We consider new data on high energy neutrinos (Ev>2 Gev) obtained from the Frejus and Kamioka detectors as well as previous data from the IMB detector and compare the experimental limits on neutrinos from the sun to our expectations based on a cold dark matter hypothesis. We also extend previous work to include a wide variety of cold dark matter candidates.
Bibliographical noteFunding Information:
We wouldl ike to thankD avidC aldwella ndRick Watkinsf or helpfuld iscussionsK.. A.O. is supported in part by DOE Grant No. DE-AC02-83ER-40105, andb ya PresidentiaYlo ungI nvestigatoArw ard.M .S. is supporteidn partb yNSF GrantN o. PHY86-14185, andb y an AlfredP . SloanR esearchFe llowship.