Ushbu ishga iqtibos qilgan ishlar

6 ta ish

Ish: What Do We (Not) Know Theoretically about Solar Neutrino Fluxes?

1. Astrophysical S-factor for the 3He(α,γ)7Be reaction via the asymptotic normalization coefficient (ANC) method

   G. Kiss, M. La Cognata, C. Spitaleri +38

   MaqolaNuclear physics research studiesPhysics Letters B20205 iqtibos

   ABIABI:AkademIndex/openalex/2020.article.000135

2. Extrapolation of astrophysical S factors for the reaction 14N((p, γ) 15O to near-zero energies

   S. V. Artemov, S. B. Igamov, K. I. Tursunmakhatov +1

   MaqolaNuclear physics research studiesPhysics of Atomic Nuclei20124 iqtibos

   ABIABI:AkademIndex/openalex/2012.article.000050

3. Three-Body Treatment of the pep Reaction in the Sun

   B. F. Irgaziev, V.B. Belyaev

   MaqolaNeutrino Physics ResearchFew-Body Systems20130 iqtibos

   ABIABI:AkademIndex/openalex/2013.article.000307

4. Determination of the ³He(<i>α</i>, <i>γ</i>)⁷Be and ⁶Li(<i>p</i>, <i>γ</i>)⁷Be astrophysical factors down to zero energy using the asymptotic normalization coefficients

   M. La Cognata, G. Kiss, R. Yarmukhamedov +38

   MaqolaNuclear physics research studiesEPJ Web of Conferences20230 iqtibos

   ABIABI:AkademIndex/openalex/2023.article.005771

5. Determination of the astrophysical factor of the ³He(α,γ)⁷Be down to zero energy using the asymptotic normalization coefficient method

   M. La Cognata, G. Kiss, R. Yarmukhamedov +38

   MaqolaNuclear physics research studiesJournal of Physics Conference Series20230 iqtibos

   ABIABI:AkademIndex/openalex/2023.article.010700

6. Radiative capture of proton through the ¹⁴N(p,γ)¹⁵O reaction at low energy

   B. F. Irgaziev, Abdul Kabir, Jameel‐Un Nabi

   MaqolaAtmospheric Ozone and ClimateChinese Physics C20240 iqtibos

   ABIABI:AkademIndex/openalex/2024.article.001730