We perform an angular analysis of the decay for the dielectron mass squared, , range of using the full Belle dataset in the and channels, incorporating new methods of electron identification to improve the statistical power of the dataset. This analysis is sensitive to contributions from right-handed currents from physics beyond the Standard Model by constraining the Wilson coefficients . We perform a fit to the differential decay rate and measure the imaginary component of the transversality amplitude to be , and the transverse asymmetry to be , with and fixed to the Standard Model values. The resulting constraints on the value of are consistent with the Standard Model within a confidence interval. Published by the American Physical Society2024 
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                    This content will become publicly available on March 1, 2026
                            
                            Condensate decay in a radiation dominated cosmology
                        
                    
    
            We study the decay of a homogeneous condensate of a massive scalar field of mass into massless fields in thermal equilibrium in a radiation dominated cosmology. The model is a for the nonequilibrium dynamics of a misaligned axion condensate decaying into radiation. After consistent field quantization in the cosmological background, we obtain the linearized causal equations of motion for a homogeneous condensate including the finite temperature self-energy corrections up to one loop. The dynamical renormalization group is implemented to obtain the time dependent relaxation rate that describes the decay dynamics of the condensate amplitude from stimulated emission and recombination of massless quanta in the medium. It is explicitly shown that a simple friction term in the equation of motion does not describe correctly the decay of the condensate. During the super-Hubble regime, relevant for ultralight dark matter, the condensate amplitude decays as . In the sub-Hubble regime the amplitude decays as with ; therefore, the finite temperature contribution to the decay rate vanishes fast during the expansion. A main conclusion is that a phenomenological friction term is inadequate to describe the decay in the super-Hubble regime, and the decay function is always than that from a local friction term as a consequence of the cosmological expansion. For ultralight dark matter, the timescale, during which transient dynamics is sensitive to cosmological expansion and a local friction term is inadequate, is much longer. A friction term always the timescale of decay in the sub-Hubble case. Published by the American Physical Society2025 
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                            - Award ID(s):
- 2412374
- PAR ID:
- 10596763
- Editor(s):
- Ray, Rashmi
- Publisher / Repository:
- physical review d
- Date Published:
- Journal Name:
- Physical Review D
- Edition / Version:
- 1
- Volume:
- 111
- Issue:
- 6
- ISSN:
- 2470-0010
- Page Range / eLocation ID:
- 1-26
- Subject(s) / Keyword(s):
- condensate decay cosmology
- Format(s):
- Medium: X Size: 26 pages Other: xls
- Size(s):
- 26 pages
- Sponsoring Org:
- National Science Foundation
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