Median statistics estimates of Hubble and Newton's Constant
arXiv:1701.01789 · doi:10.1140/epjp/i2017-11390-3
Abstract
Robustness of any statistics depends upon the number of assumptions it makes about the measured data. We point out the advantages of median statistics using toy numerical experiments and demonstrate its robustness, when the number of assumptions we can make about the data are limited. We then apply the median statistics technique to obtain estimates of two constants of nature, Hubble Constant () and Newton's Gravitational Constant(), both of which show significant differences between different measurements. For , we update the analysis done by Chen and Ratra (2011) and Gott et al. (2001) using measurements. We find after grouping the different results according to their primary type of measurement, the median estimates are given by km/sec/Mpc with errors corresponding to 95% c.l. (2) and corresponding to 68% c.l. (1).
8 pages. For full list of and G measurements, see http://goo.gl/gJ2hAn
References in corpus (6)
- Bayes in the sky: Bayesian inference and model selection in cosmology
- The trouble with
- Measurements of Newton's gravitational constant and the length of day
- Recent measurements of the gravitational constant as a function of time
- Bayesian Model Averaging in Astrophysics: A Review
- Frequentist model comparison tests of sinusoidal variations in measurements of Newton's gravitational constant
Cited by in corpus (17)
- Late time acceleration due to generic modification of gravity and Hubble tension
- A test of cosmic distance duality relation using SPT-SZ galaxy clusters, Type Ia supernovae, and cosmic chronometers
- Growth Rate and Configurational Entropy in Tsallis Holographic Dark Energy
- Vacuum dynamics in the Universe versus a rigid const
- MFV approach to robust estimate of neutron lifetime
- The Hubble constant from galaxy cluster scaling-relation and SNe Ia observations: a consistency test
- Bayesian inference of -boson mass
- Determination of Hubble constant from Megamaser Cosmology Project using Profile Likelihood
- Effect of Peak Absolute Magnitude of Type Ia Supernovae and Sound Horizon Values on Hubble Tension using DESI results
- A test for the redshift dependence of using measurements
- A meta-analysis of distance measurements to M87
- Implications of Dynamical Dark Energy in the expansion of the Universe and the Structure Formation
- Median Statistics Estimate of the Distance to M87
- Comparison of CDM and with updated galaxy cluster measurements using Bayesian inference
- Search for variability in Newton's constant using local gravitational acceleration measurements
- Testing the cosmic distance duality relation using model-independent approach
- A Chi-Squared Analysis of the Measurements of Two Cosmological Parameters Over Time