Abstract
If Gamma Ray Bursts (GRBs) are associated with a stellar collapse-like phenomenon then it is reasonable to expect neutrino production to occur at the source. We have performed a temporal correlation analysis with GRBs using the IMB low-energy neutrino dataset during 809 days of livetime between 1986 and 1990. No correlations were observed placing a 90% C.L. limit of 0.046 v interactions per GRB. The dependence of the GRB distances to neutrino yield using volume and shell distribution models is discussed. Lower limits are derived which exclude galactic stellar collapse-like models.
| Original language | English |
|---|---|
| Title of host publication | Compton Gamma-Ray Observatory |
| Editors | Neil Gehrels, Michael W. Friedlander, Daryl J. Macomb |
| Publisher | American Institute of Physics Inc. |
| Pages | 838-842 |
| Number of pages | 5 |
| ISBN (Electronic) | 1563961040 |
| DOIs | |
| State | Published - 1993 |
| Event | Compton Symposium - St. Louis, United States Duration: Oct 15 1992 → Oct 17 1992 |
Publication series
| Name | AIP Conference Proceedings |
|---|---|
| Volume | 280 |
Conference
| Conference | Compton Symposium |
|---|---|
| Country/Territory | United States |
| City | St. Louis |
| Period | 10/15/92 → 10/17/92 |
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