Black Holes, Gravitational Waves and Space Time Singularities

© SpringerThis special issue of Foundations of Physics addresses these exciting topics includes articles by several pioneers in these fields. Originating from a workshop at the Vatican Observatory in May 2017, which honored the legacy of George Lemaître.

Bellucci, S., Bonanno, A, Gabriele Gionti, S.J. and Scardigli, F. (eds):
"Special Issue: Black Holes, Gravitational Waves and Space Time Singularities",
Found Phys (2018) 48

The contents have been significantly shaped by the recent detections of gravitational waves, which have opened a new window for our understanding of the universe. They have also been fostered by recent speculations on the true nature of the space–time singularities that signal the breakdown of classical physics, and the need for a new physics to operate at the beginning of our universe and at the end of gravitational collapse. The questions focus on the limits of modern cosmology and the scientific challenges that can be explored in the near future.

A central topic to emerge from these contents is the nature of the loss of unitarity evolution inside a Black Hole. Several different approaches to Quantum Gravity theories, such as Asymptotic Safety, Loop Quantum Gravity and String Theory are discussed and compared. Some attempts at Quantum Gravity theories show that the central singularity of Quantum Black Holes (i.e., making the Black Holes “Quantum”) disappears in such a way that the information paradox can be overcome.

One clear result from the contents is that the idea of an early phase of Inflation is more of a general concept than a satisfactory theory; some of its implications such as multiverses were seriously challenged. In spite of many remaining questions, such as fine tuning and cosmological coincidence, the standard model of cosmology (ΛCDM) appears to be the most accurate theory available today in cosmology to fit the observational data; but it needs two exotic ingredients: Cold Dark Matter and Dark Energy. The very nature of Cold Dark Matter is an important theme of this special issue. Its “supersymmetric” nature appears to remain in question, while the debate continues as to whether it is a particle or something completely different.

Another hotly debated topic is the measure of the Hubble constant: attempts to measure it by direct and indirect methods give two different results.

The Conformal Cyclic Cosmology proposal deserves special mention. It attempts to solve the entropy problem of the universe; it does not need the Inflation mechanism and there is no beginning of the universe. It does account for the Cold Dark Matter and for the unitarity of loss into a Black Hole.

Of course, Gravitational Waves are another central theme of this collection. While they are a natural prediction of Einstein’s General Theory of Relativity, they have only recently been detected. They open a new window in modern cosmology and astrophysics, providing the possibility of detecting new phenomena as well as new ways of observing our universe.

The idea for this special issue was born during a workshop held in the beautiful pontifical Villas of Castel Gandolfo, home of the Vatican Observatory. This was the setting for a gathering from May 9 to 12, 2017 of forty scientists coming from Europe, America, Asia, and Africa to discuss “Black Holes, Gravitational Waves and Space–Time Singularities.” In order to set the scientific framework of the workshop, a number of renowned scientists gave invited talks. This workshop honored the person and the scientific legacy of Mons. George Lemaître, 50 years after his death. In addition, on the last day of the workshop all the participants had the privilege of being received by Pope Francis in a private audience in Vatican City.

The editors thank all authors who contributed to making this publication possible and hope, in the near future, to organize a follow-on to this workshop at the Vatican Observatory.