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Nobel Prize 2020: Selected Articles on Black Hole and General Relativity

This special issue belongs to the section “Compact Objects“.

Special Issue Information

Dear Colleagues,

On behalf of the Advisory and Editorial Board members of Universe, it is a pleasure for me, as the journal’s Editor-in-Chief, to announce a Special Issue to celebrate Professor Roger Penrose, who serves on Universe’s Advisory Board, being jointly awarded the Nobel Prize in Physics 2020.

The possibility that peculiar regions in spacetime allow only for the inward motion of light and matter, which later gained notoriety as Black Holes (BHs), is one of the most exotic and, at the same time, disorienting fruits to have fallen from the branched tree of the Einsteinian General Theory of Relativity (GTR) soon after its birth. A gift that the latter’s father himself denied, convinced that there could be no realistic physical processes capable of actually creating such a bizarre spacetime configuration at the end of the gravitational collapse of any real astrophysical object. Decades later, Professor Penrose elucidated that, on the contrary, the GTR cannot avoid the formation of BHs even in physically realistic scenarios for the latter stages of the life of a sufficiently heavy star. Perhaps even more astounding and disturbing, the final act of the infalling matter after its crossing of the event horizon signals, at the BH’s center, the GTR reaching the boundaries of its validity. An unescapable spacetime singularity warns us that Einstein’s theory cannot be the last word about gravity, pointing toward the need for its marriage, to date not yet celebrated, with quantum mechanics.

A subtle red thread ideally connects such theoretical studies to the empirical investigations carried out in recent decades by the other laureates of the Nobel Prize in Physics 2020, Professor Genzel and Professor Ghez, that aimed to observationally corroborate the concept of BHs to which the results of Professor Penrose gave so firm theoretical support.

His fertile physical intuition, his multidisciplinary curiosity, and the elegance of his mathematical methods have also tirelessly led Professor Penrose on other roads at the intersection of different scientific domains. Our hope is that he will continue treading these paths, in the hope that he will discover new interesting ones.

In the footsteps of Professor Penrose, we invite all researchers in this field to contribute their valuable papers to this celebratory Special Issue of Universe.

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Key discoveries

Gravitational Lensing in Presence of Plasma: Strong Lens Systems, Black Hole Lensing and Shadow
A Model of Black Hole Evaporation and 4D Weyl Anomaly
Influence of Cosmic Repulsion and Magnetic Fields on Accretion Disks Rotating around Kerr Black Holes
Reissner–Nordström Anti-de Sitter Black Holes in Mimetic F(R) Gravity
On a Model of Magnetically Charged Black Hole with Nonlinear Electrodynamics
Searching for Quantum Black Hole Structure with the Event Horizon Telescope
Shadow Images of a Rotating Dyonic Black Hole with a Global Monopole Surrounded by Perfect Fluid
Small Black/White Hole Stability and Dark Matter
Perspectives on Constraining a Cosmological Constant-Type Parameter with Pulsar Timing in the Galactic Center
Thermodynamic Analysis of Non-Linear Reissner-Nordström Black Holes
Analogies between the Black Hole Interior and the Type II Weyl Semimetals
Kerr Black Holes within a Modified Theory of Gravity
The First Detection of Gravitational Waves
Quantum Tunneling Radiation from Loop Quantum Black Holes and the Information Loss Paradox
Investigating the Poor Match among Different Precessing Gravitational Waveforms
The Origin of Matter at the Base of Relativistic Jets in Active Galactic Nuclei
Quantum Analysis of BTZ Black Hole Formation Due to the Collapse of a Dust Shell
On the Energy of a Non-Singular Black Hole Solution Satisfying the Weak Energy Condition

Further reading

Classical Collapse to Black Holes and Quantum Bounces: A Review
Black Holes: Eliminating Information or Illuminating New Physics?
Dark Energy and Spacetime Symmetry
Brief Review on Black Hole Loop Quantization
Generic Features of Thermodynamics of Horizons in Regular Spherical Space-Times of the Kerr-Schild Class
The Effects of Finite Distance on the Gravitational Deflection Angle of Light
Approaching the Black Hole by Numerical Simulations
Jetted Narrow-Line Seyfert 1 Galaxies & Co.: Where Do We Stand?
Visible Shapes of Black Holes M87* and SgrA*

Prof. Dr. Lorenzo Iorio
Collection Editor

Manuscript Submission Information

Manuscripts should be submitted online at www.mdpi.com by registering and logging in to this website. Once you are registered, click here to go to the submission form. Manuscripts can be submitted until the deadline. All submissions that pass pre-check are peer-reviewed. Accepted papers will be published continuously in the journal (as soon as accepted) and will be listed together on the special issue website. Research articles, review articles as well as short communications are invited. For planned papers, a title and short abstract (about 250 words) can be sent to the Editorial Office for assessment.

Submitted manuscripts should not have been published previously, nor be under consideration for publication elsewhere (except conference proceedings papers). All manuscripts are thoroughly refereed through a single-blind peer-review process. A guide for authors and other relevant information for submission of manuscripts is available on the Instructions for Authors page. Universe is an international peer-reviewed open access monthly journal published by MDPI.

Please visit the Instructions for Authors page before submitting a manuscript. Submitted papers should be well formatted and use good English. Authors may use MDPI's English editing service prior to publication or during author revisions.

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Universe - ISSN 2218-1997