Results 121 to 130 of about 114,518 (203)
Determination of the Hubble Constant
Recent developments in the determination of H0 are reviewed in the context of the 3 following questions: 1) What is required to measure an accurate value of H0? Given the wide range of H0 values quoted in the current literature, is there any evidence that the situation has changed very much at all in the last couple of decades? And 3), is a measurement
openaire +2 more sources
Testing the coupling of dark radiations in light of the Hubble tension
We are studying the effects of Self-Interacting dark radiation (SIdr) on the evolution of the universe. Our main focus is on the cosmic microwave background (CMB) and how SIdr could potentially help resolve the Hubble tension.
Zhiyu Lu +3 more
doaj +1 more source
Time-Delay Cosmography: Measuring the Hubble Constant and Other Cosmological Parameters with Strong Gravitational Lensing. [PDF]
Birrer S +8 more
europepmc +1 more source
Tension in the Hubble constant
There has been some hand-wringing of late about the tension between the value of the expansion rate of the universe – the famous Hubble constant, H <sub> 0 </sub> , measured directly from observed redshifts and distances, and that obtained by multi-parameter fits to the cosmic microwave background.
openaire +1 more source
Two Dynamical Scenarios for Binned Master Sample Interpretation. [PDF]
Montani G +3 more
europepmc +1 more source
Information Storage in a Black Hole's Gravitational Field. [PDF]
He D, Li J, Qiu Q.
europepmc +1 more source
f(Q) gravity as a possible resolution of the H<sub>0</sub> and S<sub>8</sub> tensions with DESI DR2. [PDF]
Kavya NS, Swagat Mishra S, Sahoo PK.
europepmc +1 more source
Screened axio-dilaton cosmology: novel forms of early dark energy. [PDF]
Smith A +4 more
europepmc +1 more source
The nature of phantom dark energy and its relation to time crystals. [PDF]
Mersini-Houghton L.
europepmc +1 more source
Challenges to the [Formula: see text]CDM cosmology. [PDF]
Efstathiou G.
europepmc +1 more source

