activity
20132023
most citedGeV excess in the Milky Way: The Role of Diffuse Galactic gamma ray Emission template

169 citations · 841 across the 22 of their papers we have counts for

collaborators

22 papers

hep-ph2023

The Photon Content of the Neutron

Keping Xie, Bei Zhou, T. J. Hobbs

In this work, we complete our CT18qed study with the neutron's photon parton distribution function (PDF), which is essential for the nucleus scattering phenomenology. Two methods,…

hep-ph2023★ 12 cited

Scalar Co-SIMP Dark Matter: Models and Sensitivities

Aditya Parikh, Juri Smirnov, Weishuang Linda Xu +1

In this work, we present UV completions of the recently proposed number-changing Co-SIMP freeze-out mechanism. In contrast to the standard cannibalistic-type dark matter picture th…

astro-ph.HE2022★ 10 cited

High-energy neutrinos from choked-jet supernovae: Searches and implications

Po-Wen Chang, Bei Zhou, Kohta Murase +1

The origin of the high-energy astrophysical neutrinos discovered by IceCube remains largely unknown. Multimessenger studies have indicated that the majority of these neutrinos come…

gr-qc2022★ 8 cited

Compact Binary Foreground Subtraction in Next-Generation Ground-Based Observatories

Bei Zhou, Luca Reali, Emanuele Berti +4

The stochastic gravitational-wave backgrounds (SGWBs) for current detectors are dominated by binary black-hole (BBH) and binary neutron-star (BNS) coalescences. The sensitivity of…

gr-qc2022★ 41 cited

Subtracting Compact Binary Foregrounds to Search for Subdominant Gravitational-Wave Backgrounds in Next-Generation Ground-Based Observatories

Bei Zhou, Luca Reali, Emanuele Berti +4

Stochastic gravitational-wave backgrounds (SGWBs) derive from the superposition of numerous individually unresolved gravitational-wave (GW) signals. Detecting SGWBs provides us wit…

astro-ph.HE2021★ 3 cited

Seeking Neutrino Emission from AGN through Temporal and Spatial Cross Correlation

Cyril Creque-Sarbinowski, Marc Kamionkowski, Bei Zhou

Active galactic nuclei (AGN) are a promising source for high-energy astrophysical neutrinos (HEANs). By the end of 2022, the Vera C. Rubin Observatory (VRO) will begin to observe $…