Sep 2 – 6, 2024
Machupicchu Pueblo (Aguas Calientes), Peru
America/Lima timezone

Physics and Cosmology on a Gravitational Wave Background

Not scheduled
20m
Pachacuteq Theater (Machupicchu Pueblo (Aguas Calientes), Peru)

Pachacuteq Theater

Machupicchu Pueblo (Aguas Calientes), Peru

Aguas Calientes 08681, Peru
Talk

Speaker

Dr Tonatiuh Matos (Cinvestav)

Description

It is a fact that the universe lives on a Gravitational Wave Background (GWB), which may be in the form of extra energy, which is not contained in Einstein's field equations. In previous work, a new model called Compton Mass Dark Energy (CMaDE) was developed to explain the current accelerated expansion of the universe where a GWB was incorporated by extending Einstein's equations to
$R_{\mu\nu}-\frac{1}{2}Rg_{\mu\nu}+\frac{2\pi^2}{\lambda^2}g_{\mu\nu}=\kappa^2T_{\mu\nu}$,
where $\lambda$ is the Compton wavelength of the graviton. In the present talk we show that the geodesics in a GWB satisfy the Klein Gordon equation and then we show that
the CMaDE model agrees very well with the observations of the cosmic chronometers, Baryon Acoustic Oscillations and Pantheon Super Novae type Ia, reproducing the observational data with a $\Delta\chi^2 = 3.26$ in favor of the current model compared to the ΛCDM. The values favored by these observations are $\Omega_m = 0.31 ± 0.02$, $H_0 = 68 ± 0.02$ Km/s/Mpc, $\Omega_k = 0.001 ± 0.011$. Using these same values we also find excellent consistency of this model with the Cosmic Microwave Background and the Power Spectrum of Matter, provided that $H_0 = 68.3$ Km/s/Mpc. We conclude that this model is an excellent alternative to explain the accelerated expansion of the universe without incorporating the cosmological constant or adding extra matter.

Author

Dr Tonatiuh Matos (Cinvestav)

Presentation materials

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