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  <title>Dr.</title>
  <name first="Pablo" middle="" last="Roig"></name>
  <organization>Cinvestav</organization>
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<title>RADPyC2023</title>
<description>The Division of Particles and Fields of the Mexican Physical Society (DPyC-SMF) organizes every year the Annual Meeting (RADPyC). This space is dedicated mainly for the exposure of results of graduate students and young researchers working in high energy physics and includes some review talks on the hot topics of the field. This year the meeting will be held in Auditorio José Ádem (Multidisciplinario for Wednesday), Cinvestav, Mexico City, México. The scientific programme will consist of invited and contributed talks, and a poster session. It will begin in the morning of Monday 12 June and end before lunch on Wednesday 14 June.

We will have the following invited talks:

- ALICE status update, Gerardo Herrera Corral (Cinvestav)

- Belle-II status update, Pedro Podesta (UAS)

- CMS status update, Rogelio Reyes (Cinvestav)

- Dirac or Majorana nature of neutrinos, C.S. Kim (Yonsei Univ, South Korea)

- Flavor symmetries, Myriam Mondragón (IF-UNAM)

- Grand Unified Theories, Carlos Vaquera (Conacyt &amp; IF-UG)

- Looking for CEvNS of reactor antineutrinos with the CONNIE Experiment, Alexis Aguilar-Arévalo (ICN-UNAM)

- Machine Learning techniques in high energy colliders, Roger Hernández-Pinto (UAS)

- Theoretical perspectives on hep, Lorenzo Díaz-Cruz (BUAP)

The whole event can be followed by Zoom:

https://us06web.zoom.us/j/82178499407?pwd=WG96WXZ2ek9ScE1pSTRvdHc0RExOUT09

 
Meeting ID: 821 7849 9407

Passcode: 992552

and will be broadcasted via the DPyC facebook account.</description>
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<startDate>2023-06-12T08:30:00</startDate>
<endDate>2023-06-14T18:30:00</endDate>
<creationDate>2023-05-04T17:25:28</creationDate>
<modificationDate>2023-09-03T22:11:22</modificationDate>
<timezone>Mexico/General</timezone>
<chair>
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  <title>Dr.</title>
  <name first="GAbriel" middle="" last="Lopez Castro"></name>
  <organization>cinvestav</organization>
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  <title>Dr.</title>
  <name first="Omar" middle="" last="Miranda"></name>
  <organization>Cinvestav</organization>
  <emailHash>b45925fc905052dd8f365f65d9c1cc54</emailHash>
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  <title>Prof.</title>
  <name first="Eduard" middle="" last="De La Cruz Burelo"></name>
  <organization>CINVESTAV-IPN Mexico</organization>
  <emailHash>207484e6583dd9c0c1af2f52ce04fdd8</emailHash>
 </user>
 <user>
  <title>Dr.</title>
  <name first="Pablo" middle="" last="Roig"></name>
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 <title>Topological defects in the O(2) model out of equilibrium</title>
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   <name first="Jaime Fabián" middle="" last="Nieto Castellanos"></name>
   <organization>ICN, UNAM</organization>
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   <title></title>
   <name first="Jaime Fabián" middle="" last="Nieto Castellanos"></name>
   <organization>ICN, UNAM</organization>
   <emailHash>49c1b3aa79f8e1033293efecdfde3590</emailHash>
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   <title>Dr.</title>
   <name first="Wolfgang" middle="" last="Bietenholz"></name>
   <organization>ICN, UNAM</organization>
   <emailHash>31a43f9098b4cb652d6bf53a1319aab7</emailHash>
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   <title></title>
   <name first="Edgar" middle="" last="López Contreras"></name>
   <organization>ICN, UNAM</organization>
   <emailHash>7be7a28b1c8c2499d6e770d45dc48866</emailHash>
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   <title>Dr.</title>
   <name first="Elías" middle="" last="Polanco"></name>
   <organization>ICN, UNAM</organization>
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 <duration>00:15</duration>
 <abstract>We present a study of the 2- and 3-dimensional O(2) model, or XY model, out of equilibrium through Monte Carlo simulations. In particular, we analyze the dynamics of the topological defects of the system (vortices) when we linearly lower the temperature at various cooling rates, starting above the critical temperature, $T_c$, down to $T &lt; T_c$. We test Zurek's prediction for the scaling behavior of the density of topological defects that remains after a cooling procedure for a system that undergoes a second order phase transition. We find that the remnant density depends on the cooling rate with a power law, in partial agreement with Zurek's prediction. This property is independent of the Monte Carlo algorithm that we choose. Still, the exact scaling behavior depends on the algorithm. A power law has also been observed in experiments of systems with continuous phase transitions. This approach could be extended to estimate the density of cosmic strings that persist from the expansion and cooling of the early universe, by simulating a more realistic model.</abstract>
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