At.Data Nucl.Data Tables 96, 645 (2010)

B.Pritychenko, S.F.Mughabghab, A.A.Sonzogni

Calculations of Maxwellian-averaged cross sections and astrophysical reaction rates using the ENDF/B-VII.0, JEFF-3.1, JENDL-3.3, and ENDF/B-VI.8 evaluated nuclear reaction data libraries

COMPILATION Z=1-100; A=1-255; compiled, analyzed Maxwellian averaged neutron capture σ, neutron-induced fission σ, astrophysical reaction rates.

NUCLEAR REACTIONS ^1,2H, ³He, ^6,7Li, ⁹Be, ^10,11B, C, ^14,15N, ^16,17O, ¹⁹F, ^22,23Na, ^24,25,26Mg, ²⁷Al, ^28,29,30Si, ³¹P, ^32,33,34,36S, ^35,37Cl, ^36,38,40Ar, ^39,40,41K, ^{40,42,43,44,46,48}Ca, ⁴⁵Sc, ^{46,47,48,49,50}Ti, V, ^50,52,53,54Cr, ⁵⁵Mn, ^54,56,57,58Fe, ^58,59Co, ^{58,59,60,61,62,64}Ni, ^63,65Cu, ^69,71Ga, ^{70,72,73,74,76}Ge, ^74,75As, ^{74,76,77,78,79,80,82}Se, ^79,81Br, ^{78,80,82,83,84,85,86}Kr, ^85,86,87Rb, ^{84,86,87,88,89,90}Sr, ^89,90,91Y, ^{90,91,92,93,94,95,96}Zr, ^93,94,95Nb, ^{92,94,95,96,97,98,99,100}Mo, ⁹⁹Tc, ^{96,98,99,100,101,102,103,104,105,106}Ru, ^103,105Rh, ^{102,104,105,106,107,108,110}Pd, ^{107,109,110,111}Ag, ^{106,108,110,111,112,113,114,115,116}Cd, ^113,115In, ^{112,113,114,115,116,117,118,119,120,122,123,124,125,126}Sn, ^{121,123,124,125,126}Sb, ^{120,122,123,124,125,126,127,128,129,130,132}Te, ^{127,129,130,131,135}I, ^{123,124,126,128,129,130,131,132,133,134,135,136}Xe, ^{133,134,135,136,137}Cs, ^{130,132,133,134,135,136,137,138,140}Ba, ^138,139,140La, ^{136,138,139,140,141,142,143,144}Ce, ^141,142,143Pr, ^{142,143,144,145,146,147,148,150}Nd, ^{147,148,149,151}Pm, ^{144,147,148,149,150,151,152,153,154}Sm, ^{151,152,153,154,155,156,157}Eu, ^{152,153,154,155,156,157,158,160}Gd, ^159,160Tb, ^{156,158,160,161,162,163,164}Dy, ^165,166Ho, ^{162,164,166,167,168,170}Er, ^175,176Lu, ^{174,176,177,178,179,180}Hf, ^181,182Ta, ^{182,183,184,186}W, ^185,187Re, ^191,193Ir, ¹⁹⁷Au, ^{196,198,199,200,201,202,204}Hg, ^{204,206,207,208}Pb, ²⁰⁹Bi, ^{223,224,225,226}Ra, ^225,226,227Ac, ^{227,228,229,230,232,233,234}Th, ^231,232,233Pa, ^{232,233,234,235,236,237,238,239,240,241}U, ^{235,236,237,238,239}Np, ^{236,237,238,239,240,241,242,243,244,246}Pu, ^{241,242,243,244}Am, ^{240,241,242,243,244,245,246,247,248,249,250}Cm, ^247,249,250Bk, ^{249,250,251,252,253,254}Cf, ^253,254,255Es, ²⁵⁵Fm(n, γ), E=0.001-1 MeV; calculated Maxwellian-averaged σ and astrophysical reaction rates using evaluated neutron libraries; deduced ENDF/B-VII.0, JENDL-3.3, JEFF-3.1, ENDF/B-VI.8 neutron-induced reaction σ deficiencies. Comparison with experimental data and KADONIS.

NUCLEAR REACTIONS ^223,226Ra, ²²⁷Ac, ^{227,228,229,230,232,233,234}Th, ^231,232,233Pa, ^{232,233,234,235,236,237,238,239,240,241}U, ^{235,236,237,238,239}Np, ^{236,237,238,239,240,241,242,243,244,246}Pu, ^{241,242,243,244}Am, ^{240,241,242,243,244,245,246,247,248,249,250}Cm, ^247,249,250Bk, ^{249,250,251,252,253,254}Cf, ^254,255Es, ²⁵⁵Fm(n, F), E=0.001-1 MeV; calculated Maxwellian-averaged σ and astrophysical reaction rates using evaluated neutron libraries.

doi: 10.1016/j.adt.2010.05.002