Zobrazeno 1 - 10
of 70
pro vyhledávání: '"Prajapati, P.M."'
Publikováno v:
EPJ Web of Conferences, Vol 297, p 00001 (2024)
Externí odkaz:
https://doaj.org/article/4181aaddb77f45c3aa62ae374d0617aa
Autor:
Guruprasad, Shet, Sachin, Prajapati, P.M., Suryanarayana, S.V., Karkera, Meghna, Subbaiah, K.V., Raviprakash, Y., Shivashankar, B.S.
Publikováno v:
In Nuclear and Particle Physics Proceedings September 2023
Autor:
Shet, Sachin, Subbaiah, K.V., Prajapati, P.M., Singh, Kapil Deo, Anand, S., Suryanarayna, S.V.
Publikováno v:
In Nuclear and Particle Physics Proceedings July 2023
Autor:
Hingu, Akash, Soni, Bhargav, Parashari, Siddharth, Makwana, Rajnikant, Prajapati, P.M., Vashi, Vibhuti, Mehta, Mayur, Palit, R., Suryanarayana, S.V., Nayak, B.K., Katovsky, K., Mukherjee, S.
Publikováno v:
In Radiation Physics and Chemistry October 2022 199
Autor:
Prajapati, P.M.1 pareshkumar.p@manipal.edu, Qureshi, Mahin2, Hingu, A.2, Pizzone, R.G.3, La Cognata, M.3, Suryanarayna, S.V.1,4, Shet, Sachin1, Mukherjee, S.5
Publikováno v:
EPJ Web of Conferences. 2/3/2023, Vol. 275, p1-4. 4p.
Publikováno v:
EPJ Web of Conferences, Vol 275, p 02017 (2023)
Externí odkaz:
https://doaj.org/article/e1ce484c9fbd4bb5915deebfe991f292
Publikováno v:
EPJ Web of Conferences, Vol 275, p 02006 (2023)
Abstract. Low energy proton capture cross sections on heavy isotopes are necessary for a better understanding of the astrophysical p-process. There are around 35 proton-rich stable isotopes between 74S e and 196Hg which are bypassed by the s- and r-
Externí odkaz:
https://doaj.org/article/d3f1055da61e471ca67239d7a43fe488
Autor:
Prajapati P.M., Qureshi Mahin, Hingu A., Pizzone R.G., La Cognata M., Suryanarayna S.V., Shet Sachin, Mukherjee S.
Publikováno v:
EPJ Web of Conferences, Vol 275, p 02014 (2023)
The 13C(α, n)16O reaction operates in the He intershell of low-mass(M < 4 M⊙) AGB stars and it is the neutron source that allows the creation of the main component of the s-process elements. The reaction rate is then required to be well known in t
Externí odkaz:
https://doaj.org/article/232686c7f83643e7a5c63397ba75fabd
Autor:
Hingu, Akash1 hinguaakash@gmail.com, Prajapati, P.M.2,3 pareshkumar.p@manipal.edu, Mukherjee, S.1,4 sk.mukherjee-phy@msubaroda.ac.in, Pizzone, R.G.3, Katovsky, K.5
Publikováno v:
EPJ Web of Conferences. 2/3/2023, Vol. 275, p1-3. 3p.
Autor:
Spampinato C., Pizzone R.G., Spartà R., Couder M., Tan W., Burian V., Chae K.Y., D’Agata G., Guardo G.L., Indelicato I., Cognata M. La, Lamia L., Lattuada D., Mrazek J., Oliva A., Palmerini S., Prajapati P.M., Rapisarda G.G., Romano S., Sergi M.L., Spitaleri C., Tumino A., Wiescher M., Anguilar S., Bardyan D., Blankstein D., Boccioli L., Callahan L., Clark A., Frentz B., Hall M., Gula A., Henderson S., Kelmar R., Liu Q., Long J., Majumdar A., McGuinness S., Nelson A., O’Malley P., Seyymour C., Skulski M., Wilkinson J.
Publikováno v:
EPJ Web of Conferences, Vol 227, p 02013 (2020)
In the network of reactions present in the Big Bang nucleosynthesis, the 3He(n, p)3H has an important role which impacts the final 7Li abundance. The Trojan Horse Method (THM) has been applied to the 3He(d, pt)H reaction in order to extract the astro
Externí odkaz:
https://doaj.org/article/06bbca1ae6f3443fa3c99858b8c6a6b1