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MEASUREMENT OF 182,184,186W (N, N’ γ) CROSS SECTIONS AND WHAT WE CAN LEARN FROM IT [PDF]
Today’s development of nuclear installations rely on numerical simulation for which the main input are evaluated nuclear data. Inelastic neutron scattering (n, xn) is a reaction of importance because it modifies the neutron population, the neutron energy
Henning Greg+17 more
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Nuclear data for space exploration
Understanding the harmful effects of galactic cosmic rays (GCRs) on space exploration requires a substantial amount of nuclear data. Specifically, the interaction of energetic GCR charged particles with spacecraft materials generates secondary radiations
Michael S. Smith+3 more
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Examining the fluorine overabundance problem by conducting Jinping deep underground experiment
BackgroundNuclear reactions have been crucial in the evolution of the universe since the big bang. The cross section of nuclear reaction that occurs during the early evolution of the star is extremely low, so it cannot be accurately measured in a ground ...
CHEN Yinji, ZHANG Liyong
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Search for neutron-hidden neutron interbrane transitions with MURMUR, a low-noise neutron passing-through-walls experiment [PDF]
Multi-braneworld universe is at the heart of many scenarios of physics beyond the Standard Model and the cosmological model ΛCDM. It is thus an important concern to constrain these scenarios which also allow for experiments below the GeV scale. MURMUR is
Stasser Coraline+2 more
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Nuclear Energy Levels in 44Ca using FPD6pn Interaction
Nuclear energy levels; total angular moment, even-even parity, and even odd parities for nucleons that were present outside closed core for the isobars 44Ca nuclei, which occupied low levels fp-LS shell (1f7/2,1f5/2, 2p3/2,2p1/2), within shell model ...
Maryam K. Hassan, Firas Z. Majeed
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Absolute measurement of the isotopes 16O and 18O in bombarded H218O sample using deuteron-induced gamma-ray emission technique [PDF]
In this research work, we used the Deuteron Induced Gamma-ray Emission (DIGE) method based on 18O(d,pγ)19O (Eγ=1376 keV), and 16O(d,pγ)17O (Eγ= 871 keV) nuclear reactions to determine absolute amounts of the stable isotopes 16O and 18O in the irradiated
H. Rafi-Kheiri+3 more
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s-process Nuclear Reaction Rates [PDF]
In stars the 13C(α, n)16O and 22Ne(α, n)25Mg reactions are the two main sources of neutrons for the so-called slow neutron capture process (s-process), which is one of the main mechanisms for the stellar synthesis of heavy elements.
Rapagnani David
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Journey to the cosmos: Navigating stellar evolution with differential equations
Differential equations are a fundamental and versatile mathematical tool that finds widespread application across diverse academic disciplines, from physics and biology to economics and engineering.
Anshuman Jha+3 more
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Investigation of the production of cobalt-60 via particle accelerator [PDF]
The production process of cobalt-60 was simulated by a particle accelerator in the energy range of 5 to 100 MeV, particle beam current of 1 mA, and irradiation time of 1 hour to perform yield, activity of reaction, and integral yield for charged
Artun Ozan
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The present paper examines the luminescence of ternary Ar-Kr-Xe and Ne-Ar-Kr mixtures of noble gases in the spectral range from 300 to 970 nm, excited by the 6Li(n,α)3H nuclear reaction products in the core of a nuclear reactor.
K. Samarkhanov+7 more
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