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<category>DPyC SMF</category>
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  <title>Dr.</title>
  <name first="Pablo" middle="" last="Roig"></name>
  <organization>Cinvestav</organization>
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<title>XXI Mexican School on Particles and Fields 2026</title>
<description>&lt;p style="text-align:justify"&gt;The &lt;strong&gt;XXI Mexican School on Particles and Fields&lt;/strong&gt; takes place from &lt;strong&gt;October 19th to 23rd, 2026&lt;/strong&gt;, in the city of Puebla, Puebla, M&amp;eacute;xico. The format of the school is&amp;nbsp;such that the morning sessions are devoted to theoretical and experimental reviews, whereas parallel thematic sessions shall be held in the afternoons. All the reviews and seminars are delivered by experts of international prestige on subjects which are of current interest to the global scientific community and are also actively pursued within M&amp;eacute;xico. ​&lt;/p&gt;

&lt;p style="text-align:justify"&gt;In order to equip graduate students and attending postdocs with the necessary tools to perform fully in the school, courses of interest are taught, with English being the language of instruction. An informal and friendly atmosphere is encouraged during the courses so that the students can overcome their inhibitions and actively participate in the discussions. ​&lt;/p&gt;

&lt;p style="text-align:justify"&gt;&lt;em&gt;&lt;u&gt;&lt;strong&gt;Organizing Committee&lt;/strong&gt;&lt;/u&gt;&lt;/em&gt;&lt;/p&gt;

&lt;p style="text-align:justify"&gt;Dr. Isabel Pedraza Morales (President DPyC-SMF) [BUAP]&lt;br /&gt;
Dr. Humberto G. Maury Cuna (Vice-President DPyC-SMF)&amp;nbsp;[UGTO]&lt;/p&gt;

&lt;p style="text-align:justify"&gt;&lt;em&gt;&lt;u&gt;&lt;strong&gt;Local Organizing Committee&lt;/strong&gt;&lt;/u&gt;&lt;/em&gt;&lt;/p&gt;

&lt;p style="text-align:justify"&gt;Dr. Haydee Hern&amp;aacute;ndez [BUAP]&lt;br /&gt;
Dr. Arturo Fern&amp;aacute;ndez [BUAP]&lt;br /&gt;
Dr. Humberto Salazar [BUAP]&lt;br /&gt;
Dr. Olga F&amp;eacute;lix Beltr&amp;aacute;n [BUAP]&lt;/p&gt;
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 <name>Puebla</name>
 <address>1. Edificio Carolino, Calle 4 Sur 104, Centro, Puebla, Puebla.
2. Ciudad Universitaria 2, Calle Heberto Rodríguez N°119, Colonia San Antonio Toluquilla, C.P. 72960, San Pedro Zacachimalpa, Puebla</address>
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<startDate>2026-10-19T07:30:00</startDate>
<endDate>2026-10-23T19:30:00</endDate>
<creationDate>2026-07-01T10:52:23</creationDate>
<modificationDate>2026-10-30T16:10:28</modificationDate>
<timezone>Mexico/General</timezone>
<chair>
 <user>
  <title>Prof.</title>
  <name first="Isabel" middle="" last="Pedraza"></name>
  <organization>Benemérita Universidad Autónoma de Puebla</organization>
  <emailHash>65efd11437264d48aa1f7486255a57bc</emailHash>
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  <title>Dr.</title>
  <name first="Humberto" middle="" last="Maury Cuna"></name>
  <organization>Universidad de Guanajuato</organization>
  <emailHash>0bba80e6b6d806cda49089f089616ab2</emailHash>
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 <user>
  <title>Dr.</title>
  <name first="Haydee" middle="" last="Hernandez-Arellano"></name>
  <organization>BUAP</organization>
  <emailHash>5848375cb8b0db28e94350f19dcb744f</emailHash>
 </user>
 <user>
  <title>Dr.</title>
  <name first="Beltran" middle="" last="Felix"></name>
  <organization>Benemerita Universidad Autonoma de Puebla</organization>
  <emailHash>398909c50ebb53abfbd6c5540e4e5066</emailHash>
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 <title>Hidden Vector Dark Matter Phenomenology</title>
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   <title>Mr.</title>
   <name first="Juan" middle="" last="Jimenez Roman"></name>
   <organization>Instituto de Física, UNAM</organization>
   <emailHash>8508fa6f9835480ef9ccb7b47513b20f</emailHash>
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   <title>Mr.</title>
   <name first="Juan" middle="" last="Jimenez Roman"></name>
   <organization>Instituto de Física, UNAM</organization>
   <emailHash>8508fa6f9835480ef9ccb7b47513b20f</emailHash>
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   <title>Dr.</title>
   <name first="Maria Catalina" middle="" last="Espinoza-Hernandez"></name>
   <organization>Instituto de Fisica, UNAM.</organization>
   <emailHash>cdd1b1e9c22b6f1743dd72d03dc22c5b</emailHash>
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  <name>Puebla</name>
  <address>1. Edificio Carolino, Calle 4 Sur 104, Centro, Puebla, Puebla.
2. Ciudad Universitaria 2, Calle Heberto Rodríguez N°119, Colonia San Antonio Toluquilla, C.P. 72960, San Pedro Zacachimalpa, Puebla</address>
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 <startDate>2026-10-20T18:30:00</startDate>
 <endDate>2026-10-20T18:40:00</endDate>
 <duration>00:10</duration>
 <abstract>This work investigates the phenomenology of a vector dark matter model based on an additional hidden gauge symmetry, (SU(2){HS}), introduced through a scalar doublet (\Phi). The scalar potential exhibits a global (SO(4)) symmetry, which is spontaneously broken by the vacuum expectation value of (\Phi), giving mass to the new gauge bosons (A\mu^i). The resulting custodial (SO(3)) symmetry ensures their mass degeneracy and stability, making them viable dark matter candidates.

The model is tested through a statistical analysis of the dark matter relic density and direct detection cross-section. Its parameter space is explored using publicly available numerical tools, incorporating constraints from XENON1T, Planck, and LHC Higgs measurements, as well as collider searches for the additional scalar, perturbative unitarity, and vacuum stability.

The resulting likelihood analysis shows that the model can explain either part or all of the observed dark matter abundance while offering promising prospects for detection in future direct detection experiments.</abstract>
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