PanScales parton showers for hadron collisions: formulation and fixed-order studies
Journal of High Energy Physics Springer Nature 2022:11 (2022) 19
PanScales showers for hadron collisions: all-order validation
Journal of High Energy Physics Springer Nature 2022:11 (2022) 20
Ising Machines for Diophantine Problems in Physics
Fortschritte Der Physik 70:11 (2022)
Abstract:
Diophantine problems arise frequently in physics, in for example anomaly cancellation conditions, string consistency conditions and so forth. We present methods to solve such problems to high order on annealers that are based on the quadratic Ising Model. This is the intrinsic framework for both quantum annealing and for common forms of classical simulated annealing. We demonstrate the method on so-called Taxicab numbers (discovering some apparently new ones), and on the realistic problem of anomaly cancellation in U(1) extensions of the Standard Model.Searches for Neutrinos from Gamma-Ray Bursts Using the IceCube Neutrino Observatory
Astrophysical Journal 939:2 (2022)
Abstract:
Gamma-ray bursts (GRBs) are considered as promising sources of ultra-high-energy cosmic rays (UHECRs) due to their large power output. Observing a neutrino flux from GRBs would offer evidence that GRBs are hadronic accelerators of UHECRs. Previous IceCube analyses, which primarily focused on neutrinos arriving in temporal coincidence with the prompt gamma-rays, found no significant neutrino excess. The four analyses presented in this paper extend the region of interest to 14 days before and after the prompt phase, including generic extended time windows and targeted precursor searches. GRBs were selected between 2011 May and 2018 October to align with the data set of candidate muon-neutrino events observed by IceCube. No evidence of correlation between neutrino events and GRBs was found in these analyses. Limits are set to constrain the contribution of the cosmic GRB population to the diffuse astrophysical neutrino flux observed by IceCube. Prompt neutrino emission from GRBs is limited to 21% of the observed diffuse neutrino flux, and emission on timescales up to 104 s is constrained to 24% of the total diffuse flux.Search for quantum gravity using astrophysical neutrino flavour with IceCube
Nature Physics Springer Nature 18:11 (2022) 1287-1292