γ-ray emission in proton-induced nuclear reactions on <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.svg"><mml:msup><mml:mrow /><mml:mrow><mml:mi>n</mml:mi><mml:mi>a</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:msup></mml:math>C and Mylar targets over the incident energy range, E = 30 – 200 MeV. Astrophysical implications-Reference-Cited by-同舟云学术

γ-ray emission in proton-induced nuclear reactions on natC and Mylar targets over the incident energy range, E = 30 – 200 MeV. Astrophysical implications

Published:2023-04 Issue: Volume:1032 Page:122622
ISSN:0375-9474
Container-title:Nuclear Physics A
language:en
Short-container-title:Nuclear Physics A

Author:

Rahma Y.,Ouichaoui S.^ORCID,Kiener J.,Lawrie E.A.,Lawrie J.J.,Tatischeff V.,Belhout A.,Moussa D.,Yahia-Cherif W.,Benhabiles-Mezhoud H.,Bucher T.D.,Dinoko T.R.S.,Chafa A.,Conradie J.L.,Damache S.,Debabi M.,Deloncle I.,Easton J.L.,Fouka M.,Hamadache C.,Hammache F.,Jones P.,Kheswa B.V.,Khumalo N.A.,Lamula T.,Majola S.N.T.,Ndayishimye J.,Negi D.,Noncolela S.P.,Ouziane S.,Papka P.,Peterson S.,Kumar Raju M.,Ramanathan V.,Rebeiro B.M.,de Séréville N.,Sharpey-Schafer J.F.,Shirinda O.,Wiedeking M.,Wyngaardt S.

Publisher

Elsevier BV

Subject

Nuclear and High Energy Physics

Reference70 articles.

1. Gamma-ray and millimeter-wave emissions from the 1991 June X-class solar flares;Ramaty;Astrophys. J.,1994

2. Using gamma-ray and neutron emission to determine solar flare accelerated particle spectra and composition and the conditions within the flare magnetic loop;Murphy;Astrophys. J. Suppl. Ser.,2007

3. Relativistic reconnection: an efficient source of non-thermal particles;Sironi;Astrophys. J. Lett.,2014

4. Erratum: “Deexcitation nuclear gamma-ray line emission from low-energy cosmic rays in the inner Galaxy” (2013, ApJ, 763, 98);Benhabiles-Mezhoud;Astrophys. J.,2013

5. Non-linear particle reacceleration by multiple shocks;Vieu;Mon. Not. R. Astron. Soc.,2022

Cited by 2 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. New γ-ray production cross sections for the 4.439 and 6.129 MeV lines of ¹²C and ¹⁶O. Astrophysical implications;Journal of Physics: Conference Series;2023-09-01

2. Shape analysis of the 4.44 MeV γ-ray line complex produced in inelastic proton scattering off ¹²C over the indent energy range of E_p = 30−200 MeV;Journal of Physics: Conference Series;2023-09-01