Results 21 to 30 of about 274 (79)

Direct measurement of resonance strengths in S 34 (α,γ) Ar 38 at astrophysically relevant energies using the DRAGON recoil separator [PDF]

open access: yes, 2018
Background: Nucleosynthesis of mid-mass elements is thought to occur under hot and explosive astrophysical conditions. Radiative α capture on S34 has been shown to impact nucleosynthesis in several such conditions, including core and shell oxygen burning,
A. A. Chen   +18 more
core   +1 more source

Proton induced reactions on 114Sn and 120Sn targets at energies up to 18 MeV

open access: yes, 2023
We measure cross sections of proton-induced reactions on tin up to energies of 18 MeV using the stacked-foil activation technique, and report first experimental values for 114Sn(p,{\alpha})111In, {^{120}}Sn(p,{\alpha})117gIn, and 114Sn(p,x)113Sn ...
Bakhshiyan, T. M.   +4 more
core   +1 more source

Probing astrophysically important states in the ²⁶Mg nucleus to study neutron sources for the s process [PDF]

open access: yes, 2015
Background: The ²²Ne(α,n) ²⁵Mg reaction is the dominant neutron source for the slow neutron capture process (s process) in massive stars, and contributes, together with C¹³(α,n)O¹⁶, to the production of neutrons for the s process in asymptotic giant ...
Adachi, T.   +22 more
core   +3 more sources

Photoactivation study of 163TB β-decay [PDF]

open access: yes, 2023
The paper is a part of the research done within the project 8.2.2.0/20/I/006 LU and VPP-IZM-CERN-2022/1-0001. Institute of Solid State Physics, University of Latvia as the Center of Excellence has received funding from the European Union Horizon 2020 ...
Chekhovska, Anastasiia   +5 more
core   +1 more source

Muon-Induced Background Study for an Argon-Based Long Baseline Neutrino Experiment

open access: yes, 2012
We evaluated rates of transversing muons, muon-induced fast neutrons, and production of $^{40}$Cl and other cosmogenically produced nuclei that pose as potential sources of background to the physics program proposed for an argon-based long baseline ...
B. Svoboda   +10 more
core   +1 more source

The impact of individual nuclear properties on $r$-process nucleosynthesis

open access: yes, 2015
The astrophysical rapid neutron capture process or `$r$ process' of nucleosynthesis is believed to be responsible for the production of approximately half the heavy element abundances found in nature. This multifaceted problem remains one of the greatest
Aprahamian, A.   +3 more
core   +1 more source

Optimization of "Glucose ¹¹C" pharmaceutical production on the beam of an electron accelerator [PDF]

open access: yes, 2021
The process of “Glucose ¹¹C” pharmaceutical production by means of a photonuclear reaction ¹²C(γ, n)¹¹C is considered. The parameters of bremsstrahlung and electron beam scattered in the converter are investigated and optimized.
Deiev, O.S.   +3 more
core   +2 more sources

Formation of mixed X,n-radiation field at an electron accelerator [PDF]

open access: yes, 2022
For conducting photonuclear programs with the use of a high-intensity photon source the latter is ordinary obtained by transformation of an electron beam into X-ray radiation. Such a process is performed using an intermediate target-converter maid from a
Malets, Eu.B.   +2 more
core   +1 more source

Product yields for the photofission of ²³⁹Pu with bremsstrahlung at 17.5 MeV boundary energy [PDF]

open access: yes, 2021
The values of relative cumulative yields of 12 products (⁸⁵mKr, ⁹¹mY, ⁹²Sr, 97Zr, ⁹⁹Mo, ¹⁰⁵Ru, ¹³³I, ¹³⁴I, ¹³⁵I, ¹³⁸Cs, ¹³⁹Ba, ¹⁴²La, ¹⁴³Ce) of the ²³⁹Pu photofission was measured at a maximum bremsstrahlung energy of 17.5 MeV (average excitation energy ~
Lengyel, A.I.   +4 more
core   +2 more sources

Excitation functions of (n, p) reactions for the production of iodine isotopes used in medical applications

open access: yesNuclear Engineering and Technology
The cross sections of 124Xe (n, p)124I, 125Xe (n, p)125I, 126Xe (n, p)126I, 128Xe (n, p)128I, 129Xe (n, p)129I, 130Xe (n, p)130I, 131Xe (n, p)131I, 132Xe (n, p)132I, 133Xe (n, p)133I, 134Xe (n, p)134I and 135Xe (n, p)135I for production of iodine ...
Adeeb Omer Jafir   +2 more
doaj   +1 more source

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