III Joint ICTP-SAIFR/ICTP-Trieste School on Particle Physics

There is no registration fee and limited funds are available for travel and local expenses.

This activity will be followed by the Second School on Dark Matter and Neutrino Detection from July 8 to 19.

Organizers:

• Gustavo Burdman (IFUSP)
• Joan Elias Miró (ICTP-Trieste)
• Rogerio Rosenfeld (IFT-UNESP/ICTP-SAIFR)
• Giovanni Villadoro (ICTP-Trieste)

List of participants: Updated on June 18, 2024.

Announcement:

Application is now closed

Lecturers:

Announcement:

Application is now closed

 The schedule might be changed.

• Adrián Moreno (Universidad de Granada): Functional two-loops matching
• Adrián Moreno Sánchez – PhD Student (Universidad de Granada): Functional Matching at two-loop order
• Ajdin Palavric (University of Basel): Leading directions and RG effects in the SMEFT
• Ana Luisa Foguel (Instituto de Física, Universidade de São Paulo): Exploring General Vector Mediators in Inelastic Dark Matter Models
• Andrea (Universidad Autónoma de Madrid (UAM)): Di-Higgs production with quantum corrections
• Daniel Aguiar (UFMG): Relics of a Bubbling Universe – First Order Phase Transitions and Their Cosmological Implications
• Fuensanta Vilches Bravo (Universidad de Granada): On Shell Matching
• Israel Hernández  (Higher Institute of Technologies and Applied Sciences): Neutrino oscillations and spontaneous breaking of Lorentz symmetry.
• Luis Gil (FTAE, Universidad de Granada): Dimensionally reduced EFTs for cosmological phase transitions
• Nicolás Avalos (Instituto Balseiro): Searching for Dark Matter in the Southern Cone with Skipper CCDs
• Sergio Manuel Cubides Pérez (GIRG-UIS): Leptogenesis
• Somasundaram Sankaranarayanan (Weizmann Institute of Science): Implications of quadratic and shift-symmetric coupling of Dark Matter to Standard Model fields
• Yoxara Sánchez Villamizar (UFABC): BSM Searches at the LHC with SModelS v3

• Ricardo César Silva Rêgo (Universidade Federal do Rio Grande do Norte (UFRN)): e+ e- colisions at CLIC considering a new Z’ boson
• Tamara Petrosillo Lago (Universidad Técnica Federico Santa María): Neutrino floor calculation: a background for the direct detection of WIMPs.
• Amanda Malagi (Federal University of Paraná): Aspects of a functional measure in the electroweak sector of the Standard Model
• Leticia Maria Valença Guedes (Universidade Federal do Rio Grande do Norte): Constraining Gamma-ray Lines from Dark Matter Annihilation using Fermi-LAT and H.E.S.S. data
• Jorge Schifferli Verdugo (Universidad técnica Federico Santa María): Exploring Unitarity-Completing Extensions of a Dark Matter Model via SO(4) Symmetry
• Monalisa Melo (Instituto de Física da USP): Study of the medium effects in jet observables in relativistic heavy-ion collisions
• Gabriel Brandao de Gracia (Unesp-IFT): On Wigner Degeneracy in Elko theory: Hermiticity and Dark Matter Phenomenological Constraints
• Gabriel Aragão (Federal University of ABC): Understanding the reheating dynamics and baryogenesis
• MARIANO JESUS EFFIO CUEVA (National University of Engineering): Cross Section Calculation for ηc Meson in Various Wave Function Models
• Alejandra Sabed Cervantes Perdomo (Benemérita Universidad Autónoma de Puebla): Direct and indirec detection of DM in 2S-SM
• Antonio Carlos Samaniego Flores – Master’s student (Institute of Physics, UNAM): S3-Modular Symmetry in Guts

• 09:00 - Christophe Grojean (DESY, Germany): Standard Model and Beyond - Class 1
  • Attachment
• 11:00 - Kfir Blum (Weizmann Institute, Israel): Cosmology and Particle Physics - Class 1
• 15:30 - Laura Reina (Florida State University, USA): Collider Physics - Class 1
  • Attachment

• 09:00 - Christophe Grojean (DESY, Germany): Standard Model and Beyond - Class 2
• 11:00 - Kfir Blum (Weizmann Institute, Israel): Cosmology and Particle Physics - Class 2
• 15:30 - Laura Reina (Florida State University, USA): Collider Physics - Class 2
  • Attachment

