GRB 060614 as a Candidate White Hole Event: Energetics, Relativistic Dynamics, Jet Geometry, Radiative Processes, and Quantum Bounce Constraints

Author(s)	Mr. Anthony J Waterfield
Country	United States
Abstract	GRB 060614 is a long-duration gamma-ray burst (T90 ∼ 108 s) that lacks an associated supernovadespite its low redshift (z ≈ 0.125), making it a major outlier in standard GRB classification. In thiswork we present an expanded analysis including energetics, relativistic dynamics, synchrotron radiation physics, radiative transfer, environmental constraints, and quantum gravity considerations. Weevaluate whether a white-hole or black-hole-to-white-hole transition can reproduce observed properties.While mathematically viable, such models require extreme fine tuning and remain less favored thanmerger or fallback accretion scenarios.
Keywords	Gamma-Ray Burst, White Hole, Synchrotron Emission, Relativistic Outflows, Quantum Bounce, Compact Binary Merger
Field	Physics > Astronomy
Published In	Volume 7, Issue 4, July-August 2026
Published On	2026-08-22

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