scholarly journals Impact of nuclear effects on the determination of the nucleon axial mass

2009 ◽  
Vol 80 (7) ◽  
Author(s):  
Omar Benhar ◽  
Davide Meloni
Keyword(s):  
2009 ◽  
Author(s):  
Davide Meloni ◽  
Federico Sanchez ◽  
M. Sorel ◽  
Luis Alvarez-Ruso
Keyword(s):  

2021 ◽  
Vol 104 (3) ◽  
Author(s):  
Christopher Thorpe ◽  
Jarosław Nowak ◽  
Kajetan Niewczas ◽  
Jan T. Sobczyk ◽  
Cezary Juszczak

2021 ◽  
Vol 81 (1) ◽  
Author(s):  
Richard D. Ball ◽  
Emanuele R. Nocera ◽  
Rosalyn L. Pearson

AbstractWe evaluate the uncertainties due to nuclear effects in global fits of proton parton distribution functions (PDFs) that utilise deep-inelastic scattering and Drell–Yan data on deuterium targets. To do this we use an iterative procedure to determine proton and deuteron PDFs simultaneously, each including the uncertainties in the other. We apply this procedure to determine the nuclear uncertainties in the SLAC, BCDMS, NMC and DYE866/NuSea fixed target deuteron data included in the NNPDF3.1 global fit. We show that the effect of the nuclear uncertainty on the proton PDFs is small, and that the increase in overall uncertainties is insignificant once we correct for nuclear effects.


2020 ◽  
Vol 2020 ◽  
pp. 1-6 ◽  
Author(s):  
Srishti Nagu ◽  
Jaydip Singh ◽  
Jyotsna Singh ◽  
R. B. Singh

The precise measurement of neutrino-oscillation parameters is one of the highest priorities in neutrino-oscillation physics. To achieve the desired precision, it is necessary to reduce the systematic uncertainties related to neutrino energy reconstruction. An error in energy reconstruction is propagated to all the oscillation parameters; hence, a careful estimation of the neutrino energy is required. To increase the statistics, neutrino-oscillation experiments use heavy nuclear targets like argon (Z=18). The use of these nuclear targets introduces nuclear effects that severely impact the neutrino energy reconstruction which in turn poses influence in the determination of neutrino-oscillation parameters. In this work, we have tried to quantify the presence of nuclear effects on the bounds of the CP phase by DUNE using final state interactions.


2003 ◽  
Vol 12 (02) ◽  
pp. 177-195
Author(s):  
K. J. Eskola ◽  
H. Honkanen ◽  
V. J. Kolhinen ◽  
P. V. Ruuskanen ◽  
C. A. Salgado

Determination of the nuclear parton distributions within the framework of perturbative QCD, the DGLAP equations in particulars, is discussed. Scale and flavour dependent nuclear effects in the parton distributions are compared with the scale and flavour independent parametrizations of HIJING and of the Hard Probe Collaboration. A comparison with the data from deep inelastic lepton-nucleus scattering and the Drell–Yan process in proton-nucleus collisions is shown.


2013 ◽  
Vol 2013 ◽  
pp. 1-16 ◽  
Author(s):  
Omar Benhar ◽  
Noemi Rocco

The quantitative description of the effects of nuclear dynamics on the measured neutrino-nucleus cross sections—needed to reduce the systematic uncertainty of long baseline neutrino oscillation experiments—involves severe difficulties. Owing to the uncertainty on the incoming neutrino energy, different reaction mechanisms contribute to the cross section measured at fixed energy and scattering angle of the outgoing lepton, and must therefore be consistently taken into account within a unified model. We research the theoretical approach based on the impulse approximation and the use of realistic nucleon spectral functions, allowing one to describe a variety of reaction mechanisms active in the broad kinematical range covered by neutrino experiments. The extension of this scheme to include more complex mechanisms involving the two-nucleon currents, which are believed to be important, is also outlined. The impact of nuclear effects on the determination of neutrino oscillation parameters is illustrated by analyzing the problem of neutrino energy reconstruction.


2011 ◽  
Author(s):  
Davide Meloni ◽  
S. K. Singh ◽  
J. G. Morfin ◽  
Makoto Sakuda ◽  
K. D. Purohit

1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.


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