On the pattern of black hole information release

Understand

We propose a step towards a resolution to black hole information paradox by analyzing scattering amplitudes of a complex scalar field around a Schwarzschild black hole.

• The scattering cross section reveals much information on the incoming state but exhibits flux loss at the same time.
• The flux loss should be temporary, and indicate mass growth of the black hole.
• The black hole should Hawking-radiate subsequently, thereby, compensating for the flux loss.