Why ghosts don't touch: a tale of two adventurers falling one after another into a black hole

Abstract

The case for the utility of Kruskal-Szekeres coordinates in classroom made by Augousti et al. in this journal (Eur. J. Phys. 33:1--11, 2012) is strengthened by extending their discussion beyond the event horizon of the black hole. Observations made by two adventurers following one another into a Schwarzschild black hole are examined in terms of these nonsingular coordinates. Two scenarios are considered, the first corresponding to one observer following the other closely, the second to a significant distance between the two of them, precluding the existence of a common inertial system. In particular, the concepts of distance and temporal separation near the horizon and the redshift of the first infaller's image as seen by the second are investigated. The results show that the notion of "touching ghosts" does not correspond to the local physics of two observers falling into a black hole. The story line is interesting enough and the mathematical details are sufficiently simple to use the example in a general relativity course, even at the undergraduate level.

arXiv commentSubmitted to European Journal of Physics, 1 figure with 2 panels

References in corpus (3)

• Black Holes: Complementarity or Firewalls?
• The river model of black holes
• Is it possible to see the infinite future of the Universe when falling into a black hole?

Cited by in corpus (4)

• The Vaidya metric: expected and unexpected traits of evaporating black holes
• Extensive/nonextensive statistics for $p_T$ distributions of various charged particles produced in p+p and A+A collisions in a wide range of energies
• Unified approach to redshift in cosmological /black hole spacetimes and synchronous frame
• Redshift/blueshift inside the Schwarzschild black hole