FIG 2 - uploaded by Samira Elghaayda
Content may be subject to copyright.
Download
View publication
A Penrose diagram is used to represent SST and showing trajectories for (O1) and (O2), where (O1) is free-falling toward the SBH and (O2) is static. Region III represents the inside of the SBH while regions I and II represent the outside of the SBH. The white hole is located in region IV.

A Penrose diagram is used to represent SST and showing trajectories for (O1) and (O2), where (O1) is free-falling toward the SBH and (O2) is static. Region III represents the inside of the SBH while regions I and II represent the outside of the SBH. The white hole is located in region IV.

Source publication
FIG. 2. A Penrose diagram is used to represent SST and showing...
FIG. 3. One-dimensional Rindler space-time diagram. Here, the curve is...
Distribution of distance-based quantum resources outside a radiating Schwarzschild black hole
Preprint
Full-text available
  • Feb 2024
We obtain analytical expressions for distance-based quantum resources and examine their distribution in the proximity of a Schwarzschild black hole (SBH) within a curved background. For an observer in free fall and their stationary counterpart sharing the Gisin state, the quantum resources are degraded at infinite Hawking temperature. The extent of...
Cite
Download full-text

Similar publications

Figure 1 summarizes the current ideas on these transitions. For small...
Figure 2. The structure of a neutron star.
Figure 3. Phases of matter at supernuclear density before the collapse.
Figure 4. The superstring vision of colour and flavour locking as a...
Does the colour-flavour locking phase of quark matter determine the scenario for black hole evaporation?
Preprint
Full-text available
  • Apr 2024
We present for consideration a hypothesis of the event horizon formation in the observed black holes of finite size based on the correspondence between the processes described by the quantum chromodynamics and the superstring theory. The relationship between the evaporation of black holes through the Hawking radiation and super-symmetric boson tran...
View
FIG. 5. Specific heat of the black hole against its event horizon...
FIG. 6. Specific heat of the black hole against the event horizon...
FIG. 7. Energy density vs rH plot for ωq = −2/3 when α = 0.05 and α = 0..
FIG. 8. ρq vs rH plot ωq = −1/3. We compare the QGUP case with the...
+3 FIG. 10. x(t) = M (t) mp is plotted against the dimensionless time t t...
Thermodynamics of a Schwarzschild black hole surrounded by quintessence in the generalized uncertainty principle framework
Preprint
Full-text available
  • Sep 2024
We investigate the thermodynamics of a Schwarzschild black hole, surrounded by the quintessence energy-matter in the linear and quadratic generalized uncertainty principle framework. Considering the variance in the position to be of the order of the event horizon radius and equating the variance in the momentum to the Hawking temperature of the bla...
View