Cross-Correlation of Cosmic Fields
Principal Investigator: Carlo Baccigalupi
Area:
- Astroparticle Physics
- Early Universe
- Structures in the Universe and Emergent Phenomena
- Theory and Phenomenology of Gravity
Abstract: Probing the cross-correlation between tracers of the Large Scale Structure (LSS) and Early Universe (EU) is one the most important front for assessing the robustness of the Lambda Cold Dark Matter Cosmology, in particular for what concerns the process of Galaxy Formation and Evolution, the physical properties of the Dark Energy and Matter. Existing projects, such as the Euclid satellite, the Squared Kilometer Array, the Linear Interferometer Gravitational Observatory (LIGO/VIRGO), the Large Scale Structure Telescope (LSST), the Laser Interferometer Space Antenna (LISA) are either operational or in preparation for this entire decade and beyond; they target Cross-Correlation measurements as most impotant ones. Members of the present proposal have responsibility roles in the preparatory work for these efforts and the subsequent exploitation of the data.This line of research at the IFPU exploits the unique location to gather all interested scientists in order to achieve coordination between various projects, growth of collaborations, production of original investigations, and maximizing the return from the results of ongoing observations.
Status of project and perspectives: The IFPU has hosted research on Cross-Correlation of Cosmic Fields, representing a cross-over for modern astrophysics and cosmology. The knowledge of Stellar Physics, Emitters of Gravitational Waves, Galaxy Formation and evolution, and their interplay with the Dark Matter and the Dark Energy in the Large Scale Structure and Cosmic Microwave Background are aspects which need to be connected and coordinated in order to maximize their impact. Affiliated scientists and visitors and working at the IFPU have been producing an impressive list of publications concerning these aspects, and have organized in particular the annual meeting of the Cosmic Microwave Background cross-correlation Working Group within the Euclid Consortium ( https://indico.sissa.it/event/55/). The IFPU offers an unique opportunity for scientists working at the different aspects to gather together in a single space, working on specific aspects, as well as overviewing the whole efforts, hosting dedicated meetings, scientific visits, and workshops. Activities are based on brainstormings and meetings on a weekly basis at the IFPU, spending at the institute 1 or 2 days per week, as well as organizing regular seminars at the site. Moreover, visits, dedicated and focussed meetings, and workshops throughout the academic year will be organized. The activities will be constantly mirrored on the IFPU site and will be set in coordination with members from the four founding institutions.
Co-PIs:
Publications:
- Detectability of the Cross-Correlation between CMB Lensing and Stochastic GW Background from Compact Object Mergers
- Exploring galaxies-gravitational waves cross-correlations as an astrophysical probe
- Intensity and anisotropies of the stochastic gravitational wave background from merging compact binaries in galaxies
- Detectability of the τes-21cm cross-correlation: a tomographic probe of patchy reionization
- Exploring galaxies-gravitational waves cross-correlations as an astrophysical probe
- Special Issue on “Cross Correlation of Cosmic Fields: A Powerful Statistical Tool for Astrophysics, Cosmology, and Fundamental Physics”, eds. A. Lapi and C. Baccigalupi, Universe
- Cosmic Voids and BAO with relative baryon-CDM perturbations
- Quantifying the impact of baryon-CDM perturbations on halo clustering and baryon fraction
- SCAMPY – A sub-halo clustering and abundance matching based PYTHON interface for painting galaxies on the dark matter halo/sub-halo hierarchy
- Euclid preparation: XVIII. Cosmic Dawn Survey. Spitzer observations of the Euclid deep fields and calibration fields
- Euclid preparation: XIX. Impact of magnification on photometric galaxy clustering
- Euclid preparation: XVI. Exploring the ultra low-surface brightness Universe with Euclid/VIS
- Euclid preparation: I. The Euclid Wide Survey
- Euclid Preparation: XIV. The Complete Calibration of the Color-Redshift Relation (C3R2) Survey: Data Release 3
- Euclid preparation: XV. Forecasting cosmological constraints for the Euclid and CMB joint analysis
- Euclid preparation: XIII. Forecasts for galaxy morphology with the Euclid Survey using Deep Generative Models
- Growth of Massive Black Hole Seeds by Migration of Stellar and Primordial Black Holes: Gravitational Waves and Stochastic Background
- Euclid preparation: XII. Optimizing the photometric sample of the Euclid survey for galaxy clustering and galaxy-galaxy lensing analyses
- Euclid preparation: XI. Mean redshift determination from galaxy redshift probabilities for cosmic shear tomography
- Euclid preparation: IX. EuclidEmulator2 – Power spectrum emulation with massive neutrinos and self-consistent dark energy perturbations
- Euclid preparation: X. The Euclid photometric-redshift challenge
- Measuring the spectrum of primordial gravitational waves with CMB, PTA and Laser Interferometers
- Constraints on the Spacetime Dynamics of an Early Dark Energy Component
- Merging Rates of Compact Binaries in Galaxies: Perspectives for Gravitational Wave Detections
- Evidence for the Cross-correlation between Cosmic Microwave Background Polarization Lensing from POLARBEAR and Cosmic Shear from Subaru Hyper Suprime-Cam
- Cross-correlation of POLARBEAR CMB Polarization Lensing with High-z Sub-mm Herschel-ATLAS galaxies