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pro vyhledávání: '"V.N. Kondratyev"'
Autor:
V.N. Kondratyev
Publikováno v:
Particles, Vol 3, Iss 2, Pp 272-277 (2020)
The properties and mass distribution of the ultramagnetized atomic nuclei which arise in heavy-ion collisions and magnetar crusts, during Type II supernova explosions and neutron star mergers are analyzed. For the magnetic field strength range of 0.1
Externí odkaz:
https://doaj.org/article/0df5885442e8424984f75ed07ee4e129
Autor:
V.N. Kondratyev
Publikováno v:
Physics Letters B, Vol 782, Iss , Pp 167-169 (2018)
Properties and mass distribution of ultramagnetized atomic nuclei that arise in heavy-ion collisions, magnetar crusts, during Type II supernova explosions and neutron star mergers are analyzed. For magnetic field strength range 0.1–10 teratesla the
Externí odkaz:
https://doaj.org/article/74bcb497aaa64b41956f96d2fd504d53
Akademický článek
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Akademický článek
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Autor:
V.N. Kondratyev
Publikováno v:
Physics of Particles and Nuclei. 50:576-580
Ultramagnetized atomic nuclei created in supernova explosions, neutron star mergers, magnetar crusts and heavy ion collisions are considered. It is shown that for field strengths of 0.1–10 teratesla, the linear magnetic response dominates and the Z
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d6373a84195e4d6e13d5e3963f60ef00
https://doi.org/10.1134/s1063779619050149
https://doi.org/10.1134/s1063779619050149
Autor:
V.N. Kondratyev
Publikováno v:
Physics of Atomic Nuclei. 81:890-893
Nuclear structure and composition in ultra-strong magnetic fields relevant for heavy-ion collisions, supernovae, andmagnetar crusts are analyzed. For field intensities exceeding 0.1 teratesla (TT) nuclear magnetic response is represented as combined
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b0f660d76e264363cefe568abede33e3
https://doi.org/10.1134/s1063778818060224
https://doi.org/10.1134/s1063778818060224
Autor:
V.N. Kondratyev
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 480:5380-5383
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b7528f4b41d4e24849639450f201e124
https://doi.org/10.1093/mnras/sty2248
https://doi.org/10.1093/mnras/sty2248
Autor:
V.N. Kondratyev
Publikováno v:
Physics of Particles and Nuclei. 50:613-615
Soft repeating gamma-ray (SGR) bursts are considered as magnetoemission of crusts of magnetars (ultramagnetized neutron stars). It is shown that all the observations of such bursts can be described and systematized within a randomly jumping interacti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8a8d7f2ee28c1a3ef0ed707dce58dd79
https://doi.org/10.1134/s1063779619050150
https://doi.org/10.1134/s1063779619050150
Autor:
V.N. Kondratyev, Yu. V. Korovina
Publikováno v:
Physics of Particles and Nuclei. 49:105-108
Soft gamma repeater (SGR) bursts are considered as a release of magnetic energy stored in the baryon degrees of freedom of the magnetar crust. It is shown that this interpretation allows all observations of these bursts to be systematized and univers
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0368d96c727732913011ec9c1b4479ef
https://doi.org/10.1134/s1063779618010240
https://doi.org/10.1134/s1063779618010240
Autor:
V.N. Kondratyev, Yu. V. Korovina
Publikováno v:
Physics of Atomic Nuclei. 80:558-561
The magnetoemission of crusts of magnetars (ultramagnetized neutron stars) is considered as an origin of repeated soft gamma-ray bursts. It is shown that all observations of such bursts can be described and systematized on the basis of amodel of rand
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::02e5b3688dfd29cef7682ba23d363850
https://doi.org/10.1134/s1063778817030139
https://doi.org/10.1134/s1063778817030139