Testing the Newton second law in the regime of small accelerations
arXiv:1002.2766 · doi:10.1051/0004-6361/200811520
Abstract
It has been pointed out that the Newtonian second law can be tested in the very small acceleration regime by using the combined movement of the Earth and Sun around the Galactic center of mass. It has been shown that there are only two brief intervals during the year in which the experiment can be completed, which correspond to only two specific spots on the Earth surface. An alternative experimental setup is presented to allow the measurement to be made on Earth at any location and at any time.
5 pages
References in corpus (27)
- Particle Dark Matter: Evidence, Candidates and Constraints
- A direct empirical proof of the existence of dark matter
- Relativistic gravitation theory for the MOND paradigm
- Non-Baryonic Dark Matter - Observational Evidence and Detection Methods
- Modified Newtonian Dynamics as an Alternative to Dark Matter
- Modified Newtonian Dynamics in the Milky Way
- A Dark-Matter Spike at the Galactic Center?
- On the Proof of Dark Matter, the Law of Gravity and the Mass of Neutrinos
- A Dark Core in Abell 520
- The dwarf galaxy DDO 47 as a dark matter laboratory: testing cusps hiding in triaxial halos
- Tidal dwarf galaxies as a test of fundamental physics
- Insight into the baryon-gravity relation in galaxies
- Spectroscopic study of blue compact galaxies V. oxygen abundance and the metallicity-luminosity relation
- Milky Way potentials in CDM and MOND. Is the Large Magellanic Cloud on a bound orbit?
- Escaping from MOND
- Determining the WIMP mass using direct detection experiments
- Loss of mass and stability of galaxies in MOND
- Hubble Space Telescope survey of the Perseus Cluster - I: The structure and dark matter content of cluster dwarf spheroidals
- Could dark energy be measured in the lab?
- Forming Galaxies with MOND
- A weak lensing estimate from GEMS of the virial to stellar mass ratio in massive galaxies to z~0.8
- Is violation of Newton's second law possible?
- Analysis of galactic tides and stars on CDM microhalos
- Spectroscopic study of blue compact galaxies IV. Star formation rates and gas depletion timescales
- Has Dark Energy really been discovered in the Lab?
- Testing MOND with Local Group spiral galaxies
- Galaxy Bulges As Tests of CDM vs MOND in Strong Gravity
Cited by in corpus (5)
- A Machian Request for the Equivalence Principle in Extended Gravity and non-geodesic motion
- The Double Galaxy Cluster Abell 2465 I. Basic Properties: Optical Imaging and Spectroscopy
- Satellite Test of the Equivalence Principle as a Probe of Modified Newtonian Dynamics
- Testing MOND on Earth
- Constraining the MOdified Newtonian Dynamics from spherically symmetrical hydrodynamic accretion