d
https://doi.org/10.1088/1402-4896/ac3a4d
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