Article
Astronomy & Astrophysics
Azadeh Moradinezhad Dizgah, Matteo Biagetti, Emiliano Sefusatti, Vincent Desjacques, Jorge Norena
Summary: Upcoming galaxy redshift surveys are expected to improve limits on primordial non-Gaussianity (PNG) through measurements in Fourier space. A Monte-Carlo Markov Chain analysis was performed to confront perturbation theory predictions with N-body simulations, focusing on the local model of PNG parameterized by f(NL). Informative priors on the linear non-Gaussian bias parameter can significantly improve constraints on f(NL) in statistical inference.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
Alexandre Barreira, Titouan Lazeyras, Fabian Schmidt
Summary: The study uses field-level forward models of galaxy clustering and EFT likelihood formalism to infer the relations between linear bias parameters (b(1), b(2), b(K2)) in self-consistently simulated galaxies. It finds that bias relations in total mass selected objects are broadly preserved in simulated galaxies selected by various characteristics, and shows good agreement with observed galaxy samples. The use of EFT likelihood also recovers sigma(8) values from different galaxy samples, demonstrating the potential of forward models in inferring cosmological information from galaxy data.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
Alexandre Barreira
Summary: In this study, hydrodynamical separate universe simulations with the IllustrisTNG model were used to predict the local primordial non-Gaussianity (PNG) bias parameters b(phi) and b(phi delta), which play a leading role in the analysis of galaxy power spectrum and bispectrum. It was found that the popular assumption of universality overpredicts the relation between b(phi delta) and linear density bias in the range of 1 ≤ b(1) ≤ 3 for dark matter halos. The study also revealed that the relations between b(phi)(b(1)) and b(phi delta)(b(1)) are redshift-dependent and sensitive to the selection of galaxies. The uncertainties in these bias parameters have a significant impact on the constraints of the local PNG parameter fnl. Moreover, it was shown that priors on galaxy bias are useful even in analyses that fit for products f(NL)b(phi) and f(NL)b(phi delta). The strategies discussed in this study can be implemented in existing f(NL) constraint analyses.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2022)
Article
Astronomy & Astrophysics
Joyce Byun, Andrea Oddo, Cristiano Porciani, Emiliano Sefusatti
Summary: This study compares the standard method of estimating the bispectrum with the compressed modal bispectrum method, finding that the latter provides consistent and competitive constraints. The modal bispectrum requires fewer expansion coefficients to achieve constraints comparable to the standard bispectrum estimator, demonstrating its efficiency in compression and constraint generation.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
Davide Gualdi, Sergi Novell, Hector Gil-Marin, Licia Verde
Summary: The study focuses on the power spectrum, bispectrum, and i-trispectrum, finding that the i-trispectrum provides significant improvements in constraining local primordial non-Gaussianity amplitude parameters. Using simulated data, the added-value provided by the i-trispectrum is quantified, showing up to a 32% reduction in constraints on f(nl) in redshift space compared to constraints obtained without the i-trispectrum.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
James M. Sullivan, Uros Seljak, Sukhdeep Singh
Summary: The updated Halo Zeldovich Perturbation Theory (HZPT) model provides an analytic and accurate description of the two-point statistics of dark matter on nonlinear scales, with applications to halo and galaxy clustering as well as galaxy-matter cross-correlation.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
ChangHoon Hahn, Michael Eickenberg, Shirley Ho, Jiamin Hou, Pablo Lemos, Elena Massara, Chirag Modi, Azadeh Moradinezhad Dizgah, Bruno Regaldo-Saint Blancard, Muntazir M. Abidi
Summary: Simulation-Based Inference of Galaxies (SIMBIG) is a forward modeling framework that uses simulation-based inference to analyze galaxy clustering. It accurately infers the parameters of galaxy clustering and effectively handles observational systematics. The framework has been validated through a mock challenge, demonstrating its robustness and capability to handle different statistical measures.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2023)
Article
Astronomy & Astrophysics
Dan Pryer, Robert E. Smith, Robin Booth, Chris Blake, Alexander Eggemeier, Jon Loveday
Summary: The study derives expressions for the galaxy power spectrum convolved by survey window in real space, considering the geometric lightcone effect for full sky and deep redshift surveys. It investigates the impact of using the standard mean redshift approximation, showing both overall amplitude suppression and scale-dependent error compared to the 'true' spectrum. However, it also demonstrates that accurate approximation to the full model can be achieved by carefully choosing an 'effective fixed-time' within a certain range of scales.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2022)
