São Paulo Research Group meetings in Astro & Cosmo

Next meeting: August 29, 2025
São Paulo, Brazil
Venue: Instituto Principia
Zoom id: 862 0094 6662
Password: cosmo
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Organizers:
- Raul Abramo (IFUSP)
- Chee Sheng Fong (UFABC)
- Rogério Rosenfeld (IFT-UNESP)
- Riccardo Sturani (IFT-UNESP)
Announcement:
Invited Speakers
- 11:00 Alexandre Le Tiec (IFT-UNESP — CNRS): What’s in a Name: the Anthropocene”
Can we continue to sustain forms of social organization sufficiently stable and complex to guarantee the ongoing pursuit of the exploration of the Universe—and to do so in a manner that proves durable over time? Confronted with the exhaustion of fossil energy resources, the destabilization of the global climate, and the manifold devastations of ecological systems, the very possibility of the modern scientific enterprise is placed under profound scrutiny. Through an interdisciplinary investigation mobilizing an extensive corpus of knowledge from both the natural sciences and the humanities and social sciences, we shall endeavor to trace the genealogical roots of the Anthropocene.
- 14:00 Fernanda Lima (IF-USP): Ultra-light dark matter and power spectra emulators
The nature of dark matter constitutes one of the main open questions in contemporary physics. In cosmological scales, we have a remarkable success of the cold dark matter description in explaining precise observations. However, in scales below Mpc, the dark matter behavior is not precisely constrained. This motivates the study of models that have different phenomenologies in small scales, such as ultra-light dark matter. In this talk, I will briefly present this class of dark matter candidates and discuss the utility of building emulators to calculate its power spectra in the context of parameter inference. - 15:15 João Ferri (IF-USP): What can we gain from small scales in shear analysis? A comparison between Fourier and Real spaces.
Abs: A known problem in cosmic shear two-point statistics is the apparent inconsistency between analyses done in harmonic/Fourier space (power spectrum) and real space (angular correlation). This arises from the fact that scale cuts in one space correspond to “soft” cuts in the other, as the relationship between these two spaces is given by Bessel functions. For the same reason, astrophysical effects that are compact in one space may not be in the other, which can lead to biased parameter estimation. I will present the consequences of pushing the boundaries of our analyses to smaller scales in both spaces, accounting for different models of Intrinsic Alignment and Baryonic Feedback in HSC Y3 data.
Previous Meetings
- 10:00 Walter Riquelme (IFT-UNESP): Imprints of Large-Scale Structures in the Anisotropies of the Cosmological Gravitational Wave Background – Video
- 11:15 Ricardo Medina (UFEI): Determining self-force corrections to the equation of the separatrix of a Schwarzschild black hole – Video
- 14:00 Gustavo Figueiredo Severiano Alves (IF-USP): Chasing Serendipity: Tackling Transient Sources with Neutrino Telescopes – Video
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- 10:00 Pedro Bittar (USP): Baryogenesis just around the corner: Generating the matter asymmetry at or below the weak scale – Video
- 11:15 Rodrigo Voivodic (Donostia Int. Physics Cent. San Sebastian & IFT-UNESP): Likelihoods – Video
- 14:00 Gustavo Henrique dos Santos (UFABC): ACT Constraints on Low Scale Inflation and a Mechanism for Vector Dark Matter Production – Video
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- 10:00 Parth Bambhaniya (USP): Are We Sure It’s a Supermassive Black Hole at the Heart of Our Galaxy? – Video
- 11:15 Natalia Villa Rodrigues (USP) : Modeling halo bias with neural networks – Video
- 14:00 Vitor Sampaio (UNICID): Disks and Spheroids across cosmic time: Morphological and Star Formation Evolution of Galaxies from z = 2.4 to z = 0.2 – Video
March 14, 2025
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10:00 Jorge Luiz Meléndez Moreno (IAG, USP): Solar Twins and their implications for Planets, Stars and the Galaxy – Video
Participants List: Here
2024
November 8, 2024
- 10:00 Abdias Aires (IFT-UNESP): Mitigation of nonlinear galaxy bias with theoretical-error likelihood – Video
- 11:00 Giorgio Torrieri (Unicamp): Non-local effective field theory in general relativity – Video
- 14:00 Daniel Lopez-Cano (IF-USP): Machine Learning Applications in Cosmology: Past, Present, and Future – Video
Participants List: Here
October 11, 2024
- 10:00 Walter Riquelme (IFT/UNESP): Unveiling the initial conditions of the universe with galaxy surveys – Video
- 11:00 Yago Porto (UFABC): Flavor Matters, but Matter Flavors: Matter Effects on Flavor Composition of Astrophysical Neutrinos – Video
- 14:00 Lilianne Nakazono (USP): Searching for quasars in the era of large multi-wavelength datasets – Video
Participants List: Here
September 13, 2024
- 10:00 – João Victor Silva (IFT UNESP): Dynamical Dark Energy and Massive Neutrinos in Light of DESI 2024 BAO – Video
- 11:00 – Lia Doubrawa (IAG USP): Galaxy clusters in photometric surveys: detection and analysis – Video
Participants List: Here
August 16, 2024
- 10:00 – Edivaldo Moura Santos (USP): The ultra-high energy cosmic ray sky – Video
- 11:00 – João Vitor Dinarte Ferri (USP): A cosmic standard ruler from the cross-correlations of galaxies and dark sirens – Video
- 14:00 – Natali de Santi (USP São Carlos): Cosmology with graph neural networks – Video
Participants List: Here
June 14, 2024
- 10:00 – Nickolas de Aguiar Alves (UFABC): Don’t forget about the memory
- 11:00 – Reinaldo de Carvalho (UNICID): Studies on Galaxy Morphology: Diving into the Primordial Era
- 14:00 – Isabela Santiago de Matos (IFT-UNESP): Cosmological tests with bright and dark standard sirens
Participants List: Here
May 10, 2024
- 10:00 – Lucas Gabriel Silva (IAG USP): Galaxy cluster mass estimation using the splashback radius
- 11:00 – Adriana Valio (Mackenzie): Exoplanetas: atmosferas e habitabilidade
- 14:00 – Carol Guandalin (Institute for Astronomy (IfA), University of Edinburgh): I see bispectrum everywhere
April 12, 2024
- 10:00 – Rodrigo Voivodic (Donostia Intl. Phys. Ctr., San Sebastian): The Hybrid Lagrangian Perturbation Theory
- 11:00 – Louis Legrand (ICTP-SAIFR): Next generation galaxy and CMB surveys: optimal estimators and cross-correlations
- 14:00 – Chee Sheng Fong (UFABC): How much baryon asymmetry and dark matter can be generated from primordial black holes?
Announcement:
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Photos
Additional Information
How to reach the Principia Institute: The meeting will be held in the first-floor auditorium of the Science Center at Principia Institute located at Rua Pamplona, 145 near the Trianon-Masp metro station.