Resolving the space-time structure of sonoluminescence by intensity interferometry

Physical Review E - Statistical Physics, Plasmas, Fluids, and Related Interdisciplinary Topics

Volumn 58, Issue 1, 1998, Pages 526-531

  Slotta, Claus ^a   Heinz, Ulrich ^a  

^a UNIVERSITY OF REGENSBURG   (Germany)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0008155253     PISSN: 1063651X     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevE.58.526     Document Type: Article

References (22)

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22. In the quantum vacuum radiation scenario of Ref. 7, time profiles R(t) for the bubble radius were used that led to much larger radial velocities, which might indeed be measurable via an E dependence of the HBT radii. As pointed out in 7, these large radial velocities are not really necessary for the scenario to work because what really matters for the light generation process is the fourth time derivative of the radial velocity at the turnaround point. Still, establishing the (approximate) E independence of the HBT radii conjectured by us would put significant empirical constraints on dynamical scenarios such as the one discussed in 7.