Paulo Montero-Camacho PengCheng Lab
时间： 2022-12-01 14:00-2022-12-01 15:00
地点：Zoom Meeting ID: 987 9360 1531 Passcode: 202212
Cosmic reionization is the last major phase transition that our Universe goes through. In this milestone, the intergalactic medium transitions from primarily neutral, dark, and cold into mainly ionized, more luminous, and warmer. However, as exciting as the reionization process surely was, many aspects remain unknown, e.g. what are the sources of the ionizing photons? or what is the timeline of reionization? Current and upcoming telescopes (e.g. JWST and HERA/SKA) will directly probe cosmic reionization; nonetheless, interpretation of said measurements will strongly rely on modeling the surroundings of luminous objects (JWST) or on foreground removal (21 cm). In this talk, I will describe a promising novel method to constrain reionization through its impact on the post-reionization intergalactic medium using two promising probes of this era: the Lyman-alpha forest (e.g. DESI) and 21 cm line intensity mapping (e.g. PUMA/SKA). I will focus on both the astrophysics of reionization as a potential source of bias for cosmological analyses and as a promising new avenue to learn about the astrophysics that governs cosmic reionization and the standard cosmological model. Furthermore, I will showcase the potential of this effect to constrain the nature of dark matter via its exquisite small-scale sensitivity.
Paulo Montero-Camacho did his undergraduate studies at Universidad de Costa Rica, he then obtained his Ph.D. at The Ohio State University, USA, in 2019. Later, he joined prof. Yi Mao's group as a postdoctoral researcher and Shuimu scholar at the Department of Astronomy of Tsinghua University. Paulo will join Pengcheng Laboratory as a research assistant this autumn. Paulo has broad research interests in cosmology and astrophysics spanning the range from cosmic microwave background to primordial black holes and detection of magnetic fields in exoplanets. His current primary research interest lies in the study of the impact of inhomogeneous reionization in the intergalactic medium millions of years after hydrogen reionization has ended.