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Article << Previous     |     Next >>   Contents Vol 26(3)

A Method to Obtain a Maxwell–Boltzmann Neutron Spectrum at kT = 30 keV for Nuclear Astrophysics Studies

J. Praena A C, P. F. Mastinu A, G. Martín Hernández B

A INFN-Laboratori Nazionali di Legnaro, Padova, Italy
B Centro de Aplicaciones Tecnologicas y Desarrollo Nuclear, La Habana, Cuba
C Corresponding author. Email: jpraena@lnl.infn.it
 
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Abstract

A method to shape the neutron energy spectrum at low-energy accelerators is proposed by modification of the initial proton energy distribution. A first application to the superconductive RFQ of the SPES project at Laboratori Nazionali di Legnaro is investigated for the production of a Maxwell–Boltzmann neutron spectrum at kT = 30 keV via the 7Li(p, n)7Be reaction. Concept, solutions and calculations for a setup consisting of a proton energy shaper and a lithium target are presented. It is found that a power dentisity of 3 kW cm–2 could be sustained by the lithium target and a forward-directed neutron flux higher than 1010 s–1 at the sample position could be obtained. In the framework of the SPES project the construction of a LEgnaro NeutrOn Source (LENOS) for Astrophysics and for validation of integral nuclear data is proposed, suited for activation studies on stable and unstable isotopes.

Keywords: nuclear astrophysics, Maxwellian averaged cross sections, neutron production


   
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