Article
Astronomy & Astrophysics
Luis Atayde, Noemi Frusciante
Summary: Observational constraints were studied on nonmetricity f(Q)-gravity, reproducing an exact Lambda CDM background expansion history while modifying the evolution of linear perturbations. By utilizing various measurements, it was found that the model is preferred over Lambda CDM in certain statistical aspects, primarily due to a better fit to the low-l tail of CMB temperature anisotropies.
Article
Astronomy & Astrophysics
Pawel Drozda, Wojciech A. Hellwing, Maciej Bilicki
Summary: Using N-body simulations, the study examines the angular clustering of galaxies, halos, and dark matter in different gravity scenarios. Results show that the optimal redshift range for maximizing the modified gravity (MG) signal is between 0.15 < z < 0.3. Significant deviations from general relativity (GR) are observed in MG measurements, with different significance levels depending on the statistics used and the scale analyzed. The study suggests that third-order statistics provide sensitive probes for different structure formation scenarios. The findings also highlight the potential of future applications to test GR and MG with higher precision and significance.
Article
Astronomy & Astrophysics
Michael Boylan-Kolchin
Summary: Early data from the James Webb Space Telescope (JWST) show that high-redshift galaxy candidates have unexpectedly high stellar masses, posing a concern regarding their consistency with the standard CDM cosmological model. The mass function of dark matter haloes limits the number and stellar mass density of galaxies more massive than a certain stellar mass at any epoch, and the most massive galaxy candidates at z approximately 7-10 observed by JWST push the limits, indicating unresolved issues with galaxy properties derived from observations and the formation of galaxies in the CDM model or within the standard cosmology itself.
Article
Astronomy & Astrophysics
Oliver Mueller, Marcel S. Pawlowski, Federico Lelli, Katja Fahrion, Marina Rejkuba, Michael Hilker, Jamie Kanehisa, Noam Libeskind, Helmut Jerjen
Summary: The study reveals the presence of co-rotating planes of satellites in the satellite system of Centaurus A, posing a challenge to the ΛCDM model. While similar structures have been found in cosmological simulations, they are found to be short-lived and arise from chance projection rather than co-orbiting.
ASTRONOMY & ASTROPHYSICS
(2021)
Article
Astronomy & Astrophysics
Fotios K. Anagnostopoulos, Spyros Basilakos, Emmanuel N. Saridakis
Summary: The novel model proposed in the f(Q) gravity framework shows improved performance compared to standard ΛCDM model in background and perturbation levels, according to AIC, BIC, and DIC criteria. It presents a unique cosmological scenario distinct from ΛCDM, while statistically similar, and exhibits no early dark energy features, passing BBN constraints.
Article
Astronomy & Astrophysics
Han Aung, Daisuke Nagai, Erwin T. Lau
Summary: Recent studies have found discrepancies between the location of the accretion shock and the splashback radius of dark matter, with the former being larger by 20-100%. This has implications for multiwavelength studies of galaxy clusters.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Mathematics
Vladimir V. Uchaikin, Vladimir A. Litvinov, Elena V. Kozhemyakina, Ilya I. Kozhemyakin
Summary: A new statistical model for the spatial distribution of observed galaxies is described, using Markov chain ensembles and parameters extracted from the observable power spectrum. The model effectively reproduces two-point correlation functions and cell-count data, showing potential for use in cosmological studies post-processing of astronomical data.
Article
Engineering, Geological
C. S. Chang, T. T. Ma
Summary: This study aims to predict the permeability of soils based on bimodal void sizes and evaluate the developed model by comparing it with experimental results. The findings can contribute to a better understanding of the important influence of pore structure on permeability prediction.
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
Oliver H. E. Philcox, Mikhail M. Ivanov
Summary: We present a full CDM analysis of the BOSS DR12 dataset, including various statistics such as power spectrum multipole, real-space power spectrum, reconstructed power spectrum, and bispectrum monopole. The inclusion of the bispectrum provides consistent parameter constraints and reduces the error bars. Our results are broadly consistent with the observations from the Planck satellite.
