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  <title>Dr.</title>
  <name first="Pablo" middle="" last="Roig"></name>
  <organization>Cinvestav</organization>
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<title>XV Latin American Symposium on High Energy Physics</title>
<description>&lt;p&gt;The &lt;strong&gt;Latin American Symposium on High Energy Physics (SILAFAE)&lt;/strong&gt;&amp;nbsp;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.&lt;/p&gt;

&lt;p&gt;This is the 15th edition&amp;nbsp;of the SILAFAE series, which will&amp;nbsp;take place in Mexico City, Mexico, at the beautiful campus of &lt;a href="https://www.cinvestav.mx/"&gt;Cinvestav&lt;/a&gt;.&amp;nbsp;&lt;/p&gt;

&lt;p&gt;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.&lt;/p&gt;

&lt;p&gt;The SILAFAE conference started in 1996 in M&amp;eacute;rida-Mexico, followed by editions in San Juan-Puerto Rico (1998), Cartagena de Indias-Colombia (2000), Aguas de Lindoia-Brazil (2002),&amp;nbsp;Lima-Peru (2004), Puerto Vallarta-Mexico (2006), San Carlos de Bariloche-Argentina (2009), Valpara&amp;iacute;so-Chile (2010), &lt;a href="https://www.ictp-saifr.org/2012-silafae-workshop/"&gt;S&amp;atilde;o Paulo-Brazil (2012)&lt;/a&gt;, Medell&amp;iacute;n-Colombia (2014), &lt;a href="https://ecfm.usac.edu.gt/silafae/"&gt;Antigua-Guatemala (2016) &lt;/a&gt;and&amp;nbsp;&lt;a href="https://indico.cern.ch/event/701855/"&gt;Lima-Peru (2018)&lt;/a&gt;.&amp;nbsp; The conference was cancelled in 2020 due to the Covid-19 pandemic but a&amp;nbsp;special, remote version&amp;nbsp;took place in 2021 in &lt;a href="http://www.ictp-saifr.org/silafae-xii-21/"&gt;virtual S&amp;atilde;o Paulo-Brazil&lt;/a&gt;. &lt;span style="background-color:rgba(0, 0, 0, 0); color:#000000"&gt;Returning in-person for the 2022 edition, the event took place in&lt;/span&gt; &lt;a href="https://indico.cern.ch/event/1151741/"&gt;Quito-Ecuador&lt;/a&gt;.&lt;/p&gt;
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<startDate>2024-11-04T08:00:00</startDate>
<endDate>2024-11-08T20:10:00</endDate>
<creationDate>2023-10-20T16:27:55</creationDate>
<modificationDate>2025-05-02T18:28:14</modificationDate>
<timezone>Mexico/General</timezone>
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  <title>Dr.</title>
  <name first="Pablo" middle="" last="Roig"></name>
  <organization>Cinvestav</organization>
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  <title>Dr.</title>
  <name first="Alejandro" middle="" last="Ayala"></name>
  <organization>Instituto de Ciencias Nucleares, UNAM</organization>
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  <title>Dr.</title>
  <name first="Alexis" middle="" last="Aguilar-Arevalo"></name>
  <organization>Instituto de Ciencias Nucleares, UNAM</organization>
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  <name first="Eduard" middle="" last="De La Cruz Burelo"></name>
  <organization>CINVESTAV-IPN Mexico</organization>
  <emailHash>207484e6583dd9c0c1af2f52ce04fdd8</emailHash>
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  <organization>IF UNAM</organization>
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  <title>Dr.</title>
  <name first="Gabriel" middle="" last="Lopez Castro"></name>
  <organization>cinvestav</organization>
  <emailHash>eab8fa4d5cccb2cb1eec6274ac246efe</emailHash>
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  <title>Dr.</title>
  <name first="Omar" middle="" last="Miranda"></name>
  <organization>Cinvestav</organization>
  <emailHash>6be00aeecce15d4b2547496f45352003</emailHash>
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 <user>
  <title>Dr.</title>
  <name first="Myriam" middle="" last="Mondragon Ceballos"></name>
  <organization>Instituto de Fisica, UNAM</organization>
  <emailHash>ccdabd182a8890b607e31f4424c79212</emailHash>
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  <title>Prof.</title>
  <name first="Alberto" middle="" last="Sanchez-Hernandez"></name>
  <organization>Departamento de Física, Cinvestav</organization>
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  <name first="Eric" middle="" last="Vazquez-Jauregui"></name>
  <organization>SNOLAB</organization>
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 <title>Decaimiento del Mesón Phi (1020) bajo Lagrangiano Efectivo</title>
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   <name first="Hernan" middle="" last="Valtierra"></name>
   <organization>CICFIM - UANL</organization>
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   <title>Mr.</title>
   <name first="Hernan" middle="" last="Valtierra"></name>
   <organization>CICFIM - UANL</organization>
   <emailHash>0270c6cc1fbb01eed525066103023cb0</emailHash>
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 <duration>00:15</duration>
 <abstract>Based on the work by E. Cremmer and M. Gourdin (1969), radiative correction calculations for the decays of the phi meson into neutral and charged kaons are reproduced, as these are its main decay modes:

\phi \rightarrow K^+ K^-

\phi \rightarrow K^0 \bar{K}^0

An effective Lagrangian is used, coupling massive spin-1 particles with neutral and charged scalar (spin-0) particles.

The radiative corrections appear in second-order processes within perturbation theory, requiring the regularization of loop integrals created by the interaction between the electromagnetic field and the charged kaons. Dimensional regularization and Passarino-Veltman functions are used for this purpose. The identified ultraviolet divergences are renormalized using counterterms, allowing for the identification of coupling constants and physical fields. Soft bremsstrahlung is included to remove infrared divergences from the theory.

It is proposed to continue the development under a effective theory of QCD, based on chiral symmetry with resonances, in order to improve the precision of the observables.</abstract>
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