8th Barcelona Initiative for Gravitation (BIG) Meeting
Friday, February 13, 2026 -
9:00 AM
Monday, February 9, 2026
Tuesday, February 10, 2026
Wednesday, February 11, 2026
Thursday, February 12, 2026
Friday, February 13, 2026
10:00 AM
Reception
Reception
10:00 AM - 10:30 AM
Room: Seminar room
10:30 AM
TBA
-
Nanda REA
(
ICE-CSIC UAB Barcelona
)
TBA
Nanda REA
(
ICE-CSIC UAB Barcelona
)
10:30 AM - 11:30 AM
Room: Seminar room
11:30 AM
Coffee
Coffee
11:30 AM - 12:00 PM
Room: Seminar room
12:00 PM
TBA
-
Ennio SALVIONI
(
UAB & IFAE
)
TBA
Ennio SALVIONI
(
UAB & IFAE
)
12:00 PM - 1:00 PM
Room: Seminar room
1:00 PM
Lunch
Lunch
1:00 PM - 2:30 PM
Room: Seminar room
2:30 PM
Tracing the Origin of the Nanohertz Gravitational Wave Background
-
Andrea MITRIDATE
(
Imperial College, London
)
Tracing the Origin of the Nanohertz Gravitational Wave Background
Andrea MITRIDATE
(
Imperial College, London
)
2:30 PM - 3:30 PM
Room: Seminar room
By tracking the radio pulses from an array of millisecond pulsars, several pulsar timing array collaborations have found evidence for a stochastic background of gravitational waves permeating our Galaxy. In this talk, I will briefly review how this evidence was obtained, then discuss ongoing efforts to identify the origin of the signal and explore its implications for cosmology and astrophysics. I will focus in particular on the challenges of mapping the sky distribution of the gravitational-wave power and on searches for non-Gaussian features in the background.
3:30 PM
Coffee
Coffee
3:30 PM - 4:00 PM
Room: Seminar room
4:00 PM
Temperature-Dependent CPT Violation: Constraints from Big Bang Nucleosynthesis
-
Anne-Katherine BURNS
(
Barcelona U
)
Temperature-Dependent CPT Violation: Constraints from Big Bang Nucleosynthesis
Anne-Katherine BURNS
(
Barcelona U
)
4:00 PM - 5:00 PM
Room: Seminar room
In this talk, I will explore temperature-dependent CPT violation during Big Bang Nucleosynthesis (BBN) modeled as an electron–positron mass asymmetry controlled by a finite-temperature background. Using a modified version of the BBN code PRyMordial with dynamically-solved chemical potentials and appropriate finite-mass corrections, my collaborator and I have constrained electron-positron mass differences using the observed abundances of Helium-4, Deuterium, and Neff. We find no region of parameter space consistent with all three observables at 1σ, though pairwise combinations yield allowed bands that tightly bound the mass asymmetry. I will present three toy models demonstrating how the type of CPT violation can arise from field-theoretic mechanisms, including temperature-driven phase transitions. The results that I will discuss provide the most stringent constraints on early-universe CPT violation in this regime, probing parameter space inaccessible to laboratory experiments.