NewEvery arXiv paper, its researchers & institutions — mapped.
the archive

astro-ph.CO

45.6k results
astro-ph.CO2026

Spin-1 Ultralight Dark Matter under Cosmological Scrutiny: Mass Constraints from CMB and Distance Probes

Guadalupe Ahumada Acuña, Tomas Ferreira Chase, Diana López Nacir +1

astro-ph.CO2026

Domain walls through different cosmologies

I. Dankovsky, D. Gorbunov, S. Ramazanov +1

The paper uses lattice simulations to study how domain wall networks evolve under various early‑universe expansion histories, showing that the particle horizon largely determines w…

#domain walls#early universe#cosmological expansion#gravitational waves
astro-ph.CO2026

Inflation, Open Universes, and Dark Energy

Anton Chudaykin, Mikhail M. Ivanov, Renata Kallosh +3

The authors analyze how allowing a small negative spatial curvature and/or a time‑varying dark energy equation of state changes the inferred scalar spectral index nₛ from CMB and g…

#inflation#spatial curvature#dark energy#cosmic microwave background
astro-ph.CO2026

A Simulation Based Inference Approach to Modelling of Type Ia Supernova Populations

B. Popovic, M. Grayling, M. O'Callaghan +11

astro-ph.CO2026

Understanding constraints on primordial mass black holes made of dark matter using fast radio bursts

Surajit Kalita, Shruti Bhatporia, Amanda Weltman

astro-ph.CO2026

Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation

Drew Jamieson, Angelo Caravano, Eiichiro Komatsu

astro-ph.CO2026

Single Frequency CMB Foreground Removal with Inter-scale Machine Learning

Helen Shao, Fiona McCarthy, Blake D. Sherwin +2

astro-ph.CO2026

Local bandpower diagnostics for the hemispherical power asymmetry in CMB E-mode polarization

Robert A Lynch

astro-ph.CO2026

Multi-branch classification of diffuse cluster radio emission

Markus Bredberg, Emma Tolley

The paper investigates machine‑learning methods, specifically scattering‑transform encoders and squeeze‑excitation attention in multi‑branch neural networks, to improve detection o…

#diffuse radio emission#galaxy clusters#machine learning classification#scattering transform
astro-ph.CO2026

Axion Inflation with a Massive Abelian Gauge Field

Ricardo Z. Ferreira, Alessio Notari, José Jaime Terente Díaz

The paper studies how an axial coupling between an inflaton (axion) and a massive Abelian gauge field can cause tachyonic amplification of one helicity, analyzes the resulting back…

#axion inflation#massive gauge field#tachyonic instability#backreaction
astro-ph.CO2026

Dark Matter Constraints from Small-Scale Cosmic Structure

Ethan O. Nadler, Keir K. Rogers, Alex Drlica-Wagner

The paper reviews how observations of small‑scale cosmic structures, such as dwarf galaxies and the Lyman‑α forest, constrain the microphysical properties of dark matter models.

#dark matter#small-scale structure#halo abundance#cosmic simulations
astro-ph.CO2026

A study of the large-scale formation in the environment of A3266: Infalling groups, filaments, and a premerger cold front

J. Dietl, A. Veronica, T. H. Reiprich +7

The paper uses eROSITA X‑ray data to map the outskirts of the galaxy cluster Abell 3266, revealing a hot X‑ray filament linking the cluster to a nearby group and showing how the cl…

#galaxy clusters#large-scale structure#x-ray astronomy#filaments
astro-ph.CO2026

Growth, geometry, and early-universe split of the matter density parameter $Ω_{\rm m}$

Felicitas Keil, Isaac Tutusaus, Alain Blanchard

The paper separates the present‑day matter density parameter Ωₘ into geometric, growth, and early‑universe contributions using DES, Planck, DESI BAO, Pantheon+ supernovae, and RSD…

#matter density parameter#parameter splitting#geometry#growth of structure
astro-ph.CO2026

GGI Lectures on Large-Scale Structure Perturbation Theory (Effective Field Theory)

Mikhail M. Ivanov

These lecture notes introduce non-linear perturbation theory and effective field theory methods for modeling the large-scale distribution of galaxies, targeting undergraduate and e…

