Article
Astronomy & Astrophysics
Thiago Mergulhao, Henrique Rubira, Rodrigo Voivodic, L. Raul Abramo
Summary: In this study, we investigate the impact of the perturbative bias expansion combined with the multi-tracer technique on the extraction of cosmological parameters. Our results show that using the multi-tracer approach provides more accurate and less biased constraints on omega(cdm) and h compared to using a single tracer. The multi-tracer approach also improves the constraints on the bias expansion parameters and reduces their errors.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2022)
Article
Astronomy & Astrophysics
Daniel Geiss, Ivan Kostyuk, Robert Lilow, Matthias Bartelmann
Summary: This paper presents a new analytical description of cosmic structure formation in a mixture of dark and baryonic matter using the framework of Kinetic Field Theory. The authors demonstrate how to extend the KFT formalism to describe mixtures of two particle species and show the validity of this approach by computing the linear evolution of matter power spectra. The results accurately reproduce expected behavior, showing suppression of structure growth on small scales in good agreement with numerical results.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
C. Pixius, S. Celik, M. Bartelmann
Summary: This paper presents recent improvements in the perturbative treatment of particle interactions in Kinetic Field Theory (KFT) for inertial Zel'dovich trajectories. The study derives a more rigorous treatment of phase-space trajectories of particles in an expanding universe, and applies these results to calculate corrections to the late-time dark matter power spectrum at second order. The findings show that the modified treatment of interactions improves the agreement between KFT and simulation results, and including particle interactions up to second order systematically improves the non-linear power spectrum.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2022)
Article
Astronomy & Astrophysics
Anton Chudaykin, Konstantin Dolgikh, Mikhail M. Ivanov
Summary: This study presents limits on the parameters of ΛCDM, w(0)CDM, and w(0)w(a)CDM models obtained from a joint analysis of various data sources, independent of cosmic microwave background data. The results show consistency of dark-energy equation of state parameter with a cosmological constant, as well as spatial curvature consistent with a flat universe. The study also demonstrates the strong constraints provided by full-shape and baryon acoustic oscillations data on nonminimal cosmological models.
Article
Astronomy & Astrophysics
Xiaohan Wu, Julian B. Munoz, Daniel Eisenstein
Summary: We propose a non-parametric halo biasing model that can accurately represent the ratio of halo and mass densities. Our model shows a monotonically increasing halo-to-mass ratio with linear overdensity in the initial Lagrangian space, while the traditional perturbative halo bias model does not guarantee non-negativity of the halo counts. We demonstrate that our non-parametric model can recover the halo power spectra to sub-percent level accuracy for certain halo masses when given a proper smoothing scale to filter the initial density field. However, the recovery of the halo power spectrum is mildly dependent on the smoothing scale and other input parameters. Our findings qualitatively agree with intuitions from extended Press-Schechter theory.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2022)
Article
Astronomy & Astrophysics
Henrique Rubira, Rodrigo Voivodic
Summary: A logarithm transformation of the matter overdensity field allows information from higher-order functions to be transferred to the power spectrum, improving computational efficiency and accuracy. Studies show that the large-scale behavior of the log-transformed field can be represented by a small number of free parameters, and the non-linear transformation enables access to information on smaller scales.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
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
Adria Gomez-Valent, Ziyang Zheng, Luca Amendola, Valeria Pettorino, Christof Wetterich
Summary: The study reveals that the fraction of early dark energy (EDE) is constrained to be around 0.4%, and its impact on cosmological tensions is significant, although constraints considerably weaken when the sound speed is allowed to vary. The presence of EDE in different epochs helps both alleviate and worsen cosmological tensions.
Article
Astronomy & Astrophysics
Jorge Venzor, Gabriela Garcia-Arroyo, Abdel Perez-Lorenzana, Josue De-Santiago
Summary: Nonstandard self-interactions can affect the evolution of cosmological neutrinos and leave detectable traces in cosmological observables. With cosmological data including Planck 2018, BAO measurements, local H0, Ly-??, and SNIa, we constrain the self-interactions of massive neutrinos with a light scalar mediator. The effective coupling constant is found to be geff < 1.94 x 10^-7 using Planck 2018 data and 1.97 x 10^-7 when combining Planck and BAO. This study has significant implications for understanding neutrino interactions in cosmology.
Article
Physics, Particles & Fields
Jie Zheng, Shuo Cao, Yujie Lian, Tonghua Liu, Yuting Liu, Zong-Hong Zhu
Summary: In this paper, the authors investigate a series of Chaplygin gas models as candidates for unified dark matter and dark energy using the latest observations of quasars. Different statistical methods are applied to constrain and distinguish these models. The results show that the standard ruler data provide more stringent constraints on the cosmological parameters and are consistent with previous results. The consistency between Chaplygin gas and the concordance ACDM model is demonstrated, but deviations are found for certain models in the framework of statefinder diagnostics. The MCG and VGCG models have substantial observational support from high-redshift quasars, while the GCG and NGCG models lack support but cannot be ruled out.
