activity
20032009
most citedCornering Solar Radiative-Zone Fluctuations with KamLAND and SNO Salt

50 citations · 303 across the 10 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2009★ 7 cited

Mimicking diffuse supernova antineutrinos with the Sun as a source

Georg Raffelt, Timur Rashba

Measuring the electron antineutrino component of the cosmic diffuse supernova neutrino background (DSNB) is the next ambitious goal for low-energy neutrino astronomy. The largest f…

astro-ph2005★ 16 cited

Radiative zone solar magnetic fields and g-modes

T. I. Rashba, V. B. Semikoz, J. W. F. Valle

We consider a generalized model of seismic-wave propagation that takes into account the effect of a central magnetic field in the Sun. We determine the g-mode spectrum in the pertu…

hep-ph2004★ 41 cited

Enhanced solar anti-neutrino flux in random magnetic fields

O. G. Miranda, T. I. Rashba, A. I. Rez +1

We discuss the impact of the recent KamLAND constraint on the solar anti-neutrino flux on the analysis of solar neutrino data in the presence of Majorana neutrino transition magnet…

hep-ph2004

Efficient solar anti-neutrino production in random magnetic fields

O. G. Miranda, T. I. Rashba, A. I. Rez +1

We have shown that the electron anti-neutrino appearance in the framework of the spin flavor conversion mechanism is much more efficient in the case of neutrino propagation through…

hep-ph2003★ 50 cited

Cornering Solar Radiative-Zone Fluctuations with KamLAND and SNO Salt

C. P. Burgess, N. S. Dzhalilov, M. Maltoni +4

We update the best constraints on fluctuations in the solar medium deep within the solar Radiative Zone to include the new SNO-salt solar neutrino measurements. We find that these…

astro-ph2003★ 41 cited

Resonant origin for density fluctuations deep within the Sun: helioseismology and magneto-gravity waves

C. P. Burgess, N. S. Dzhalilov, T. I. Rashba +2

We analyze helioseismic waves near the solar equator in the presence of magnetic fields deep within the solar radiative zone. We find that reasonable magnetic fields can significan…