20-26 October 2011
León, Guanajuato
Mexico/General timezone
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Place

Location: León, Guanajuato
Address: Prol. Calzada de los Héroes #308 Col. La Martinica, (FORUM CULTURAL GTO) LEON, GTO
Room: Auditorio Jorge Ibargüengoitia
Date: from 20 Oct 09:00 to 26 Oct 11:00

Conveners

  • 20 Oct 09:00 - 10:00 Electroweak and Flavor, R1
    • Dr. Díaz, Lorenzo (Instituto de Física BUAP)
  • 20 Oct 10:00 - 11:00 Astroparticles, Strings, Cosmology and Beyond the Standard Model, R2
    • Dr. Díaz, Lorenzo (Instituto de Física BUAP)
  • 20 Oct 16:30 - 17:30 Astroparticles, String, Cosmology and Beyond the Standard Model, R3
    • Dr. Sabido, Miguel (DCI)
  • 21 Oct 09:00 - 10:00 Hadronic Matter, R4
    • Dr. Kirchbach, Mariana (Instituto de Física de la Universidad Autónoma de San Luis Potosí)
  • 21 Oct 10:00 - 11:00 Hadronic Matter, R5
    • Dr. Kirchbach, Mariana (Instituto de Física de la Universidad Autónoma de San Luis Potosí)
  • 22 Oct 09:00 - 10:00 Electroweak and Flavor, R6
    • Dr. Delepine, David (DCI)
  • 22 Oct 10:00 - 11:00 Electroweak and Flavor, R7
    • Dr. Delepine, David (DCI)
  • 22 Oct 16:30 - 17:30 Electroweak and Flavor R8
    • Dr. Mondragón, Alfonso (IFUNAM)
  • 24 Oct 09:00 - 10:00 Astroparticles, Cosmology, Strings and Beyond the Standard Model, R9
    • Dr. Mondragón, Myriam (IFUNAM)
  • 24 Oct 10:00 - 11:00 Astroparticles, Cosmology, Strings and Beyond the Standard Model, R10
    • Dr. Mondragón, Myriam (IFUNAM)
  • 25 Oct 09:00 - 10:00 Hadronic Matter, R11
    • Dr. Bietenholz, Wolfgang (ICN-UNAM)
  • 25 Oct 10:00 - 11:00 Hadronic Matter, R12
    • Dr. Bietenholz, Wolfgang (ICN-UNAM)

