MEASUREMENTS OF THE n+p→d+γ CROSS SECTION FOR BIG BANG NUCLEOSYNTHESIS WITH THE SPALLATION NEUTRON SOURCE AT THE LOS ALAMOS NEUTRON SCIENCE CENTER

Author(s):  
E.-I. ESCH ◽  
J. M. O'DONNELL ◽  
S. A. WENDER ◽  
D. BOWMAN ◽  
G. MORGAN ◽  
...  
2019 ◽  
Author(s):  
Eric John Pitcher ◽  
Yuri Konstantinovich Batygin ◽  
Stuart Andrew Maloy

2002 ◽  
Vol 39 (sup2) ◽  
pp. 638-641 ◽  
Author(s):  
Klaus H. Guber ◽  
Paul E. Koehler ◽  
Timothy E. Valentine ◽  
Luiz C. Leal

2020 ◽  
Vol 239 ◽  
pp. 01004
Author(s):  
Yaron Danon ◽  
Ezekiel Blain ◽  
Kumar Mohindroo ◽  
Matt Devlin ◽  
Keegan J.Kelly ◽  
...  

A neutron induced neutron emission experiment was conducted as the Los Alamos Neutron Science Center (LANSCE) facility at Los Alamos National Laboratory (LANL). In this experiment, a sample was placed in a well collimated neutron beam and was surrounded by an array of 28 fast neutron detectors (EJ-309). The experiment was performed with a neutron flight path of 21.5 m from the source to the sample, and 1 m from the sample to the detectors. The neutron emission from the sample was measured as a function of neutron time of flight covering an incident energy range from 0.7- 20 MeV. The samples included U-235, Pu-239, carbon (graphite), and blanks that matched the encapsulation of the sample. The measured samples were constantly cycled in and out of the neutron beam. This type of experiment measures neutron emission from all reactions occurring in the sample such as fission and elastic and inelastic scattering. Similar to the methodology previously developed at RPI [1], the measurements were compared with detailed simulations of the experiment using different cross section evaluations for the sample. The observed differences can be attributed to the evaluated neutron cross section and angular distributions. The carbon sample was used as a reference to validate both the experiment and simulation methodology and showed good agreement between experiments and simulations. A review of the experimental setup, analysis methods, and some of the results will be presented.


2013 ◽  
Vol 53 (A) ◽  
pp. 534-537 ◽  
Author(s):  
Carlo Gustavino

The <sup>2</sup>H(α, γ)<sup>6</sup>Li reaction is the leading process for the production of <sup>6</sup>Li in standard Big Bang Nucleosynthesis. Recent observations of lithium abundance in metal-poor halo stars suggest that there might be a 6Li plateau, similar to the well-known Spite plateau of <sup>7</sup>Li. This calls for a re-investigation of the standard production channel for <sup>6</sup>Li. As the <sup>2</sup>H(α, γ)<sup>6</sup>Li cross section drops steeply at low energy, it has never before been studied directly at Big Bang energies. For the first time the reaction has been studied directly at Big Bang energies at the LUNA accelerator. The preliminary data and their implications for Big Bang nucleosynthesis and the purported <sup>6</sup>Li problem will be shown.


2014 ◽  
Vol 89 (3) ◽  
Author(s):  
J. L. Ullmann ◽  
T. Kawano ◽  
T. A. Bredeweg ◽  
A. Couture ◽  
R. C. Haight ◽  
...  

2020 ◽  
Vol 1668 (1) ◽  
pp. 012028
Author(s):  
Viviana Mossa

Abstract The Big Bang Nucleosynthesis (BBN) describes the production of light nuclides occurred during the first minutes of cosmic time. It started with the accumulation of deuterium, whose primordial abundance is sensitive to the universal baryon density and to the amount of relativistic particles. Currently the main source of uncertainty to an accurate theoretical deuterium abundance evaluation is due to the poor knowledge of the D(p, γ)3He cross section at BBN energies. The present work wants to describe one of the two experimental approaches proposed by the LUNA collaboration, whose goal is to measure with unprecedented precision, the reaction cross section in the energy range 30 < Ecm[keV] < 300.


2010 ◽  
Author(s):  
Feirouz Hammache ◽  
Daniel Galaviz ◽  
K. Sümmerer ◽  
S. Typel ◽  
F. Uhlig ◽  
...  

1992 ◽  
Vol 538 ◽  
pp. 515-521 ◽  
Author(s):  
A. Coc ◽  
P. Aguer ◽  
S. Barhoumi ◽  
F.M. Baumann ◽  
G. Bogaert ◽  
...  

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