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<rdf:RDF xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:dc="http://purl.org/dc/elements/1.1/"><rdf:Description rdf:about="https://repozitorij.uni-lj.si/IzpisGradiva.php?id=175882"><dc:title>Beyond neutrino mass: observable $n$-$\bar{n}$ oscillations in UV complete seesaw models</dc:title><dc:creator>Doršner,	Ilja	(Avtor)
	</dc:creator><dc:creator>Fajfer,	Svjetlana	(Avtor)
	</dc:creator><dc:creator>Saad,	Shaikh	(Avtor)
	</dc:creator><dc:subject>physics of elementary particles</dc:subject><dc:description>Next-generation experiments, such as the Deep Underground Neutrino Experiment and the European Spallation Source, are set to improve sensitivity to neutron-antineutron oscillation, a direct probe of ∆B = 2 baryon number violation, with particularly significant gains expected at the latter. The discovery of such a rare ∆B = 2 process would indicate physics beyond the Standard Model and could point to specific unified theories that allow observable ▫$n$▫-▫$\bar{n}$▫ transitions. We accordingly examine ▫$n$▫-▫$\bar{n}$▫ oscillations within a unified framework that accounts for charged fermion masses and generates viable neutrino masses via the seesaw mechanism. More specifically, we show that ▫$n$▫-▫$\bar{n}$▫ oscillations can arise from two specific topologies within two distinct SU(5) scenarios. One topology requires a presence of two color-sextet scalars in the Type II seesaw framework, whereas the other involves a scalar sextet and a color-octet fermion in the Type III seesaw framework. While the former topology can be realized in the SO(10)/Pati-Salam frameworks, the latter finds a natural embedding in SU(5), which constitutes one of the key novelties of our work. Remarkably enough, the same dynamics responsible for fermion masses also induces baryon number violation, thus linking ▫$n$▫-▫$\bar{n}$▫ oscillations to the flavor structure of the theory. We show that, given a TeV-scale mass for one of the colored states, upcoming searches for such ∆B = 2 processes can probe for a presence of the other colored states with masses up to 1011 GeV, well beyond the reach of colliders. This positions ▫$n$▫-▫$\bar{n}$▫ oscillations as a rare low-energy portal to grand unification and ultra-heavy new physics.</dc:description><dc:date>2025</dc:date><dc:date>2025-11-12 13:15:18</dc:date><dc:type>Članek v reviji</dc:type><dc:identifier>175882</dc:identifier><dc:language>sl</dc:language></rdf:Description></rdf:RDF>
