Pisʹma v žurnal êksperimentalʹnoj i teoretičeskoj fiziki
ISSN (print): 0370-274X
Media registration certificate: ПИ № ФС 77 – 78169 от 27.03.2020
Founder: P.L. Kapitza Institute for Physical Problems of the Russian Academy of Sciences, Russian Academy of Sciences
Editor-in-Chief: Pudalov V.M
Frequency / Assess: 12 issues per year / Subscription
Included in: White List (1st level),Higher Attestation Commission list, RISC
Edição corrente
Volume 122, Nº 3-4 (2025)
- Ano: 2025
- Artigos: 21
- URL: https://rjdentistry.com/0370-274X/issue/view/14141
Edição completa
Articles
Analysis of astrophysical 30Si(n,γ)31Si reaction via the asymptotic normalization coefficient method
Resumo
This study investigates the 30Si(n,γ)31Si astrophysical reaction using the Asymptotic Normalization Coefficient (ANC) method. The squared neutron asymptotic normalization coefficients (ANCs), for the virtual decay 31Si → 30Si + n are extracted by reanalyzing the existing angular distributions of the 30Si(d,p)31Si reaction at 12.5 MeV. Both the Distorted Wave Born Approximation (DWBA) and Adiabatic Distorted Wave Approximation (ADWA) models are applied to refine the analysis. The results show improved ANC values compared to previous DWBA calculations. The squared neutron asymptotic normalization coefficient (ANC), for the ground state is found to be 32.49 ± 6 fm−1 with DWBA and 31.45 ± 6 fm−1 with ADWA. Additionally, the direct capture (DC) reaction rate was calculated and compared with previous work. The results show good agreement with the literature, with minor deviations at higher temperatures, highlighting the importance of the DC process in the 30Si(n,γ)31Si reaction. This work emphasizes the crucial role of neutron capture reactions in the formation of the weak s-process component in stars and provides new insights into reaction rates and cross-sections.
133-135
Uvelichivaet li vklad f 0 mezona veroyatnost' K + → π 0 π 0 π 0 e + ν raspada?
Resumo
136-138
Svetovye sdvigi rezonansov kogerentnogo pleneniya naselennostey v periodicheski-modulirovannom lazernom izluchenii
Resumo
139-146
Ispol'zovanie impul'sov sverkhizlucheniya dlya nakachki mnogoprokhodnykh komptonovskikh lazerov na svobodnykh elektronakh teragertsovogo diapazona
Resumo
147-152
General scaling behavior of superconductors
Resumo
153-155
Fazovye prevrashcheniya v geyzenbergovskikh magnetikakh, indutsirovannye odnoosnoy anizotropiey: modelirovanie metodami Vanga–Landau i mashinnogo obucheniya
Resumo
156-161
Effect of Coulomb correlations on the electronic structure of bulk V2Se2O: a DFT+DMFT study
Resumo
162-164
Porog generatsii kvantovykh vikhrey volnami na poverkhnosti sverkhtekuchego He-II
Resumo
165-170
Rezonansnoe neuprugoe rasseyanie rentgenovskikh luchey na Fe L2,3-krayakh pogloshcheniya oksidov SrFeOx (x = 2.46 i 2.82)
Resumo
171-176
Statisticheskie modeli barrenovskikh plato i antikontsentratsiya nablyudaemykh Pauli
Resumo
177-183
Mikroskopicheskiy mekhanizm denaturatsii belkov i nukleinovykh kislot bakteriy R. aeruginosa pri rezonansnom pogloshchenii femtosekundnykh lazernykh impul'sov s dlinoy volny 6 mkm
Resumo
184-190
O skachkakh mnogochastichnykh amplitud
Resumo
193-198
Topological origin of horizon temperature via the Chern–Gauss–Bonnet theorem
Resumo
199-200
Poluprovodnikovyy diskovyy lazer na geterostrukture GalnP/AlGalnP s vnutrirezonatornoy nakachkoy v kvantovye yamy
Resumo
201-207
Printsip virtual'nogo kozhukha v modelyakh s 2D plazmoy i 3D stenkoy v tokamake
Resumo
208-213
Effekty sil'noy turbulentnosti voln na vode
Resumo
214-219
Ustoychivost' nematicheskoy sverkhprovodimosti v Sr2Bi2Se3 k magnitnomu legirovaniyu
Resumo
220-226
Teploemkost' plotnykh zhidkostey: svyaz' mezhdu dvukhfaznoy model'yu i skeylingom po temperature plavleniya
Resumo
227-230
YaMR spinovoy kinetiki yader 169Tm v monokristalle Li(Y0.98Tm0.02)F4
Resumo
231-236
Lokal'naya termometriya cheshuyki NbSe2 putem izmereniya del'ta-T shuma
Resumo
237-246
Narushenie P- i T-simmetriy i magnitogal'vanicheskie effekty v metallicheskikh antiferromagnetikakh
Resumo
247-252


