29 results on '"Goswami, Srubabati"'
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2. Probing mass orderings in presence of a very light sterile neutrino in a liquid argon detector
3. Corrigendum to “Implications of the Dark-LMA solution for neutrino mass matrices” [Nucl. Phys. B 969 (2021) 115460]
4. Implications of the Dark-LMA solution for neutrino mass matrices
5. Implications of the Dark-LMA solution for neutrino mass matrices
6. Spotlighting the sensitivities of Hyper-Kamiokande, DUNE and ESSνSB
7. Challenges posed by non-standard neutrino interactions in the determination of δ at DUNE
8. The physics of antineutrinos in DUNE and determination of octant and δ CP
9. Neutrino Phenomenology: Highlights of Oscillation Results and Future Prospects
10. Evidence for leptonic CP phase from NOνA, T2K and ICAL: A chronological progression
11. Session III: Oscillation at High Energies
12. Physics Capabilities of Future Atmospheric Neutrino Detectors
13. An SO(10) model with adjoint fermions for double seesaw neutrino masses
14. Hybrid textures in minimal seesaw mass matrices
15. Renormalization group evolution of neutrino masses and mixing in the Type-III seesaw mechanism
16. Minimal textures in seesaw mass matrices and their low and high energy phenomenology
17. Physics Program of India Based Neutrino Observatory
18. Global Analysis of Neutrino Oscillation
19. Update of the solar neutrino oscillation analysis with the 766 Ty KamLAND spectrum
20. Constraints on neutrino oscillation parameters from the SNO salt phase data
21. On the measurement of solar neutrino oscillation parameters with KamLAND
22. The solar neutrino problem after the first results from KamLAND
23. Neutrino decay confronts the SNO data
24. Implications of the first neutral current data from SNO for solar neutrino oscillation
25. A three generation oscillation analysis of the Super-Kamiokande atmospheric neutrino data beyond one mass scale dominance approximation
26. Energy deposition due to neutrino pair annihilation near rotating neutron stars
27. Impact of the first SNO results on neutrino mass and mixing
28. Is neutrino decay really ruled out as a solution to the atmospheric neutrino problem from Super-Kamiokande data?
29. Status of the neutrino decay solution to the solar neutrino problem
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