Article
Astronomy & Astrophysics
Marcel Schmittfull, Marko Simonovic, Mikhail M. Ivanov, Oliver H. E. Philcox, Matias Zaldarriaga
Summary: An analytical forward model based on perturbation theory was developed to predict the redshift-space galaxy overdensity, finding residual noise characteristics in simulated galaxy density. Furthermore, comparison of galaxy velocities revealed that about 10% of galaxies contribute to half of the rms velocity residual in the simulated galaxy sample.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
Setareh Foroozan, Elena Massara, Will J. Percival
Summary: The low resolution of slitless spectroscopy may lead to line misidentification in future surveys, requiring correction for contaminants to avoid incorrect cosmological measurements.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2022)
Article
Astronomy & Astrophysics
Miguel Aparicio Resco, Antonio L. Maroto
Summary: FARO is a new public Python code that computes the Fisher matrix for galaxy survey observables, allowing for tomographic and model-independent analysis, and forecasting the sensitivity of future galaxy surveys like DESI, Euclid, J-PAS and LSST.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
Florian Beutler, Patrick McDonald
Summary: Recent developments in galaxy redshift surveys have led to the proposal of a matrix-based analysis framework for galaxy power spectrum multipoles, providing deconvolved power spectrum results for several datasets. The use of deconvolved power spectrum multipoles allows for a data analysis independent of survey-specific aspects, such as the window function. This alternative analysis method has been shown to yield similar results to standard analysis in the case of the BOSS dataset, with various analysis components and a Python toolbox provided for convenience.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
Andrea Oddo, Federic Rizzo, Emiliano Sefusatti, Cristiano Porciani, Pierluigi Monaco
Summary: In this study, a joint likelihood analysis of the halo power spectrum and bispectrum in real space was conducted using a large set of numerical simulations and halo mock catalogs. Constraints on bias and cosmological parameters were derived, and a reference bias model dependent on seven parameters was selected based on the Deviance Information Criterion. This model accurately recovers three selected cosmological parameters even for extreme simulation volumes, demonstrating the importance of considering relations among bias parameters and full covariance estimation from mock catalogs.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
Pierre Zhang, Yifu Cai
Summary: The study re-analyzed the full shape of the BOSS galaxy two-point function within Lambda-CDM, with results constraining various cosmological parameters. The effect of redshift selection on the results was discussed, emphasizing the importance of systematic assessments for ongoing and future large-volume surveys.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2022)
Article
Astronomy & Astrophysics
ChangHoon Hahn, Francisco Villaescusa-Navarro
Summary: This study examines the constraining power of the redshift-space galaxy bispectrum monopole, B-0(g), on cosmological parameters and the information content down to nonlinear scales. The results show that B-0(g) significantly improves the constraints on cosmological parameters, especially for M-nu.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
Y. Rasera, M-A Breton, P-S Corasaniti, J. Allingham, F. Roy, V Reverdy, T. Pellegrin, S. Saga, A. Taruya, S. Agarwal, S. Anselmi
Summary: This study introduces a suite of large-volume high-resolution N-body simulations designed to generate light-cone data for investigating relativistic effects on lensing-matter observables without simplifying approximations. Using this dataset, the linear and quasi-linear predictions from the CLASS relativistic code for matter-density fluctuation field and gravitational convergence can be reproduced.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Shohei Saga, Atsushi Taruya, Yann Rasera, Michel-Andres Breton
Summary: In this paper, the dipole asymmetry in the cross-correlation function of galaxies induced by the observational relativistic effects is analyzed. A new prescription is proposed, which involves only 1D integrals and provides a faster way to reproduce the results. The detectability of the dipole signal induced by the gravitational redshift effect is discussed, and it is found that current and future surveys can provide a large signal-to-noise ratio.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Shohei Saga, Atsushi Taruya, Stephane Colombi
