Standard and Nonstandard Neutrino-Nucleus Reactions Cross Sections and Event Rates to Neutrino Detection Experiments

Table 3

Total number of events per ton of the target materials for a supernova at a distance of 10 kpc. We assume various energy thresholds 5, 10, 25, or 50 keV. Our present results are in excellent agreement with those of [25, 35].

Nucleus		keV	keV	keV	keV
^12C	2.52	2.25	2.05	1.60	1.14
^16O	3.29	2.84	2.51	1.83	1.19
^20Ne	4.03	3.35	2.87	1.96	1.16
^40Ar	9.46	6.63	5.01	2.53	1.00
^48Ti	10.73	7.04	5.06	2.27	0.76
^56Fe	12.00	7.36	5.04	2.01	0.57
^76Ge	18.58	9.61	5.82	1.70	0.30
^132Xe	30.68	9.84	4.16	0.46	0.01
^208Pb	46.93	7.86	1.95	0.03	<10^−3