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XXXVI Reunión Anual de la División de Partículas y Campos

8-10 September 2022
Virtual
Mexico/General timezone
XXXVI Annual Meeting of the Division of Particles and Fields
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Short talks I

Place

Location: Virtual
Room: https://us06web.zoom.us/j/85040775843?pwd=ZnRsQkgxKzBPdStoY0Z5OU5QQ3p4QT09
Date: 8 Sep 10:30 - 11:30

Conveners

  • QCD and Hadron Physics
    • Dr. Castañeda, Alfredo (UNISON)

Timetable | Contribution List

Displaying 4 contributions out of 4
Type: Contributed Talks Session: Short talks I
We investigate the proposal by Kharzeev and Levin of a maximally entangled proton wave function in Deep Inelastic Scattering of electrons and proton in the region of low Bjorken x. Using their proposed relation between parton number and entanglement entropy, we determine the latter using both conventional parton distribution functions and parton distribution functions obtained from an unintegrated ... More
Presented by Dr. Martin HENTSCHINSKI on 8/9/2022 at 15:50
Type: Contributed Talks Session: Short talks I
In this talk, a collection of pion structural properties that can be addressed via Continuum Schwinger Methods are discussed. We shall focus on a novel computation of gravitational form factors (GFFs). GFFs exhibit an intimate connection with the energy-momentum tensor in QCD, thus enabling access to the mass distribution inside the pion, as well as pressure and shear forces. The results present ... More
Presented by Khépani RAYA on 8/9/2022 at 16:10
Session: Short talks I
A measurement of the primary Lund jet plane density in inclusive jet production in proton-proton collisions is presented. The Lund jet plane, a representation of emissions inside jets, is extracted using iterative jet declustering techniques. The transverse momentum kT and the splitting angle ΔR of an emission relative to its emitter are measured at each step of the jet declustering process. The ... More
Presented by Cristian BALDENEGRO BARRERA on 8/9/2022 at 15:30
Type: Contributed Talks Session: Short talks I
The mass composition of primary cosmic rays is deduced from the sensitivity of the observables that can be obtained when the distribution of the measured quantities is compared with hadronic models for different types of primary particles, these models usually make an extrapolation of the parameters to ultra-high energies (of the order of tens of TeV) where measurements from ultra-energetic cosmic ... More
Presented by Mr. Alejandro CONTRERAS MUNIVE
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