Summary: This study explores the structure around the shell-crossing time of cold dark matter protohaloes seeded by two or three crossed sine waves of various relative initial amplitudes by comparing Lagrangian perturbation theory up to the tenth order with high-resolution cosmological simulations. The results show that high-order LPT predictions match the exact solution well in the generic case, but convergence slows down in axial-symmetric configurations, especially when velocity-related quantities are considered.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Guilherme Brando, Bartolomeo Fiorini, Kazuya Koyama, Hans A. Winther
Summary: In this study, we compare and validate COLA simulations against existing emulators in the literature, and find that COLA method shows excellent agreement with the emulators under certain conditions. Furthermore, the implementation of massive neutrinos in COLA simulations and the ability to handle effective field theory of dark energy and modified gravity models are validated through experiments.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2022)
Article
Astronomy & Astrophysics
Joseph H. P. Jackson, Hooshyar Assadullahi, Kazuya Koyama, Vincent Vernin, David Wands
Summary: This article demonstrates the usage of importance sampling for reconstructing the statistics of rare cosmological fluctuations in stochastic inflation. The authors developed a publicly available package, PYFPT, that addresses the first-passage time problem of generic one-dimensional Langevin processes and its relation to curvature perturbation. The proposed method is applied to quadratic inflation and benchmarked against semi-analytical results, showing excellent agreement within the estimated statistical error. The computation time is relatively fast and can achieve low probability values compared to the observable universe. The study also investigates the impact of large-field boundaries on the tail of the probability distribution and demonstrates that non-perturbative deviations from Gaussianity are not always of the simple exponential type.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2022)
Article
Astronomy & Astrophysics
Shohei Saga, Teppei Okumura, Atsushi Taruya, Takuya Inoue
Summary: We study relativistic effects on the cross-correlation function between galaxy positions and intrinsic galaxy shapes (GI correlation) in an inhomogeneous universe. We find that the Doppler and gravitational redshift effects induce non-vanishing odd multipole anisotropies in the GI correlation function. The dipole anisotropy is dominated by the Doppler effect at large scales and the gravitational redshift effect at smaller scales, with a positive amplitude over all scales. We also derive the covariance matrix for the modelled GI dipole and show that the GI dipole induced by relativistic effects can be detected in future large-volume galaxy surveys when considering the full covariance.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Yohsuke Enomoto, Takahiro Nishimichi, Atsushi Taruya
Summary: Virialized halos of cold dark matter exhibit universal features of multistream structures within the splashback radius. The radial density profile of each stream, classified by the number of apocenter passages, can be described by a double power-law function with shallow inner slopes and steep outer slopes. These features persist over a wide range of halo masses, regardless of concentration or accretion rate. Replicating the profile's characteristic scale and amplitude requires considering complexities such as angular momentum distribution or mergers.
ASTROPHYSICAL JOURNAL LETTERS
(2023)
Article
Astronomy & Astrophysics
Teppei Okumura, Atsushi Taruya
Summary: We provide the first constraints on the growth rate of the universe, f(z)sigma 8(z), with intrinsic alignments (IAs) of galaxies. By combining measured IA statistics with conventional galaxy clustering statistics, we obtain tighter constraints on the growth rate, with a particularly significant improvement for the LRG sample. Our results show a 19% improvement in the constraints on f(sigma 8) by including IA, indicating the enhanced contribution of IA statistics for cosmological constraints.
ASTROPHYSICAL JOURNAL LETTERS
(2023)
Article
Physics, Multidisciplinary
A. D. Gow, H. Assadullahi, J. H. P. Jackson, K. Koyama, V. Vennin, D. Wands
Summary: We propose a non-perturbative method to calculate the abundance of primordial black holes based on an arbitrary one-point probability distribution function for the primordial curvature perturbation, P(zeta). This method is essential for considering non-Gaussianities that cannot be treated using conventional perturbative expansions. By relating zeta to a Gaussian field through equating cumulative distribution functions, we can determine the full statistics of the density field. We demonstrate that the intermediate regime, rather than the far tail, is responsible for the enhanced formation of primordial black holes, and show that non-Gaussianity significantly affects the shape of the primordial black hole mass distribution.
