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G

G. Tešić

Researcher at Carleton University

Publications -  10
Citations -  1380

G. Tešić is an academic researcher from Carleton University. The author has contributed to research in topics: Sudbury Neutrino Observatory & Neutrino. The author has an hindex of 10, co-authored 10 publications receiving 1315 citations.

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Journal ArticleDOI

Measurement of the total active B-8 solar neutrino flux at the Sudbury Neutrino Observatory with enhanced neutral current sensitivity

S. N. Ahmed, +141 more
TL;DR: The Sudbury Neutrino Observatory has precisely determined the total active (nu(x) 8B solar neutrino flux without assumptions about the energy dependence of the nu(e) survival probability.
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Independent Measurement of the Total Active 8B Solar Neutrino Flux Using an Array of 3He Proportional Counters at the Sudbury Neutrino Observatory

B. Aharmim, +174 more
TL;DR: The Sudbury Neutrino Observatory (SNO) used an array of He3 proportional counters to measure the rate of neutral-current interactions in heavy water and precisely determined the total active (x) B8 solar neutrino flux as discussed by the authors.
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Measurement of the νe and total 8B solar neutrino fluxes with the Sudbury Neutrino Observatory phase-III data set

B. Aharmim, +156 more
- 18 Jan 2013 - 
TL;DR: In this article, an array of He-3 proportional counters was installed in the heavy-water target to measure precisely the rate of neutrino-deuteron neutral-current interactions.
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Constraints on nucleon decay via invisible modes from the Sudbury Neutrino Observatory.

S. N. Ahmed, +143 more
TL;DR: Data from the Sudbury Neutrino Observatory have been used to constrain the lifetime for nucleon decay to "invisible" modes, such as n-->3nu, which is about an order of magnitude more stringent than previous constraints on invisible proton-decay modes and 400 timesMore stringent than similar neutron modes.
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A search for neutrinos from the solar hep reaction and the diffuse supernova neutrino background with the sudbury neutrino observatory

B. Aharmim, +147 more
TL;DR: In this article, a search for neutrinos from the hep reaction in the Sun and from the diffuse supernova neutrino background (DSNB) using data collected during the first operational phase of the Sudbury Neutrino Observatory, with an exposure of 0.65 ktons yr.