# Accelerating Universe: Theory versus Experiment

@article{Carmeli2002AcceleratingUT, title={Accelerating Universe: Theory versus Experiment}, author={Moshe Carmeli}, journal={arXiv: Astrophysics}, year={2002} }

We present gravitation as a theory in which the coordinates are distances and velocities between galaxies. We show that there are three possibilities for the Universe to expand: decelerating, constant and accelerating, and it is shown that the Universe is now in the latter phase. Assuming "Omega"_m=0.245, the time at which the Universe goes over from a decelerating to an accelerating expansion, occurs at 8.5 Gyr ago, at which time the cosmic radiation temperature was 146K. The theory predicts…

## 20 Citations

### Testing Cosmological General Relativity against high redshift observations

- Physics
- 2006

Several key relations are derived for Cosmological General Relativity which are used in standard observational cosmology. These include the luminosity distance, angular size, surface brightness and…

### Carmeli's Cosmology Fits Data for an Accelerating and Decelerating Universe Without Dark Matter or Dark Energy

- Physics
- 2006

A new relation for the density parameter Ω is derived as a function of expansion velocity υ based on Carmeli's cosmology. This density function is used in the luminosity distance relation DL. A…

### Extending the Redshift-Distance Relation in Cosmological General Relativity to Higher Redshifts

- Physics
- 2008

Abstract
The redshift-distance modulus relation, the Hubble Diagram, derived from Cosmological General Relativity has been extended to arbitrarily large redshifts. Numerical methods were employed and…

### Cosmological General Relativity against high redshift observations

- Physics
- 2007

Several key relations are derived for Cosmological General Relativity which are used in standard observational cosmology. These include the luminosity distance, angular size, surface brightness and…

### A Valid Finite Bounded Expanding Carmelian Universe Without Dark Matter

- Physics
- 2013

The solution of Einstein’s field equations in Cosmological General Relativity (CGR), where the Galaxy is at or cosmologically near the center of a finite yet bounded spherically symmetrical isotropic…

### The Distance Modulus Determined from Carmeli’s Cosmology Fits the Accelerating Universe Data of the High-redshift Type Ia Supernovae Without Dark Matter

- Physics
- 2006

The velocity of the Hubble expansion has been added to General Relativity by Moshe Carmeli and this resulted in new equations of motion for the expanding universe. For the first time the…

### Finite Bounded Expanding Carmelian White Hole Universe Without Dark Matter

- Physics
- 2012

The solution of Einstein’s field equations in Cosmo logical General Relativity (CGR), where the Galaxy is at or cosmologically near the center of a finite yet b ounded spherically symmetrical…

### Testing CGR against High Redshift Observations

- Physics
- 2008

Several key relations are derived for Cosmological General Relativity which are used in standard observational cosmology. These include the luminosity distance, angular size, surface brightness and…

### A pr 2 00 7 Finite bounded expanding white hole universe without dark matter

- Physics
- 2008

The solution of Einstein’s field equations in Cosmological General Relativity (CGR), where the Galaxy is at the center of a finite yet bounded spherically symmetrical isotropic gravitational field,…

### Properties of Gravitational Waves in Cosmological General Relativity

- Physics
- 2006

The 5D Cosmological General Relativity theory developed by Carmeli reproduces all of the results that have been successfully tested for Einstein's 4D theory. However the Carmeli theory because of its…

## References

SHOWING 1-6 OF 6 REFERENCES

### The Meaning of Relativity

- Physics
- 1921

In 1921, five years after the appearance of his comprehensive paper on general relativity and twelve years before he left Europe permanently to join the Institute for Advanced Study, Albert Einstein…

### Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant

- Physics
- 1997

We present here the final results of the Hubble Space Telescope (HST) Key Project to measure the Hubble constant. We summarize our method, the results, and the uncertainties, tabulate our revised…

### Cosmological special relativity : the large-scale structure of space, time and velocity

- Physics
- 1997

Cosmological special relativity: fundamentals of special relativity present-day cosmology postulates cosmic frames space velocity in cosmology pre-special-relativty relative cosmic time inadequacy of…

### Classical Fields: General Relativity and Gauge Theory

- Physics, Geology
- 1982

The gravitational field the geometry of curved space-time the Einstein field equations gravitational fields of elementary mass systems properties of the gravitational field equations of motion in…

### Status of the big bang cosmology, in: Texas/Pascos 92: Relativistic Astrophysics and Particle Cosmology

- C.W. Akerlof and M.A. Srednicki, Editors (New York Academy of Sciences,
- 1993

### Cosmological relativity: a general relativistic theory for the accelerating universe, Talk given at Dark Matter

- Los Angeles, February
- 2000