Article
Astronomy & Astrophysics
Guilherme Brando, Kazuya Koyama, Hans A. Winther
Summary: We revisit and extend a method proposed by R. Scoccimarro to incorporate the Vainshtein screening mechanism in N-body simulations, allowing for the study of Horndeski theories that evade the speed limit on gravitational waves. The method computes a scale-dependent gravitational coupling that accounts for the screening of the fifth-force, significantly reducing computational time and complexity compared to solving the full equation of motion. By implementing this method in a COmoving Lagrangian Approximation (COLA) code and comparing it with full N-body simulations, we validate its accuracy and find high agreement for the prediction of the boost function, a crucial quantity for beyond-ACDM models.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2023)
Article
Astronomy & Astrophysics
Marco Raveri, Levon Pogosian, Matteo Martinelli, Kazuya Koyama, Alessandra Silvestri, Gong -Bo Zhao
Summary: In this paper, a non-parametric reconstruction method is presented to determine three time-dependent functions in the cosmological model. The data constraints on the structure of these functions and their eigenmodes are analyzed. The results show that the combination of all data can constrain 15 combined eigenmodes of the three functions and explain the tensions between datasets.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2023)
Review
Physics, Particles & Fields
Pierre Auclair, David Bacon, Tessa Baker, Tiago Barreiro, Nicola Bartolo, Enis Belgacem, Nicola Bellomo, Ido Ben-Dayan, Daniele Bertacca, Marc Besancon, Jose J. Blanco-Pillado, Diego Blas, Guillaume Boileau, Gianluca Calcagni, Robert Caldwell, Chiara Caprini, Carmelita Carbone, Chia-Feng Chang, Hsin-Yu Chen, Nelson Christensen, Sebastien Clesse, Denis Comelli, Giuseppe Congedo, Carlo Contaldi, Marco Crisostomi, Djuna Croon, Yanou Cui, Giulia Cusin, Daniel Cutting, Charles Dalang, Valerio De Luca, Walter Del Pozzo, Vincent Desjacques, Emanuela Dimastrogiovanni, Glauber C. Dorsch, Jose Maria Ezquiaga, Matteo Fasiello, Daniel G. Figueroa, Raphael Flauger, Gabriele Franciolini, Noemi Frusciante, Jacopo Fumagalli, Juan Garcia-Bellido, Oliver Gould, Daniel Holz, Laura Iacconi, Rajeev Kumar Jain, Alexander C. Jenkins, Ryusuke Jinno, Cristian Joana, Nikolaos Karnesis, Thomas Konstandin, Kazuya Koyama, Jonathan Kozaczuk, Sachiko Kuroyanagi, Danny Laghi, Marek Lewicki, Lucas Lombriser, Eric Madge, Michele Maggiore, Ameek Malhotra, Michele Mancarella, Vuk Mandic, Alberto Mangiagli, Sabino Matarrese, Anupam Mazumdar, Suvodip Mukherjee, Ilia Musco, Germano Nardini, Jose Miguel No, Theodoros Papanikolaou, Marco Peloso, Mauro Pieroni, Luigi Pilo, Alvise Raccanelli, Sebastien Renaux-Petel, Arianna I. Renzini, Angelo Ricciardone, Antonio Riotto, Joseph D. Romano, Rocco Rollo, Alberto Roper Pol, Ester Ruiz Morales, Mairi Sakellariadou, Ippocratis D. Saltas, Marco Scalisi, Kai Schmitz, Pedro Schwaller, Olga Sergijenko, Geraldine Servant, Peera Simakachorn, Lorenzo Sorbo, Lara Sousa, Lorenzo Speri, Daniele A. Steer, Nicola Tamanini, Gianmassimo Tasinato, Jesus Torrado, Caner Unal, Vincent Vennin, Daniele Vernieri, Filippo Vernizzi, Marta Volonteri, Jeremy M. Wachter, David Wands, Lukas T. Witkowski, Miguel Zumalacarregui, James Annis, Feanor Reuben Ares, Pedro P. Avelino, Anastasios Avgoustidis, Enrico Barausse, Alexander Bonilla, Camille Bonvin, Pasquale Bosso, Matteo Calabrese, Mesut