2011/05/31 by V. Fleurov, R. Schilling · 1 citation
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Entropy (arrow of time) #Hawking radiation #Horizon #Mathematical physics #Physics #Quantum #Quantum Electrodynamics and Casimir Effect #Quantum electrodynamics #Quantum fluctuation #Quantum mechanics #Regularization (linguistics) #cond-mat.quant-gas #nlin.PS #physics.optics
paper · pdf · doi:10.1103/physreva.85.045602
23 pages, 2 figures
arxiv created 2011/11/29 · openalex publication_date 2012/04/30 · arxiv updated 2015/05/28 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We consider dynamics of fluctuations in transonically accelerating Bose-Einstein condensates and/or luminous fluids using the hydrodynamic approach. It is known that neglecting the quantum potential (QP) leads to a singular behavior of quantum and classical fluctuations in the vicinity of the Mach (sonic) horizon, which in turn gives rise to Hawking radiation. The neglect of the QP is well founded at not too small distances |x|\ensuremath≫lh from the horizon, where lh is the healing length. Taking the QP into account, we show that a second characteristic length lr>lh exists, such that the linear fluctuation modes become regularized for |x|\ensuremath≪lr. At |x|\ensuremath≫lr the modes keep their singular behavior, which, however, is influenced by the QP. As a result we find a deviation of the high frequency tail of the spectrum of Hawking radiation from Planck's black-body radiation distribution, which can be described by an effective Hawking temperature decreasing with increasing frequency.