Al'bert Dzhazairov-kakhramanov

Astrofizicheskie S-faktory Legkikh Atomnykh Yader Al'bert Dzhazairov-kakhramanov Russian edition

V dannoy rabote, ispol'zuya supermul'tipletnuyu klasternuyu model' legkikh yader, issleduyutsya protsessy radiatsionnogo zakhvata i uprugogo rasseyaniya na legkikh atomnykh yadrakh. Privedeny rezul'taty rascheta astrofizicheskogo S-faktora radiatsionnogo zakhvata protona na deytrone v potentsial'noy klasternoy modeli, dlya utochnennykh potentsialov rd-vzaimodeystviya, vplot' do energii 1 keV. Poluchen astrofizicheskiy S-faktor radiatsionnogo rt-zakhvata pri energii do 1 keV na osnove utochnennykh potentsialov osnovnogo sostoyaniya yadra 4Ne v ramkakh potentsial'noy klasternoy modeli s zapreshchennymi sostoyaniyami i klassifikatsiey orbital'nykh sostoyaniy po skhemam Yunga. Ispol'zovana potentsial'naya klasternaya model' s zapreshchennymi sostoyaniyami dlya potentsialov, poluchennykh na osnove fazovogo analiza uprugogo 4Ne12S-rasseyaniya, dlya rascheta astrofizicheskogo S-faktora reaktsii radiatsionnogo zakhvata 12S(4Ne,gamma)16O. Dany rezul'taty rascheta astrofizicheskogo S-faktora radiatsionnogo r12S-zakhvata pri nizkikh energiyakh, poluchennye na osnove novykh potentsialov vzaimodeystviya, kotorye soglasovany s fazovym analizom uprugogo r12S-rasseyaniya.