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<title>DFTC - Comunicaciones congresos, conferencias,...</title>
<link href="https://hdl.handle.net/10481/28382" rel="alternate"/>
<subtitle/>
<id>https://hdl.handle.net/10481/28382</id>
<updated>2026-04-19T07:56:15Z</updated>
<dc:date>2026-04-19T07:56:15Z</dc:date>
<entry>
<title>Trilepton signals: the golden channel for seesaw searches at LHC</title>
<link href="https://hdl.handle.net/10481/30589" rel="alternate"/>
<author>
<name>Águila Giménez, Francisco Del</name>
</author>
<author>
<name>Aguilar Saavedra, Juan Antonio</name>
</author>
<author>
<name>Blas Mateo, Jorge de</name>
</author>
<id>https://hdl.handle.net/10481/30589</id>
<updated>2022-10-25T10:13:32Z</updated>
<summary type="text">Trilepton signals: the golden channel for seesaw searches at LHC
Águila Giménez, Francisco Del; Aguilar Saavedra, Juan Antonio; Blas Mateo, Jorge de
The comparison of samples with different number of charged leptons shows that trilepton signals are the most significant ones for seesaw mediators. As previously pointed out, this is indeed the case for scalar (type II) and fermion (type III) triplets at LHC, which can be discovered in this channel for masses up to 500-700 GeV and an integrated luminosity of 30 fb^-1; whereas fermion singlets (type I) are marginally observable if there are no further new physics near the TeV scale. However, if there are new gauge interactions at this scale coupling to right-handed neutrinos, as in left-right models, heavy neutrinos are observable up to masses ~ 2 TeV for new gauge boson masses up to ~ 4 TeV, as we discuss in some detail.
Contribution to the Proceedings of the XXXIII International School of Theoretical Physics "Matter To The Deepest", Ustron, Poland, September 11-16, 2009.
</summary>
</entry>
<entry>
<title>Overview of models for the tt asymetry</title>
<link href="https://hdl.handle.net/10481/30529" rel="alternate"/>
<author>
<name>Aguilar Saavedra, Juan Antonio</name>
</author>
<id>https://hdl.handle.net/10481/30529</id>
<updated>2021-06-15T12:13:56Z</updated>
<summary type="text">Overview of models for the tt asymetry
Aguilar Saavedra, Juan Antonio
We review the most popular models proposed to explain the anomalous forward-backward asymmetry in t tbar production at the Tevatron. We discuss their viability in view of recent LHC data. We summarise their predictions for charge asymmetries at the LHC.
4th International Workshop on Top Quark Physics, 25-30th September 2011, Sant Feliu de Guixols, Spain.
</summary>
</entry>
<entry>
<title>tt  charge asymmetry, family and friends [presentación]</title>
<link href="https://hdl.handle.net/10481/30470" rel="alternate"/>
<author>
<name>Aguilar Saavedra, Juan Antonio</name>
</author>
<id>https://hdl.handle.net/10481/30470</id>
<updated>2021-06-15T12:13:53Z</updated>
<summary type="text">tt  charge asymmetry, family and friends [presentación]
Aguilar Saavedra, Juan Antonio
</summary>
</entry>
<entry>
<title>Limit on the diffuse flux of Ultra High Energy Neutrinos with the Pierre Auger</title>
<link href="https://hdl.handle.net/10481/29091" rel="alternate"/>
<author>
<name>Navarro, J. L.</name>
</author>
<id>https://hdl.handle.net/10481/29091</id>
<updated>2021-06-15T12:13:53Z</updated>
<summary type="text">Limit on the diffuse flux of Ultra High Energy Neutrinos with the Pierre Auger
Navarro, J. L.
</summary>
</entry>
<entry>
<title>Neutrino Astrophysics with the Pierre Auger Observatory</title>
<link href="https://hdl.handle.net/10481/29090" rel="alternate"/>
<author>
<name>Navarro, J. L.</name>
</author>
<id>https://hdl.handle.net/10481/29090</id>
<updated>2021-06-15T12:13:52Z</updated>
<summary type="text">Neutrino Astrophysics with the Pierre Auger Observatory
Navarro, J. L.
</summary>
</entry>
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