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  <title>Dr.</title>
  <name first="Lukas" middle="" last="Nellen"></name>
  <organization>ICN-UNAM</organization>
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<supportEmail caption="Support">proig@fis.cinvestav.mx</supportEmail>
<title>XXXI Reunión Anual de la División de Partículas y Campos de la SMF</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 (https://goo.gl/aUkCVe), Cinvestav, Mexico City, Mexico.


Invited review talks (preliminary titles): 

- CMS status report (Javier Murillo, Cinvestav-IPN)
- Belle-II status report (Emilie Passemar, Indiana Univ.)
- Forward physics and gluon at small x (Martin Hentschinski, UDLAP)
- Black holes everywhere (Omar López Cruz, INAOE)
- Loss of information in black hole evaporation? (Sujoy Modak, Colima Univ.)
- ALICE status report (Iraís Bautista, Conacyt-BUAP)
- Lepton flavor and CPV (Alex Stuart, Colima Univ.)
- New world leading limit on dark matter search from PICO experiment (Eric Vázquez Jáuregui, IF-UNAM)
- The discovery of gravitational waves (Juan Carlos Degollado, ICN-UNAM)
- New sources of CP violation (Agustín Moyotl, Cinvestav-IPN)
- Relación CERN-México: Resultado reciente de ALICE (Gerardo Herrera Corral, Cinvestav-IPN)
- Status of Long Baseline Neutrino Experiments at Fermilab (Fernanda Psihas, Indiana Univ.)

Registration fee:

    Students: 300 MXN
    Postdocs and professors: 500 MXN


It can be paid at the site of the conference or previously by bank transfer to the following account:

 Cliente: Sociedad Mexicana de Física, A.C.

 Banco: Banamex, S.A., Suc. 349

 No. de Cuenta: 1866151

 CLABE: 002180034918661519

 Referencia: RADPyC2017


 Deadline: 05/05/17

 Scholarships: There will be a limited number of scholarships covering the fee and accommodation. In this case, the students will share room.</description>
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 <name>Cinvestav-Zacatenco</name>
 <address>Physics Department, Cinvestav
Av. IPN 2508, Col. San Pedro Zacatenco, Del. Gustavo A. Madero, C.P. 07360 Ciudad de México</address>
 <room>José Ádem Auditorium</room>
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<startDate>2017-05-24T08:00:00</startDate>
<endDate>2017-05-26T19:25:00</endDate>
<creationDate>2017-02-24T19:13:25</creationDate>
<modificationDate>2021-03-24T19:23:41</modificationDate>
<timezone>Mexico/General</timezone>
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  <organization>Cinvestav</organization>
  <emailHash>ea481e58ca9c64e14d7982cb66bcd604</emailHash>
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  <organization>CINVESTAV-IPN</organization>
  <emailHash>9bf36ecbe9b65adb84a5bd4539767c02</emailHash>
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  <title>Dr.</title>
  <name first="Arturo" middle="" last="Fernandez Tellez"></name>
  <organization>Facultad de Ciencias Fisico Matematicas BUAP, Mexico</organization>
  <emailHash>81489ac17fbe3b967aba80a1a0143bf4</emailHash>
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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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 <title>Revealing the source of the radial flow patterns in proton–proton collisions using hard probes</title>
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   <title>Dr.</title>
   <name first="Antonio" middle="" last="Ortiz Velasquez"></name>
   <organization>ICN, UNAM</organization>
   <emailHash>3cc916d5f73ae193b3b29364a50e4b40</emailHash>
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   <name first="Gyula" middle="" last="Bencedi"></name>
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  <name>Cinvestav-Zacatenco</name>
  <address>Physics Department, Cinvestav
Av. IPN 2508, Col. San Pedro Zacatenco, Del. Gustavo A. Madero, C.P. 07360 Ciudad de México</address>
  <room>José Ádem Auditorium</room>
 </location>
 <duration>00:15</duration>
 <abstract>In this work (based on a recent published paper), we propose a tool to reveal the origin of the collective-like phenomena observed in proton–proton collisions. We exploit the fundamental difference between the underlying mechanisms, color reconnection and hydrodynamics, which produce radial flow patterns in Pythia 8 and Epos 3, respectively. Specifically, we proceed by examining the strength of the coupling between the soft and hard components which, by construction, is larger in Pythia 8 than in Epos 3. We study the transverse momentum (${p}_{{\rm{T}}}$) distributions of charged pions, kaons and (anti) protons in inelastic pp collisions at $\sqrt{s}=7$ TeV produced at mid-rapidity. Specific selections are made on an event-by-event basis as a function of the charged particle multiplicity and the transverse momentum of the leading jet (${p}_{{\rm{T}}}^{\mathrm{jet}}$) reconstructed using the FastJet algorithm at mid-pseudorapidity ($| \eta | \lt 1$). From our studies, quantitative and qualitative differences between Pythia 8 and Epos 3 are found in the ${p}_{{\rm{T}}}$ spectra when (for a given multiplicity class) the leading jet ${p}_{{\rm{T}}}$ is increased. In addition, we show that for low-multiplicity events the presence of jets can produce radial flow-like behavior. Motivated by our findings, we propose to perform a similar analysis using experimental data from LHC.</abstract>
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