Gravitational Wave in the Theory with the Universal Charge

2021

IJAA

The problem of gravitation near the Schwarzschild radius is addressed. The pressure due to free fall velocity is introduced. At the Schwarz-schild radius, this pressure produces the force balancing the gravity thus stopping the collapse of the matter. The minimum radius of the source of gravity is defined as a radius at which the proton reaches the Planck energy. The compact object as a thin shell at the minimum radius is considered. The proton is assumed to decay at the Planck scale into positron and hypothetical Planck neutrinos. Under accretion onto the compact object, half the protons decay, and the other protons retain at the minimum radius.

Section: Introductionsupporting

confidence: 65%

Gravitation near the Schwarzschild radius

2021

IJAA

“…Consider the scenario in which UHECRs arise in the decay of the protons falling onto the gravastar. Assume that the proton decays at the Planck scale into positron and four hypothetical Planck neutrinos, p → e + 4ν Pl , as it was proposed in Khokhlov (2011). Suppose that Planck neutrino is a massless particle which takes part in the interaction at the Planck scale (Newton gravity, scattering by the proton), and does not in the electromagnetic, weak and strong interactions.…”

Section: Planck Neutrino Spectrummentioning

confidence: 99%

“…Consider the scattering of the Planck neutrinos by the proton at the Planck scale. The interaction at the Planck scale is supposed to go through the tensor Planck field of the Planck mass (Khokhlov 2011). Keeping in mind p → e + 4ν Pl , one can describe the process as…”

Section: Planck Neutrino Spectrummentioning

confidence: 99%

“…Then, the protons are scattered at the Planck scale. The Lagrangian of the interaction at the Planck scale can be written in the form (Khokhlov 2011…”

Section: Planck Neutrino Spectrummentioning

confidence: 99%

“…One may consider another mode of the proton decay. The decay of proton at the Planck scale into positron and hypothetical Planck neutrinos, p → e + 4ν Pl , was proposed in Khokhlov (2011). To this end, Planck neutrino may be considered as a dark matter candidate (Khokhlov 2015).…”

Section: Introductionmentioning

confidence: 99%

See 2 more Smart Citations

Planck Neutrinos as Ultra High Energy Cosmic Rays

2020

Open Astronomy

AbstractThe studied conjecture is that ultra high energy cosmic rays (UHECRs) are hypothetical Planck neutrinos arising in the decay of the protons falling onto the gravastar. The proton is assumed to decay at the Planck scale into positron and four Planck neutrinos. The supermassive black holes inside active galactic nuclei, while interpreted as gravastars, are considered as UHECR sources. The scattering of the Planck neutrinos by the proton at the Planck scale is considered. The Planck neutrinos contribution to the CR events may explain the CR spectrum from 5 × 1018 eV to 1020 eV. The muon number in the Planck neutrinos-initiated shower is estimated to be larger by a factor of 3/2 in comparison with the standard model that is consistent with the observational data.

Dark matter radiation from Sgr A ∗ $\mbox{A}^{*}$

2015

Astrophys Space Sci

An excess of 511 keV radiation from positron annihilation from the centre of the Galaxy may be explained by the decay of the protons falling onto Sgr A * while interpreting Sgr A * as a gravitational vacuum star. In a recent paper, this explanation was studied against the constraints imposed by the accretion rate onto Sgr A * and the observed luminosity of Sgr A * . The photons as proton decay products are ruled out by the constraints. The proton decay products may be interpreted as dark matter particles. Then, Sgr A * may be considered a source of dark matter radiation. In the present paper, observational constraints on the supposed flux of dark matter radiation from Sgr A * are under consideration.