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Dive into the research topics where Bhag C. Chauhan is active.

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Featured researches published by Bhag C. Chauhan.


European Physical Journal C | 2007

Quark–lepton complementarity with lepton and quark mixing data predict θ13 PMNS=(9+1 -2)°

Bhag C. Chauhan; Marco Picariello; Joao Pulido; E. Torrente-Lujan

The complementarity between the quark and lepton mixing matrices is shown to provide a robust prediction for the neutrino mixing angle


Journal of High Energy Physics | 2004

LMA and sterile neutrinos: a case for resonance spin flavour precession?

Bhag C. Chauhan; Joao Pulido

\theta_{13}^{PMNS}


Physical Review D | 2003

KamLAND, solar antineutrinos, and the solar magnetic field

Bhag C. Chauhan; Joao Pulido; Emilio Torrente-Lujan

. We obtain this prediction by first showing that the matrix


Physical Review D | 2006

Neutrino mass matrices with vanishing determinant

Bhag C. Chauhan; Joao Pulido; Marco Picariello; I.N.F.N.-Milano

V_M


Journal of High Energy Physics | 2005

Low energy solar neutrinos and spin flavour precession

Bhag C. Chauhan; Joao Pulido; Raju S. Raghavan

, product of the CKM and PMNS mixing matrices, may have a zero (1,3) entry which is favored by experimental data. Hence models with bimaximal or tribimaximal forms of the correlation matrix


Physical Review D | 2002

Resonance spin flavor precession of solar neutrinos after SNO neutral current data

Bhag C. Chauhan; Joao Pulido

V_M


International Journal of Modern Physics A | 2007

Predictions from non trivial Quark-Lepton complementarity

Marco Picariello; Bhag C. Chauhan; Joao Pulido; Emilio Torrente-Lujan

are quite possible. Any theoretical model with a vanishing (1,3) entry of


Journal of High Energy Physics | 2004

SNO, SuperKamiokande data, antineutrinos and sterile neutrinos

Bhag C. Chauhan; Joao Pulido

V_M


Journal of High Energy Physics | 2006

7Be neutrino signal variation in KamLAND

Bhag C. Chauhan

that is in agreement with quark data, solar, and atmospheric mixing angle leads to


arXiv: High Energy Physics - Phenomenology | 2006

SOLAR NEUTRINOS: SPIN FLAVOUR PRECESSION AND LMA

Joao Pulido; Raju S. Raghavan; Bhag C. Chauhan

\theta_{13}^{PMNS}=(9{^{+1}_{-2}})^\circ

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Joao Pulido

Instituto Superior Técnico

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Gazal Sharma

Central University of Himachal Pradesh

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Shankita Bhardwaj

Central University of Himachal Pradesh

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Surender Verma

Central University of Himachal Pradesh

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Zoltan Batiz

Instituto Superior Técnico

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Ashish Sharma

Central University of Himachal Pradesh

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Govind Singh

Central University of Himachal Pradesh

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S. Dev

Himachal Pradesh University

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