| The Simons Observatory: science goals and forecasts |
92 |
| Tale of stable interacting dark energy, observational signatures, and the H-0 tension |
53 |
| Femtolensing by dark matter revisited |
49 |
| Does the Hubble constant tension call for new physics? |
48 |
| Revisiting constraints on asteroid-mass primordial black holes as dark matter candidates |
42 |
| H-0 from cosmic chronometers and Type la supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method |
39 |
| The BAO plus BBN take on the Hubble tension |
36 |
| Shadow cast and deflection angle of Kerr-Newman-Kasuya spacetime |
35 |
| Gravitational wave energy budget in strongly supercooled phase transitions |
33 |
| Formation and evolution of primordial black hole binaries in the early universe |
32 |
| Structure formation in f(T) gravity and a solution for H-0 tension |
31 |
| Baryon Acoustic Oscillations and the Hubble constant: past, present and future |
30 |
| Reconstructing the spectral shape of a stochastic gravitational wave background with LISA |
30 |
| Hot axions and the H-0 tension |
30 |
| The string swampland constraints require multi-field inflation |
28 |
| Constraining the mass of dark photons and axion-like particles through black-hole superradiance |
28 |
| Gravitational wave decay into dark energy |
28 |
| MeV-scale reheating temperature and thermalization of oscillating neutrinos by radiative and hadronic decays of massive particles |
28 |
| Steepest growth of the power spectrum and primordial black holes |
27 |
| Updated bounds on sum of neutrino masses in various cosmological scenarios |
26 |
| Can the H-0 tension be resolved in extensions to Lambda CDM cosmology? |
26 |
| On the maximal strength of a first-order electroweak phase transition and its gravitational wave signal |
26 |
| Holographic dark energy through Tsallis entropy |
25 |
| Vector dark matter production at the end of inflation |
25 |
| An improved model-independent assessment of the late-time cosmic expansion |
24 |
| Nonlocal gravity. Conceptual aspects and cosmological predictions |
24 |
| Thermalisation of sterile neutrinos in the early universe in the 3+1 scheme with full mixing matrix |
23 |
| Physics potential of the International Axion Observatory (IAXO) |
23 |
| Palatini inflation in models with an R-2 term |
22 |
| Improved axion emissivity from a supernova via nucleon-nucleon bremsstrahlung |
22 |
| Gravitational waves from first-order phase transition in a simple axion-like particle model |
22 |
| Curvature radius and Kerr black hole shadow |
21 |
| Dark, cold, and noisy: constraining secluded hidden sectors with gravitational waves |
21 |
| Interacting dark sector and precision cosmology |
21 |
| Testing modified gravity at cosmological distances with LISA standard sirens |
21 |
| Distance priors from Planck final release |
21 |
| Primordial black holes from alpha-attractors |
21 |
| Logarithmic-corrected R-2 gravity inflation in the presence of Kalb-Ramond fields |
21 |
| Cosmological dynamics of mimetic gravity |
20 |
| Quantifying baryon effects on the matter power spectrum and the weak lensing shear correlation |
20 |
| Listening to the sound of dark sector interactions with gravitational wave standard sirens |
20 |
| The ineludible non-Gaussianity of the primordial black hole abundance |
20 |
| Strange stars in f (R, T) gravity |
20 |
| A cosmological signature of the SM Higgs instability: gravitational waves |
20 |
| Scalaron from R-2-gravity as a heavy field |
20 |
| Inflation with R-2 term in the Palatini formulation |
19 |
| From primordial black holes abundance to primordial curvature power spectrum (and back) |
19 |
| Looking for ultralight dark matter near supermassive black holes |
19 |
| The promising future of a robust cosmological neutrino mass measurement |
18 |
| MassiveNuS: cosmological massive neutrino simulations |
18 |