EUROPEAN PHYSICAL JOURNAL C
(2022)
Article
Astronomy & Astrophysics
Maresuke Shiraishi, Teppei Okumura, Kazuyuki Akitsu
Summary: In this study, the galaxy intrinsic alignment is used to test the cosmic isotropy along with galaxy number density and peculiar velocity. The impacts of isotropy breaking on the configuration-space two-point correlation functions (2PCFs) are analyzed, and it is found that anisotropic distortions appear and have shapes determined by a preferred direction causing the isotropy violation. The study also suggests that the plane parallel (PP) approximation may not be valid in certain cases, and an accurate test for cosmic isotropy requires a formulation of 2PCF that does not rely on this approximation.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2023)
Article
Astronomy & Astrophysics
Uendert Andrade, Rodrigo S. Goncalves, Gabriela C. Carvalho, Carlos A. P. Bengaly, Joel C. Carvalho, Jailson Alcaniz
Summary: We report measurements of the angular scale of cosmic homogeneity using the luminous red galaxy sample from SDSS-IV LRG DR16, finding that they are consistent with the predictions of the standard cosmology.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2022)
Article
Astronomy & Astrophysics
Rodrigo S. Goncalves, Gabriela C. Carvalho, Uendert Andrade, Carlos A. P. Bengaly, Joel C. Carvalho, Jailson Alcaniz
Summary: Using the quasar sample from the sixteenth data release of the Sloan Digital Sky Survey, we found a decreasing trend in the cosmic homogeneity scale with redshift, which is in good agreement with the ΛCDM prediction. Our results confirm the presence of a homogeneity scale in the spatial distribution of quasars as predicted by the standard cosmological model.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
Azadeh Moradinezhad Dizgah, Farnik Nikakhtar, Garrett K. Keating, Emanuele Castorina
Summary: Line intensity mapping is an emerging technique that has the potential to accurately probe signals at different scales and redshifts. By using simulations and modeling, researchers have been able to accurately predict clustering power and stochastic contributions of intensity fluctuations. Furthermore, this technique shows promise in measuring the baryon acoustic oscillations, which has important implications for cosmological studies in the future.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2022)
Article
Astronomy & Astrophysics
Debabrata Chandra, Supratik Pal
Summary: In this article, we investigate the competency of upcoming Cosmic Microwave Background (CMB) and Galaxy surveys in probing the features in the primordial power spectrum. We focus on three major features, including the Bump feature, Sharp feature signal, and Resonance feature signal, and analyze their constraints using different observational data. The research findings suggest that these upcoming observations have relative capabilities in shedding light on crucial aspects of precision cosmology.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2022)
Article
Astronomy & Astrophysics
M. M. Ivanov, Y. Y. Kovalev, M. L. Lister, A. G. Panin, A. B. Pushkarev, T. Savolainen, S. Troitsky
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2019)
Article
Astronomy & Astrophysics
Mikhail M. Ivanov, Alexander A. Kaurov, Sergey Sibiryakov
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2019)
Article
Astronomy & Astrophysics
Shun Arai, Sergey Sibiryakov, Yuko Urakaw
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2019)
Article
Astronomy & Astrophysics
Diego Blas, Andrea Caputo, Mikhail M. Ivanov, Laura Sberna
PHYSICS OF THE DARK UNIVERSE
(2020)
Article
Astronomy & Astrophysics
Andrey Katz, Joachim Kopp, Sergey Sibiryakov, Wei Xue
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2020)
Article
Physics, Particles & Fields
Maxim Fitkevich, Dmitry Levkov, Sergey Sibiryakov
JOURNAL OF HIGH ENERGY PHYSICS
(2020)
Article
Physics, Particles & Fields
Sergey Sibiryakov, Philip Sorensen, Tien-Tien Yu
JOURNAL OF HIGH ENERGY PHYSICS
(2020)
Article
Physics, Particles & Fields
Arthur Marakulin, Sergey Sibiryakov
Summary: This study investigates the supersymmetric extension of the Einstein-aether gravitational model, incorporating aether to break local Lorentz invariance and describing the dynamics of linear perturbations. The resulting model features an on-shell gravity multiplet with superluminal and light speed excitations, with observational constraints outlined based on low-energy phenomenology.
JOURNAL OF HIGH ENERGY PHYSICS
(2021)
Article
Astronomy & Astrophysics
Mikhail M. Ivanov, Marko Simonovic, Matias Zaldarriaga
Article
Astronomy & Astrophysics
Diego Blas, Diana Lopez Nacir, Sergey Sibiryakov
Article
Astronomy & Astrophysics
Andrei O. Barvinsky, Mario Herrero-Valea, Sergey M. Sibiryakov