Zobrazeno 1 - 10
of 37
pro vyhledávání: '"Kundalia K."'
Autor:
Mitra R., Gupta D., Maity S., Samanta S., Kundalia K., Ali Sk M., Saha Swapan K., Tengblad O., Perea A., Martel I., Cederkall J.
Publikováno v:
EPJ Web of Conferences, Vol 297, p 02005 (2024)
The measurement of the breakup of the radioactive nucleus 7Be on 12C at 5 MeV/u is reported for the first time. Significant coincidence counts of α and 3He from 7Be breakup have been identified. Analysis is ongoing to identify the breakup events fro
Externí odkaz:
https://doaj.org/article/425e46f3c85a49418ad8e9bd4ae3d8e8
Autor:
Ali, Sk M., Gupta, D., Kundalia, K., Maity, S., Saha, Swapan K, Tengblad, O., Ovejas, J. D., Perea, A., Martel, I., Cederkall, J., Park, J., Moro, A. M.
Publikováno v:
Phys. Lett. B 853 (2024) 138673
The measurement of the $^7$Be($d$,$^3$He)$^6$Li* transfer cross section at 5 MeV/u is carried out. The population of the 2.186 MeV excited state of $^6$Li in this reaction channel is observed for the first time. The experimental angular distributions
Externí odkaz:
http://arxiv.org/abs/2405.02892
Autor:
Kundalia, K., Gupta, D., Ali, Sk M., Saha, Swapan K, Tengblad, O., Ovejas, J. D., Perea, A., Martel, I., Cederkall, J., Park, J., Szwec, S., Moro, A. M.
Publikováno v:
Physics Letters B 833(2022)137294
The elastic and inelastic scattering of $^7$Be from $^{12}$C have been measured at an incident energy of 35 MeV. The inelastic scattering leading to the 4.439 MeV excited state of $^{12}$C has been measured for the first time. The experimental data c
Externí odkaz:
http://arxiv.org/abs/2207.10865
Autor:
Ali, Sk M., Gupta, D., Kundalia, K., Saha, Swapan K., Tengblad, O., Ovejas, J. D., Perea, A., Martel, I., Cederkall, J., Park, J., Szwec, S.
Publikováno v:
Physical Review Letters 128, 252701 (2022)
The anomaly in lithium abundance is a well-known unresolved problem in nuclear astrophysics. A recent revisit to the problem tried the avenue of resonance enhancement to account for the primordial $^7$Li abundance in standard big-bang nucleosynthesis
Externí odkaz:
http://arxiv.org/abs/2206.14563
Akademický článek
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Autor:
Mitra, R., Gupta, D., Maity, S., Samanta, S., Kundalia, K., Ali, Sk M., Saha, Swapan K., Tengblad, O., Perea, A., Martel, I., Cederkall, J.
Publikováno v:
EPJ Web of Conferences; 6/27/2024, Vol. 297, p1-4, 4p
Autor:
Gupta, D, Kundalia, K, Ali, Sk M, Maity, S, Mitra, R, Saha, Swapan K, Tengblad, O, Tavora, V G, Perea, A, Borge, M J G, Martel, I, Cederkall, J, Chishti, M, Park, J, Moro, A M
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od________65::a6b2776873c08125bb0c5daadb9b46aa
http://cds.cern.ch/record/2834501
http://cds.cern.ch/record/2834501
Autor:
Kundalia, K., Gupta, D., Ali, Sk M., Saha, Swapan K., Tengblad, O., Ovejas, J.D., Perea, A., Martel, I., Cederkall, J., Park, J., Szwec, S., Moro, A.M.
Publikováno v:
Physics Letters
The elastic and inelastic scattering of $^{7}$Be from $^{12}$C have been measured at an incident energy of 35 MeV. The inelastic scattering leading to the 4.439 MeV excited state of $^{12}$C has been measured for the first time. The experimental data
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3000::88f74c8287f35edd8a48ef4c9c26d15f
http://repo.scoap3.org/api
http://repo.scoap3.org/api
Autor:
Ali, Sk M., Gupta, D., Kundalia, K., Saha Swapan, K., Tengblad, O., Ovejas, J. D., Perea, A., Martel, I., Cederkall, J., Park, J., Szwec, S.
The anomaly in lithium abundance is a well-known unresolved problem in nuclear astrophysics. A recent revisit to the problem tried the avenue of resonance enhancement to account for the primordial 7Li abundance in standard big-bang nucleosynthesis. P
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______1222::42e43b6fb67fa45e1d282d21ff05da81
http://urn.fi/URN:NBN:fi:jyu-202208164140
http://urn.fi/URN:NBN:fi:jyu-202208164140
Autor:
Ali, Sk M, Gupta, D, Kundalia, K, Saha, Swapan K, Tengblad, O, Ovejas, J D, Perea, A, Martel, I, Cederkall, J, Park, J, Szwec, S
The Big Bang Nucleosynthesis (BBN) theory has been very successful in predicting the observed abundances of light elements like $^2$H, ${3,4}$He. There is, however, a serious discrepancy of a factor of about four in the observed abundance of $^7$Li a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od________65::5e0dce96e020ea2eeeec54edcc7a843d
http://cds.cern.ch/record/2836503
http://cds.cern.ch/record/2836503