Results 31 to 40 of about 424,503 (339)

Neutron Thermal Cross Sections, Westcott Factors, Resonance Integrals, Maxwellian Averaged Cross Sections and Astrophysical Reaction Rates Calculated from Major Evaluated Data Libraries

open access: yes, 2013
We present calculations of neutron thermal cross sections, Westcott factors, resonance integrals, Maxwellian-averaged cross sections and astrophysical reaction rates for 843 ENDF materials using data from the major evaluated nuclear libraries and ...
Abusaidi   +56 more
core   +1 more source

Nuclear Radii of Unstable Nuclei

open access: yes, 2011
In the presented review we discuss the problem of extraction the parameters of nuclear matter and charge distribution in stable and unstable isotopes.
Alkhazov, G. D.   +2 more
core   +1 more source

Differences between stellar and laboratory reaction cross sections [PDF]

open access: yes, 2009
Nuclear reactions proceed differently in stellar plasmas than in the laboratory due to the thermal effects in the plasma. On one hand, a target nucleus is bombarded by projectiles distributed in energy with a distribution defined by the plasma ...
Fowler W A, Rauscher T, Thomas Rauscher
core   +2 more sources

Unveiling radii and neutron skins of unstable atomic nuclei via nuclear collisions

open access: yesFrontiers in Physics
Total reaction, interaction, and charge-changing cross sections, which are kinds of cross sections standing for total nuclear collision probability in medium-to high-energy region from a few to several hundred MeV, have been extensively utilized to probe
Masaomi Tanaka   +6 more
doaj   +1 more source

Delta Decay in Nuclear Medium

open access: yes, 1996
Proton-nucleus collisions, where the beam proton gets excited to the delta resonance and then decays to p$\pi ^+$, either inside or outside the nuclear medium, are studied.
Jain, B. K., Kundu, Bijoy
core   +2 more sources

Astrophysical S-factor of the $^7$Be($p,\gamma)^8$B reaction from Coulomb dissociation of $^8$B

open access: yes, 1996
The Coulomb dissociation method to obtain the astrophysical S-factor, $S_{17}(0)$, for the $^7$Be($p,\gamma)^8$B reaction at solar energies is investigated by analysing the recently measured data on the breakup reaction $^{208}$Pb$(^8$B,$^7$Be$~p)^{208 ...
A.K. Dutt-Mazumder   +30 more
core   +2 more sources

Disordered but rhythmic—the role of intrinsic protein disorder in eukaryotic circadian timing

open access: yesFEBS Letters, EarlyView.
Unstructured domains known as intrinsically disordered regions (IDRs) are present in nearly every part of the eukaryotic core circadian oscillator. IDRs enable many diverse inter‐ and intramolecular interactions that support clock function. IDR conformations are highly tunable by post‐translational modifications and environmental conditions, which ...
Emery T. Usher, Jacqueline F. Pelham
wiley   +1 more source

The energy dependence of nuclear reaction cross sections

open access: yesPhysics Letters B, 1984
Abstract The reaction cross section σ R pA ( E ) for proton-nucleus collisions varies with energy as the total cross section σ t pN ( E ) does for proton-nucleon scattering in the energy regime 100 MeV ⩽ E ⩽400 GeV. We propose several empirical relations, and test them by a χ 2 analysis of various data.
N.H. Kwong, J. Hüfner
openaire   +1 more source

Protein pyrophosphorylation by inositol pyrophosphates — detection, function, and regulation

open access: yesFEBS Letters, EarlyView.
Protein pyrophosphorylation is an unusual signaling mechanism that was discovered two decades ago. It can be driven by inositol pyrophosphate messengers and influences various cellular processes. Herein, we summarize the research progress and challenges of this field, covering pathways found to be regulated by this posttranslational modification as ...
Sarah Lampe   +3 more
wiley   +1 more source

Revised Reaction Rate for the Astrophysical Reaction 18O(p, α)15N via a Global R-matrix Analysis

open access: yesThe Astrophysical Journal
The ^18 O( p , α ) ^15 N reaction is of particular importance for influencing the abundances of key isotopes such as ^19 F, ^18 O, and ^15 N. Peculiar abundances for these nuclei are observed from spectra or meteorite grains originating in asymptotic ...
Yi-Yang Li   +4 more
doaj   +1 more source

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