Works matching DE "HUBBLE constant"
Results: 807
Cosmology: Planck team replies to data 'anomalies'.
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- Nature, 2014, v. 506, n. 7486, p. 34, doi. 10.1038/506034c
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An eclipsing-binary distance to the Large Magellanic Cloud accurate to two per cent.
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- Nature, 2013, v. 495, n. 7439, p. 76, doi. 10.1038/nature11878
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Luminosity Distance Reconstruction using an Ensemble of Neural Networks.
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- Iranian Journal of Astronomy & Astrophysics, 2024, v. 11, n. 2, p. 81, doi. 10.22128/ijaa.2024.809.1180
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Low-Redshift Observational Constraints on Dark Energy Cosmologies.
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- Iranian Journal of Astronomy & Astrophysics, 2023, v. 10, n. 2, p. 27, doi. 10.22128/ijaa.2023.719.1164
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Non-Parametric Reconstruction of Cosmological Observables Using Gaussian Processes Regression.
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- Universe (2218-1997), 2024, v. 10, n. 12, p. 464, doi. 10.3390/universe10120464
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2D BAO vs. 3D BAO: Solving the Hubble Tension with Bimetric Cosmology.
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- Universe (2218-1997), 2024, v. 10, n. 11, p. 406, doi. 10.3390/universe10110406
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Combined Studies Approach to Rule Out Cosmological Models Which Are Based on Nonlinear Electrodynamics.
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- Universe (2218-1997), 2024, v. 10, n. 9, p. 353, doi. 10.3390/universe10090353
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Gravitational Particle Production and the Hubble Tension.
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- Universe (2218-1997), 2024, v. 10, n. 9, p. 338, doi. 10.3390/universe10090338
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On the Effects of Non-Metricity in an Averaged Universe.
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- Universe (2218-1997), 2024, v. 10, n. 6, p. 261, doi. 10.3390/universe10060261
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Phantom Scalar Field Cosmologies Constrained by Early Cosmic Measurements.
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- Universe (2218-1997), 2024, v. 10, n. 6, p. 232, doi. 10.3390/universe10060232
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Dynamics of Cosmological Scalar Fields Revisited †.
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- Universe (2218-1997), 2024, v. 10, n. 5, p. 197, doi. 10.3390/universe10050197
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Discord in Concordance Cosmology and Anomalously Massive Early Galaxies.
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- Universe (2218-1997), 2024, v. 10, n. 1, p. 48, doi. 10.3390/universe10010048
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The Unsettled Number: Hubble's Tension.
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- Universe (2218-1997), 2023, v. 9, n. 12, p. 501, doi. 10.3390/universe9120501
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Hořava–Lifshitz F ( R ¯ ) Theories and the Swampland.
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- Universe (2218-1997), 2023, v. 9, n. 11, p. 460, doi. 10.3390/universe9110460
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The Formulation of Scaling Expansion in an Euler-Poisson Dark-Fluid Model.
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- Universe (2218-1997), 2023, v. 9, n. 10, p. 431, doi. 10.3390/universe9100431
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Seven Hints That Early-Time New Physics Alone Is Not Sufficient to Solve the Hubble Tension.
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- Universe (2218-1997), 2023, v. 9, n. 9, p. 393, doi. 10.3390/universe9090393
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Fab-Four Cosmography to Tackle the Hubble Tension.
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- Universe (2218-1997), 2023, v. 9, n. 7, p. 311, doi. 10.3390/universe9070311
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Cosmological Constant from Boundary Condition and Its Implications beyond the Standard Model.
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- Universe (2218-1997), 2023, v. 9, n. 2, p. 103, doi. 10.3390/universe9020103
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The Cosmological Arrow of Time and the Retarded Potentials.
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- Universe (2218-1997), 2023, v. 9, n. 1, p. 30, doi. 10.3390/universe9010030
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H 0 Tension on the Light of Supermassive Black Hole Shadows Data.
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- Universe (2218-1997), 2023, v. 9, n. 1, p. 14, doi. 10.3390/universe9010014
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Bulk Viscous Flat FLRW Model with Observational Constraints in f (T , B) Gravity.
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- Universe (2218-1997), 2022, v. 8, n. 12, p. 650, doi. 10.3390/universe8120650
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DE Models with Combined H 0 · r d from BAO and CMB Dataset and Friends.
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- Universe (2218-1997), 2022, v. 8, n. 12, p. 631, doi. 10.3390/universe8120631
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A Reanalysis of the Latest SH0ES Data for H 0 : Effects of New Degrees of Freedom on the Hubble Tension.
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- Universe (2218-1997), 2022, v. 8, n. 10, p. N.PAG, doi. 10.3390/universe8100502
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Using Neutrino Oscillations to Measure H 0 ?
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- Universe (2218-1997), 2022, v. 8, n. 7, p. N.PAG, doi. 10.3390/universe8070377
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Ultra Long Period Cepheids: Observation and Theory.
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- Universe (2218-1997), 2022, v. 8, n. 6, p. N.PAG, doi. 10.3390/universe8060335
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Multi-Messenger Constraints on the Hubble Constant through Combination of Gravitational Waves, Gamma-Ray Bursts and Kilonovae from Neutron Star Mergers.