#large-scale structure#perturbation theory#effective field theory#galaxy bias
astro-ph.CO2026

Beyond monomial $α$-attractors

Laura Iacconi

The paper investigates inflationary α‑attractor models with a binomial (quadratic + quartic) potential, showing that the quartic term can significantly modify the scalar spectral i…

#inflation#alpha-attractors#reheating#scalar spectral index
astro-ph.CO2026

Cosmo-SPINN: Fuzzy Dark Matter Simulations with Physics-Informed Generative Networks

Ashutosh Kumar Mishra, Emma Tolley, Nicolas Cerardi

The paper introduces a physics‑informed generative U‑Net that can evolve fuzzy dark matter fields and perform super‑resolution of simulations while enforcing the Schrödinger‑Poisso…

#fuzzy dark matter#physics-informed neural networks#generative modeling#cosmological simulation
astro-ph.CO2026

No way ou$τ$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization

Paulo Montero-Camacho, Yi Mao

The authors combine CMB data (excluding large‑scale polarization), BAO measurements, and quasar‑based reionization observations to estimate the optical depth to reionization as τ≈0…

#reionization#optical depth#cmb polarization#dark energy
astro-ph.CO2026

Impact of numerical stability in Bayesian noise wave calibration on global 21-cm experiments

Saswata Dasgupta, Adarsh Kumar Dash, Dominic Anstey +3

The paper identifies and mitigates a numerical instability in the Bayesian noise‑wave calibration used for global 21‑cm experiments, improving reproducibility and accuracy of recei…

#global 21-cm signal#noise wave calibration#numerical stability#bayesian inference
astro-ph.CO2026

J-PAS & FLAMINGO: Cosmic voids and void galaxies in the gravitational landscape of photometric surveys

J. A. Mansour, B. McCarthy, L. J. Liivamägi +34

The paper presents a method that uses a quasi‑gravitational potential field to identify dynamically dominant cosmic voids and their galaxies in photometric surveys like J‑PAS, show…

#cosmic voids#photometric redshift errors#large-scale structure#galaxy surveys
astro-ph.CO2026

Shear-kSZ: A New Estimator for the Matter-Electron Power Spectrum from kSZ Tomography and Weak Lensing

Boryana Hadzhiyska

The paper introduces a new estimator that combines kinematic Sunyaev‑Zel'dovich measurements, reconstructed velocity fields, and weak‑lensing maps to directly probe the matter–elec…

#kinematic sunyaev-zeldovich#weak lensing#matter-electron power spectrum#baryonic effects
astro-ph.CO2026

Global 21cm Measurement Calibration Methodology

Martin Bucher, Christian J. Kirkham, Eloy de Lera Acedo +2

The paper derives explicit calibration equations for global 21 cm signal experiments, reconciling earlier approaches with amplifier noise formalism and providing a Möbius‑geometry…

#global 21cm signal#instrument calibration#radio astronomy#antenna impedance
astro-ph.CO2026

Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys

Walter Riquelme, Santiago Avila, Lucas Pinol +2

The paper studies how massive fields present during inflation could leave detectable signatures in galaxy clustering, using DESI imaging data and forecasting the capability of futu…

#inflation#primordial non-gaussianity#galaxy clustering#DESI imaging
astro-ph.CO2026

Phantom-divide crossing and suppressed structure growth in kinetically braided dark energy with momentum exchange

Masroor C. Pookkillath, Shinji Tsujikawa

The paper presents a stable scalar‑field model that allows the dark‑energy equation of state to cross from phantom (w < ‑1) to non‑phantom values while reducing the growth of cold…

#dark energy#phantom crossing#momentum exchange#structure growth
astro-ph.CO2026

An efficient one-loop EFTofLSS framework for Vainshtein-screened Horndeski gravity

Stan Verhoeve, Dani de Boe, Gen Ye +1

The authors extend the PyBird code to compute one-loop matter power spectra for Vainshtein‑screened Horndeski and nDGP gravity using a direct ODE approach for time‑dependent kernel…

#large-scale structure#modified gravity#Horndeski theory#Vainshtein screening