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 <user>
  <title>Dr.</title>
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<title>RADPyC2026</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, 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 Wednesday 17 June and end before lunch on Friday 19 June.

We will have the following invited talks:
 
- Ana Colmenero, HAWC (UMSNH)

- Jens Erler, The EW SM and constraints on NP (Mainz, PRISMA)

- Iván Martínez Soler, Neutrino physics (Durham Univ.)

- Cristina Oropeza, CMS (Ibero)

- Antonio Ortiz, ALICE (ICN-UNAM)

- Gabriel Palacios, Accelerator physics (UNAM)

- Antonio Pich, Flavor physics (IFIC)

- Pedro Podesta, Belle-II (UAS)

- Selomit Ramírez, QCD, Loop Tree Duality, Quantum Computing (UAS)

- Saúl Ramos, Flavor physics from a top-down perspective (IF-UNAM)

- Alfredo Raya, NICA (UMSNH)

- Eric Vázquez, DM-neutrinos (exp.) (IF-UNAM)


The whole event can be followed by Zoom:

https://us02web.zoom.us/j/85815121456?pwd=t1JWdqhgarEQRyewmXIEzNlkIcqU8a.1

(858 1512 1456 &amp; 044752).

Due to recent internet security problems at Cinvestav it will NOT be broadcasted via the DPyC facebook account (facebook is currently blocked on our premises).</description>
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<startDate>2026-06-17T09:00:00</startDate>
<endDate>2026-06-19T14:30:00</endDate>
<creationDate>2026-03-23T09:50:55</creationDate>
<modificationDate>2026-06-19T17:51:55</modificationDate>
<timezone>Mexico/General</timezone>
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  <name first="Gabriel" middle="" last="Lopez Castro"></name>
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  <organization>CINVESTAV-IPN Mexico</organization>
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 </user>
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  <title>Dr.</title>
  <name first="Pablo" middle="" last="Roig"></name>
  <organization>Cinvestav</organization>
  <emailHash>ea481e58ca9c64e14d7982cb66bcd604</emailHash>
 </user>
 <user>
  <title>Dr.</title>
  <name first="Pablo" middle="" last="Roig"></name>
  <organization>Cinvestav</organization>
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  <title>Prof.</title>
  <name first="Isabel" middle="" last="Pedraza"></name>
  <organization>Benemérita Universidad Autónoma de Puebla</organization>
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 <title>Nuclear Fano factor effect for Dark Matter and CE$\nu$NS detection</title>
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   <title>Dr.</title>
   <name first="Juan Carlos" middle="" last="D'Olivo"></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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 <duration>00:15</duration>
 <abstract>Dark matter direct detection and Coherent Elastic Neutrino-Nucleus Scattering (CE$\nu$NS) represent two of the primary frontiers for discovering new particles and exploring physics beyond the Standard Model (SM). Accurately identifying these rare signals requires a precise reconstruction of the ionization signal produced by a recoiling atom. This cascade process partitions the primary nuclear recoil energy into electronic excitation and nuclear motion, a relationship quantified by the ionization efficiency, or quenching factor (QF). While the mean QF is conventionally determined using the first moment of the Lindhard integral equation, this work derives the integral equation for the second moment. By solving the resulting second-order integro-differential equation, we define a "nuclear Fano factor" that characterizes the statistical fluctuations inherent to the ionization efficiency, particularly in the low-energy regime. Finally, we evaluate the impact of these reconstruction effects on event rates and discuss the higher-order statistical implications of nuclear skewness and  kurtosis excess.</abstract>
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