• 09:00 - Christophe Grojean (DESY, Germany): Standard Model and Beyond - Class 3
• 11:00 - Kfir Blum (Weizmann Institute, Israel): Cosmology and Particle Physics - Class 3
  • Attachment
  • Additional info
• 14:00 - Christophe Grojean (DESY): Future Circular Collider: What? Why? When?
  • Abstract
• 15:30 - Laura Reina (Florida State University, USA): Collider Physics - Class 3

• 09:00 - Christophe Grojean (DESY, Germany): Standard Model and Beyond - Class 4
• 11:00 - Kfir Blum (Weizmann Institute, Israel): Cosmology and Particle Physics - Class 4
• 15:30 - Laura Reina (Florida State University, USA): Collider Physics - Class 4
  • Attachment

• 09:00 - Christophe Grojean (DESY, Germany): Standard Model and Beyond - Class 5
• 11:00 - Kfir Blum (Weizmann Institute, Israel): Cosmology and Particle Physics - Class 5
• 15:30 - Laura Reina (Florida State University, USA): Collider Physics - Class 5
  • Attachment

• 09:00 - Nicolás Bernal (New York University Abu Dhabi, United Arab Emirates): Dark Matter - Class 1
• 11:00 - Yu-tin Huang (National Taiwan University, Taiwan): Amplitudes and applications - Class 1
• 14:00 - Markus Luty (University of California at Davis, USA): Formal developments in Beyond Standard Models - Class 1

• 09:00 - Nicolás Bernal (New York University Abu Dhabi, United Arab Emirates): Dark Matter - Class 2
• 11:00 - Yu-tin Huang (National Taiwan University, Taiwan): Amplitudes and applications - Class 2
• 14:00 - Markus Luty (University of California at Davis, USA): Formal developments in Beyond Standard Models - Class 2

• 09:00 - Nicolás Bernal (New York University Abu Dhabi, United Arab Emirates): Dark Matter - Class 3
• 11:00 - Yu-tin Huang (National Taiwan University, Taiwan): Amplitudes and applications - Class 3
• 14:00 - Markus Luty (University of California at Davis, USA): The Higgs Boson: A Tale of Possible Universes
  • Abstract
• 15:30 - Markus Luty (University of California at Davis, USA): Formal developments in Beyond Standard Models - Class 3

• 09:00 - Nicolás Bernal (New York University Abu Dhabi, United Arab Emirates): Dark Matter - Class 4
• 11:00 - Yu-tin Huang (National Taiwan University, Taiwan): Amplitudes and applications - Class 4
• 14:00 - Markus Luty (University of California at Davis, USA): Formal developments in Beyond Standard Models - Class 4

• 09:00 - Nicolás Bernal (New York University Abu Dhabi, United Arab Emirates): Dark Matter - Class 5
• 11:00 - Yu-tin Huang (National Taiwan University, Taiwan): Amplitudes and applications - Class 5
• 14:00 - Markus Luty (University of California at Davis, USA): Formal developments in Beyond Standard Models - Class 5

Attention! Some participants in ICTP-SAIFR activities have received email from fake travel agencies asking for credit card information. All communication with participants will be made by ICTP-SAIFR staff using an e-mail “@ictp-saifr.org”. We will not send any mailings about accommodation that require a credit card number or any sort of deposit.

BOARDING PASS: All participants, whose travel has been provided or will be reimbursed by ICTP-SAIFR, should bring the boarding pass  upon registration. The return boarding pass (PDF, if online check-in, scan or picture, if physical) should be sent to secretary@ictp-saifr.org by e-mail.

COVID-19: Brazilians and foreigners no longer have to present proof of vaccination before entering the country.

Visa information: Nationals from several countries in Latin America and Europe are exempt from tourist visa. Nationals from Australia, Canada and USA are exempt from tourist visa until April 10, 2025. Please check here which nationals need a tourist visa to enter Brazil.

Accommodation: Participants, whose accommodation will be provided by the institute, will stay at The Universe Flat. Hotel recommendations are available here.

How to reach the Institute: The school will be held at ICTP South American Institute, located at IFT-UNESP, which is across the street from a major bus and subway terminal (Terminal Barra Funda). The address which is closer to the entrance of the IFT-UNESP building is R. Jornalista Aloysio Biondi, 120 – Barra Funda, São Paulo. The easiest way to reach us is by subway or bus, please find instructions here.

Poster presentation: Participants who are presenting a poster MUST BRING A PRINTED BANNER . The banner size should be at most 1 m (width) x 1,5 m (length). We do not accept A4 or A3 paper. Click here to see what a banner looks like: http://designplast.ind.br/produtos/detalhe/impressao-digital/banner/119/9