Article
Physics, Multidisciplinary
Kun Xu, ChengZe Liu, YiPeng Jing, Marcin Sawicki, Stephen Gwyn
Summary: We report a giant red central disk galaxy in the XMM-LSS north region with a high stellar mass and old stellar population. The galaxy does not have any close neighbors with similar mass, challenging the current standard paradigm of galaxy formation with no known physical mechanism to explain its halted star formation. This conclusion is supported by state-of-the-art hydrodynamical simulations of galaxy formation.
SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY
(2021)
Article
Astronomy & Astrophysics
Mahmood Roshan, Neda Ghafourian, Tahere Kashfi, Indranil Banik, Moritz Haslbauer, Virginia Cuomo, Benoit Famaey, Pavel Kroupa
Summary: The study reveals significant discrepancies between cosmological simulations and observations in the evolution of barred galaxies, particularly in the ratio of corotation radius to bar length. The statistical tension in EAGLE50 is lower due to a small number of galaxies suitable for analysis. The simulated fraction of barred galaxies and their trend with stellar mass differ greatly from observations.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Radouane Gannouji, Leandros Perivolaropoulos, David Polarski, Foteini Skara
Summary: The study focuses on Horndeski modified gravity models fulfilling stability and gravitational wave speed conditions, with a further assumption of the evolution of cosmic alpha functions in a Lambda cold dark matter background. It is found that the gravitational couplings display specific properties based on various parameters, with a preference for weak gravity today and certain limits on the parameter s. The analysis also considers the growth index gamma(z) to gain insights into the past evolution of mu, revealing important information on the dynamics of gravity in different scenarios.
Article
Astronomy & Astrophysics
Man Ho Chan, Ka Chung Law
Summary: This article analytically derives the rotational curve gradient of the Milky Way in the framework of MOND and provides a rigorous analysis of the MOND phenomenology. The findings show that the recent discovery of the declining rotation curve in the outer region of the Milky Way strongly suggests that MOND is not a fundamental theory nor a universal description of galactic properties.
ASTROPHYSICAL JOURNAL
(2023)
Article
Materials Science, Multidisciplinary
Joseph Paux, Leo Morin, Renald Brenner
Summary: This paper proposes a method of using discontinuous velocity fields based on FFT numerical results to analyze the strain localization problem of periodic distributions of voids in single crystals. The experimental results show that this new method can provide a good estimation of the macroscopic yield stress.
JOURNAL OF THE MECHANICS AND PHYSICS OF SOLIDS
(2022)
Article
Astronomy & Astrophysics
K. Tisanic, G. De Zotti, A. Amiri, A. Khoram, S. Tavasoli, Z. Vidovic-Tisanic
Summary: This study focused on the link between radio emission and star formation rates or infrared luminosity in a sample of local star-forming galaxies. The research aimed to improve the calibration of the radio luminosity-SFR relation and test for potential nonlinearities, ultimately finding no deviations from linearity. The results provide insights into the importance of the relationship between radio emission and star formation for radio astronomy.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Amirnezam Amin, Saeed Tavasoli, Gianfranco De Zotti
ASTROPHYSICAL JOURNAL
(2019)
Article
Astronomy & Astrophysics
B. Javanmardi, M. Raouf, H. G. Khosroshahi, S. Tavasoli, O. Mueller, A. Molaeinezhad
ASTROPHYSICAL JOURNAL
(2019)
Article
Astronomy & Astrophysics
Moein Mosleh, Saeed Tavasoli, Sandro Tacchella
ASTROPHYSICAL JOURNAL
(2018)
Article
Astronomy & Astrophysics
S. Tavasoli, H. Rahmani, H. G. Khosroshahi, K. Vasei, M. D. Lehnert
ASTROPHYSICAL JOURNAL LETTERS
(2015)