First Observation of an X-Ray Beam Following a New Geodesic When Gravitational Waves Deform Space-Time

Jimenez, Edward S.; Recalde, Nicolas; Álvarez-Samaniego, Wilson P.; Álvarez-Samaniego, Borys; Moya-Álvarez, Douglas; Jiménez, Esteban

doi:10.5539/jmr.v11n2p53

Cited by 1 publication

(1 citation statement)

References 9 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…This risky conjecture has the support of the advances made in the first photo of a black hole and its correspondence with Einstein's gravitation equations. In addition, it is categorically demonstrated that Einstein's equations not only relate to Navier Stokes' equations but are equivalent in the event horizon [9][10][11]. I. Bredberg et al (2012) probes the respective theorems From Einstein to Navier Stokes as follows.…”

Section: Modelmentioning

confidence: 99%

Quantum Gravity Strategy for the Production of Dark Matter Using Cavitation by Minimum Entropy

Jiménez

Jimenez

2019

The 5th International Electronic Conference on Entropy and Its Applications

Self Cite

View full text Add to dashboard Cite

The minimum entropy is responsible for the formation of dark matter bubbles in a black hole, while the variation in the density of dark matter allows these bubbles to leave the event horizon. Some experimental evidence supports the dark matter production model in the inner vicinity of the border of a black hole. The principle of minima entropy explains how cavitation occurs on the event horizon, which in turn complies with the Navier–Stokes 3D equations. Moreover, current works in an axiomatic way show that in the event horizon Einstein’s equations are equivalent to Navier–Stokes’ equations. Thus, The solutions of Einstein combined with the boundary conditions establish a one-to-one correspondence with solutions of incompressible Navier–Stokes and in the near-horizon limit it provides a precise mathematical sense in which horizons are always incompressible fluids. It is also essential to understand that Cavitation by minimum entropy is the production of dark matter bubbles, by variation of the pressure inside or on the horizon of a black hole, in general Δ p = p n + 1 − p n = σ n σ n + 1 − 1 p n or in particular Δ p = − ( 1 − P ) p 0 , where ∂ P ∂ t = Δ p ρ 0 P . Finally, fluctuations in the density of dark matter can facilitate its escape from a black hole, if and only if there is previously dark matter produced by cavitation inside or on the horizon of a black hole and also ρ D M < ρ B .

show abstract

Section: Modelmentioning

confidence: 99%