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<title>Collected Works</title>
<link>https://dspace.imsc.res.in/xmlui/handle/123456789/623</link>
<description>Collected Works</description>
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<rdf:li rdf:resource="https://dspace.imsc.res.in/xmlui/handle/123456789/837"/>
<rdf:li rdf:resource="https://dspace.imsc.res.in/xmlui/handle/123456789/839"/>
<rdf:li rdf:resource="https://dspace.imsc.res.in/xmlui/handle/123456789/832"/>
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<dc:date>2026-08-25T09:04:37Z</dc:date>
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<item rdf:about="https://dspace.imsc.res.in/xmlui/handle/123456789/837">
<title>The discovery of Dirac equation and its impact on present-day Physics</title>
<link>https://dspace.imsc.res.in/xmlui/handle/123456789/837</link>
<description>The discovery of Dirac equation and its impact on present-day Physics
Rajasekaran G.
</description>
<dc:date>1993-01-01T00:00:00Z</dc:date>
</item>
<item rdf:about="https://dspace.imsc.res.in/xmlui/handle/123456789/839">
<title>Introduction to String Theories</title>
<link>https://dspace.imsc.res.in/xmlui/handle/123456789/839</link>
<description>Introduction to String Theories
Rajasekaran G.
</description>
<dc:date>1988-01-01T00:00:00Z</dc:date>
</item>
<item rdf:about="https://dspace.imsc.res.in/xmlui/handle/123456789/832">
<title>HEP research in the Indian context - Reply</title>
<link>https://dspace.imsc.res.in/xmlui/handle/123456789/832</link>
<description>HEP research in the Indian context - Reply
Rajasekaran G.; Ramachandran R.
</description>
<dc:date>1997-01-01T00:00:00Z</dc:date>
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<item rdf:about="https://dspace.imsc.res.in/xmlui/handle/123456789/827">
<title>Large neutrino mixing angles for type-I see-saw mechanism in SO(100 GUT</title>
<link>https://dspace.imsc.res.in/xmlui/handle/123456789/827</link>
<description>Large neutrino mixing angles for type-I see-saw mechanism in SO(100 GUT
Bipin.R.Desai.; Rajasekaran G.; Utpal Sarkar
We consider the neutrino mixing angles in an SO(10) GUT with the usual Higgs structure in which neutrino masses are explained by the type-I see-saw mechanism. The Dirac-neutrino Yukawa matrix then has a structure similar to that of the u-quark. We determine the light neutrino mass matrix through type-I see-saw mechanism using the experimentally consistent u-quark Yukawa matrix. We find that large neutrino mixing-angles emerge naturally in this model.
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<dc:date>2005-01-01T00:00:00Z</dc:date>
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