2125
DPyC SMF
false
[["minutes", "Minutes"], ["notes", "Notes"], ["paper", "Paper"], ["poster", "Poster"], ["slides", "Slides"], ["summary", "Summary"]]
Dr.
Cinvestav
ea481e58ca9c64e14d7982cb66bcd604
3312
XV Latin American Symposium on High Energy Physics
<p>The <strong>Latin American Symposium on High Energy Physics (SILAFAE)</strong> is an event with a tradition of over 25 years, that brings together the regional and international community of particle physics and related areas such as cosmology, gravitation and astroparticle physics. The conference has been the main regional hub for discussions on topics in the relevant fields, knowledge updates and the exploration of new ideas and perspectives towards the future. The event also promotes the expansion of regional and international cooperation as well as the professional development of young scientists and students.</p>
<p>This is the 15th edition of the SILAFAE series, which will take place in Mexico City, Mexico, at the beautiful campus of <a href="https://www.cinvestav.mx/">Cinvestav</a>. </p>
<p>The conference format consists of a series of plenary and parallel talks covering a range of theoretical and experimental topics. An active posters session is also planned.</p>
<p>The SILAFAE conference started in 1996 in Mérida-Mexico, followed by editions in San Juan-Puerto Rico (1998), Cartagena de Indias-Colombia (2000), Aguas de Lindoia-Brazil (2002), Lima-Peru (2004), Puerto Vallarta-Mexico (2006), San Carlos de Bariloche-Argentina (2009), Valparaíso-Chile (2010), <a href="https://www.ictp-saifr.org/2012-silafae-workshop/">São Paulo-Brazil (2012)</a>, Medellín-Colombia (2014), <a href="https://ecfm.usac.edu.gt/silafae/">Antigua-Guatemala (2016) </a>and <a href="https://indico.cern.ch/event/701855/">Lima-Peru (2018)</a>. The conference was cancelled in 2020 due to the Covid-19 pandemic but a special, remote version took place in 2021 in <a href="http://www.ictp-saifr.org/silafae-xii-21/">virtual São Paulo-Brazil</a>. <span style="background-color:rgba(0, 0, 0, 0); color:#000000">Returning in-person for the 2022 edition, the event took place in</span> <a href="https://indico.cern.ch/event/1151741/">Quito-Ecuador</a>.</p>
False
2024-11-04T08:00:00
2024-11-08T20:10:00
2023-10-20T16:27:55
2025-05-02T18:28:14
Mexico/General
Dr.
Cinvestav
ea481e58ca9c64e14d7982cb66bcd604
Dr.
Instituto de Ciencias Nucleares, UNAM
0e7430d668e3ccde26b8cbbd9bacb42d
Dr.
Instituto de Ciencias Nucleares, UNAM
fb4a07e67bf154a31195c2bde93f4113
Prof.
CINVESTAV-IPN Mexico
207484e6583dd9c0c1af2f52ce04fdd8
Mr.
IF UNAM
e8f8d57b00ab4619f39ebce7420e82db
Dr.
cinvestav
eab8fa4d5cccb2cb1eec6274ac246efe
Dr.
Cinvestav
6be00aeecce15d4b2547496f45352003
Dr.
Instituto de Fisica, UNAM
ccdabd182a8890b607e31f4424c79212
Prof.
Departamento de Física, Cinvestav
5bf6b28139e80a932ccc7f415ba7fd8f
Dr.
SNOLAB
d23af97e76e70a964c32ec245dce89bc
149
false
[["minutes", "Minutes"], ["notes", "Notes"], ["paper", "Paper"], ["poster", "Poster"], ["slides", "Slides"], ["summary", "Summary"]]
S3-Modular Flavor Model
Mr.
Instituto de Física,UNAM
bbd98d6299183e3f98361c638ad1a0d9
Mr.
Instituto de Física,UNAM
bbd98d6299183e3f98361c638ad1a0d9
Dr.
Instituto de Fisica, UNAM
ccdabd182a8890b607e31f4424c79212
00:15
In this work we study an extension of the $SU(5)$ grand unification model in the supersymmetric case, which consists in adding a $S_3$-modular symmetry. This symmetry takes the role of a flavour symmetry between quarks. Futhermore, the Higgs scalar sector is extended to include six doublets in contrast to the minimal Higgs sector of the Standard Model of Elementary Particles. Then we proceed to group the particle fields in the different irreducible representations of $SU(5)$ and within the irreducible representations of $S_3$. Once the matter content of the model is established, we proceed to construct the Yukawa potential where modular forms are used and specific modular weights are assigned to the particle fields in order to make the potential invariant under the flavour symmetry. From the mass matrices associated with the potential, which exhibit NNI textures, the CKM mixing matrix is constructed. In view of these results and by means of a $\chi ^2$ adjustment, we seek to reproduce the mass hierarchy and the mixing angles between the different quark flavors that are known experimentally on the $M_Z$ scale.