Timetable | Contribution List

Displaying 12 contributions out of 12
Type: Plenary Revision Talk (1 hr) Session: Revision
Track: Hadronic Matter
In November 2009 the LHC at CERN started operation by colliding protons at 900 GeV in the center of mass. In March 2010 the accelerator reached its present maximum energy of 7 TeV for proton interactions. The first heavy ion run at 2.76 TeV/nucleon took place later, in November 2010. The PbPb accelerator run was very successful reaching a luminosity of approximately producing 30 million interac ... More
Presented by Dr. Gerardo HERRERA on 21/10/2011 at 14:00
Type: Plenary Revision Talk (1 hr) Session: Revision
Track: Astroparticles, Cosmology, Strings and Beyond the Standard Model
In this talk, we shall review the current status of string phenomenology, focusing on recent developments in string model building towards the MSSM and modern cosmology.
Presented by Dr. Saul RAMOS-SANCHEZ on 20/10/2011 at 21:30
Type: Plenary Revision Talk (1 hr) Session: Revision
Track: Electroweak and Flavor Physics
Understanding the observed masses and mixing angles of the known fermions has been an interesting challenge. Several ideas - some old some not so old - have been used in different settings in order to attempt an understanding with various degrees of success. In this talk we will briefly present some of the main ideas and venues explored so far starting with the more traditional (old) ones and then ... More
Presented by Dr. Alfredo ARANDA on 22/10/2011 at 15:00
Type: Plenary Revision Talk (1 hr) Session: Revision
Track: Electroweak and Flavor Physics
There is an increasing evidence for a non zero neutrino mass coming from an large number of neutrino experiments. Moreover, the new generation of experimental setups promise to improve the current measurements of the neutrino parameters and to address new problems such as CP violation in the neutrino sector. A strong effort to build models containing the neutrino mass pattern observed in r ... More
Presented by Dr. Miranda OMAR on 22/10/2011 at 21:30
Type: Plenary Revision Talk (1 hr) Session: Revision
Track: Electroweak and Flavor Physics
The two experimental facilities called B factories, one constructed at KEK, and another at SLAC, have played essential role in understanding CP asymmetry by providing experimental proof to the Kobayashi-Maskawa model. Also, more interestingly, both experiments noticed that some phenomena may not be understood in the framework of the theory. In other words, we may be seeing the first signals of ne ... More
Presented by Dr. Masa YAMAUCHI on 22/10/2011 at 14:00
Type: Plenary Revision Talk (1 hr) Session: Revision
Track: Astroparticles, Cosmology, Strings and Beyond the Standard Model
Many theoretical attempts at understanding the Planck-scale structure of spacetime can accommodate minute departures from Lorentz and CPT invariance. At presently attainable energies, such effects are expected to be accurately described within effective field theory. Such a field theory, in turn, can be employed to identify currently feasible experimental tests. This talk presents an ove ... More
Presented by Ralf LEHNERT on 24/10/2011 at 14:00
Type: Plenary Revision Talk (1 hr) Session: Revision
Track: Hadronic Matter
The study of open heavy-flavours and quarkonia production in heavy-ion collisions is expected to play an important role in understanding the properties of the Quark Gluon Plasma. In this talk, a review of recent experimental results on this subject is given. Particular attention is given to results that have been presented by the ALICE, ATLAS and CMS collaborations, although some results by RH ... More
Presented by Dr. Daniel TAPIA TAKAKI on 25/10/2011 at 15:00
Type: Plenary Revision Talk (1 hr) Session: Revision
Track: Hadronic Matter
We report on the basis of the so-called Unitary Chiral Perturbation Theory (UChPT) in terms of the N/D method. Several applications are reviewed with special emphasis on the mesonic scalar sector and its spectroscopy, the meson-baryon system and applications of ChPT in the nuclear medium. On going efforts on nucleon-nucleon interactions and covariant pion-nucleon scattering will be also reviewed. ... More
Presented by Dr. José Antonio OLLER on 25/10/2011 at 14:00
Type: Plenary Revision Talk (1 hr) Session: Revision
Track: Electroweak and Flavor Physics
The Standard Model of Particle physics is a spectacularly successful theory of elementary particles and their interactions, and the only missing piece is the higgs bosson, responsible of the mass of the particles and which has not been yet observed. However, for many years the experiments at the Tevatron collider, and now experiments at the Large Hadron Collider have been hunting this el ... More
Presented by Eduard DE LA CRUZ BURELO on 20/10/2011 at 14:00
Type: Plenary Revision Talk (1 hr) Session: Revision
Track: Astroparticles, Cosmology, Strings and Beyond the Standard Model
The Cosmic Frontier is the study of messenger particles that originate from the non-thermal universe. These messengers include cosmic rays, gamma rays, and neutrinos. Over the past decade we have made enormous progress in understanding the origin and propagation of these particles. We are now in a position to begin to turn these observations into scientific understanding of the cosmos. The cosm ... More
Presented by Dr. Gus SINNIS on 24/10/2011 at 15:00
Type: Plenary Revision Talk (1 hr) Session: Revision
Track: Astroparticles, Cosmology, Strings and Beyond the Standard Model
Doubtless the Lambda Cold Dark Matter (LCDM) model is one of the most successful models Science has created in the last time. Nevertheless, recently with the advance of new observational instruments, some problems of the model have been emerging. In this talk we speak about the successes and problems of the LCDM model and about some alternatives that could go beyond of LCDM.
Presented by Prof. Tonatiuh MATOS on 20/10/2011 at 15:00
Type: Plenary Revision Talk (1 hr) Session: Revision
Track: Hadronic Matter
Quantum chromodynamics (QCD) is the modern theory of the strong nuclear force. For many years, many of its amazing properties were believed to be true, but had not yet been demonstrated. In this review, I survey several results from lattice gauge theory, which start with the basic equations of QCD and then, via large-scale computing, establish these features. We now know, for example, how QCD g ... More
Presented by Dr. Andreas Kronfeld KRONFELD on 21/10/2011 at 15:00
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