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- Universe (2218-1997), 2022, v. 8, n. 5, p. 289, doi. 10.3390/universe8050289
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A Short Review on the Latest Neutrinos Mass and Number Constraints from Cosmological Observables.
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- Universe (2218-1997), 2022, v. 8, n. 5, p. 284, doi. 10.3390/universe8050284
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Modified Equations of State for Dark Energy and Observational Limitations.
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- Universe (2218-1997), 2022, v. 8, n. 4, p. N.PAG, doi. 10.3390/universe8040201
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Asymptotic Solutions of a Generalized Starobinski Model: Kinetic Dominance, Slow Roll and Separatrices.
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- Universe (2218-1997), 2021, v. 7, n. 12, p. 1, doi. 10.3390/universe7120500
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Cosmological Model with Interconnection between Dark Energy and Matter.
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- Universe (2218-1997), 2021, v. 7, n. 11, p. 1, doi. 10.3390/universe7110412
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Statefinder and O<sub>m</sub> Diagnostics for New Generalized Chaplygin Gas Model.
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- Universe (2218-1997), 2021, v. 7, n. 10, p. 1, doi. 10.3390/universe7100362
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Higher Dimensional Bianchi V Models in f (R,T) Theory with Perfect Fluid Distribution.
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- Journal of Ultra Scientist of Physical Sciences - Section A (Mathematics), 2023, v. 35, n. 6, p. 54, doi. 10.22147/jusps-A/350601
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Bianchi Type-I Inflationary Cosmological Models With Constant Deceleration Parameter For Perfect Fluid Distribution In General Relativity.
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- Journal of Ultra Scientist of Physical Sciences - Section A (Mathematics), 2022, v. 34, n. 1, p. 20, doi. 10.22147/jusps-A/340104
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Determination of the Hubble Constant and Sound Horizon from Dark Energy Spectroscopic Instrument Year 1 and Dark Energy Survey Year 6 Baryon Acoustic Oscillation.
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- Galaxies (2075-4434), 2024, v. 12, n. 4, p. 48, doi. 10.3390/galaxies12040048
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The Simplest Parametrization of the Equation of State Parameter in the Scalar Field Universe.
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- Galaxies (2075-4434), 2023, v. 11, n. 2, p. 57, doi. 10.3390/galaxies11020057
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On Low Hubble Expansion Rate from Planck Data Anomalies.
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- Galaxies (2075-4434), 2022, v. 10, n. 6, p. 118, doi. 10.3390/galaxies10060118
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On the Evolution of the Hubble Constant with the SNe Ia Pantheon Sample and Baryon Acoustic Oscillations: A Feasibility Study for GRB-Cosmology in 2030.
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- Galaxies (2075-4434), 2022, v. 10, n. 1, p. 24, doi. 10.3390/galaxies10010024
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The Flatness Problem and the Variable Physical Constants.
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- Galaxies (2075-4434), 2019, v. 7, n. 3, p. 77, doi. 10.3390/galaxies7030077
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Determining Evolution of Cosmological Constant, Gravitational Constant and Speed of Light Using Nonadiabatic Cosmological Model and LLR Findings.
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- Galaxies (2075-4434), 2019, v. 7, n. 3, p. 67, doi. 10.3390/galaxies7030067
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Varying Physical Constants, Astrometric Anomalies, Redshift and Hubble Units.
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- Galaxies (2075-4434), 2019, v. 7, n. 2, p. 55, doi. 10.3390/galaxies7020055
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Hubble parameter estimation via dark sirens with the LISA-Taiji network.
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- National Science Review, 2022, v. 9, n. 2, p. 1, doi. 10.1093/nsr/nwab054
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Dust Fluid Cosmological Model.
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- ISRN Astronomy & Astrophysics, 2013, p. 1, doi. 10.1155/2013/293298
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Exact Solutions for Bianchi Type-I Cosmological Models in f(R) Theory of Gravity.
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- Applications & Applied Mathematics, 2019, v. 14, n. 1, p. 334
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Towards a New Proposal for the Time Delay in Gravitational Lensing.
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- Symmetry (20738994), 2017, v. 9, n. 10, p. 202, doi. 10.3390/sym9100202
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Bouncing Cosmology in fG,T Gravity with Logarithmic Trace Term.
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- Advances in Astronomy, 2021, p. 1, doi. 10.1155/2021/8852581
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Oscillating Cosmological Solutions in the Modified Theory of Induced Gravity.
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- Advances in Astronomy, 2019, p. 1, doi. 10.1155/2019/1502453
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Parameterizing the SFC Baryogenesis Model.
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- Advances in Astronomy, 2015, v. 2015, p. 1, doi. 10.1155/2015/425342
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Holographic Polytropic f(T) Gravity Models.
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- Advances in High Energy Physics, 2015, p. 1, doi. 10.1155/2015/798902
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Cosmological Analysis of Dynamical Chern-Simons Modified Gravity via Dark Energy Scenario.
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- Advances in High Energy Physics, 2015, v. 2015, p. 1, doi. 10.1155/2015/259578
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Hubble Parameter Corrected Interactions in Cosmology.
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- Advances in High Energy Physics, 2014, p. 1, doi. 10.1155/2014/129085
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