Caliskan, Jose A. R. Cembranos, Mikael Chala, David Chernoff, Katy Clough, Alexander Criswell, Saurya Das, Antonio da Silva, Pratika Dayal, Valerie Domcke, Ruth Durrer, Richard Easther, Stephanie Escoffier, Sandrine Ferrans, Chris Fryer, Jonathan Gair, Chris Gordon, Martin Hendry, Mark Hindmarsh, Deanna C. Hooper, Eric Kajfasz, Joachim Kopp, Savvas M. Koushiappas, Utkarsh Kumar, Martin Kunz, Macarena Lagos, Marc Lilley, Joanes Lizarraga, Francisco S. N. Lobo, Azadeh Maleknejad, C. J. A. P. Martins, P. Daniel Meerburg, Renate Meyer, Jose Pedro Mimoso, Savvas Nesseris, Nelson Nunes, Vasilis Oikonomou, Giorgio Orlando, Ogan Ozsoy, Fabio Pacucci, Antonella Palmese, Antoine Petiteau, Lucas Pinol, Simon Portegies Zwart, Geraint Pratten, Tomislav Prokopec, John Quenby, Saeed Rastgoo, Diederik Roest, Kari Rummukainen, Carlo Schimd, Aurelia Secroun, Alberto Sesana, Carlos F. Sopuerta, Ismael Tereno, Andrew Tolley, Jon Urrestilla, Elias C. Vagenas, Jorinde van de Vis, Rien van de Weygaert, Barry Wardell, David J. Weir, Graham White, Bogumila Swiezewska, Valery I. Zhdanov
Summary: This publication provides an overview of the latest advancements in LISA cosmology, including theory and methods, and identifies new opportunities to probe the universe using gravitational-wave observations by LISA.
LIVING REVIEWS IN RELATIVITY
(2023)
Article
Astronomy & Astrophysics
Shohei Saga, Atsushi Taruya, Yann Rasera, Michel-Andres Breton
Summary: Local position invariance (LPI) is a crucial component of the Einstein equivalence principle, verifying the independence of local experiments from space-time. We propose a novel cosmological test of LPI by analyzing the asymmetry in the cross-correlation function of different types of galaxies, which is primarily caused by the gravitational redshift effect induced by galactic haloes. Our study demonstrates that ongoing/upcoming galaxy surveys can provide valuable constraints on the LPI-violating parameter α in the distant universe, within cosmological scales that have not been explored previously, with an anticipated upper limit of α reaching 0.03.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Zhenyuan Wang, Donghui Jeong, Atsushi Taruya, Takahiro Nishimichi, Ken Osato
Summary: We propose a novel nEPT scheme that models the nonlinear density field by summing up to nth-order density fields in perturbation theory. The analytical power spectrum obtained shows excellent agreement with results from 20 Dark-Quest N-body simulations across a wide range of cosmologies. This method can accelerate the forward modeling of the nonlinear cosmological density field, which is an essential probe of cosmic mysteries such as inflation, dark energy, and dark matter.
Article
Astronomy & Astrophysics
Yoshiaki Himemoto, Atsushi Nishizawa, Atsushi Taruya
Summary: Search sensitivity to a stochastic gravitational-wave background (SGWB) is enhanced by cross-correlating detector signals. However, the presence of correlated environmental noise between detectors, caused by global electromagnetic fields known as Schumann resonances and instrumental magnetic couplings, is a major concern. In this paper, the authors study the detectability of SGWB in the presence of correlated magnetic noise, finding no significant degeneracy between the SGWB and noise parameters. Marginalizing over the correlated noise parameters degrades the constraint on each SGWB parameter and ignoring the correlated noise generally leads to a biased constraint.