no code implementations • 10 Feb 2021 • Oscar Macias, Harm van Leijen, Deheng Song, Shin'ichiro Ando, Shunsaku Horiuchi, Roland M. Crocker
We forecast that, in the event that $e^\pm$ injection spectra are harder than $E^{-2}$, CTA has the potential to robustly discover the IC signature of a putative Galactic bulge MSP population sufficient to explain the GCE for $e^\pm$ injection efficiencies in the range $\approx 2. 9-74. 1\%$, or higher, depending on the level of mismodeling of the Galactic diffuse emission components.
High Energy Astrophysical Phenomena
no code implementations • 2 Feb 2021 • Natalia Tapia Arellano, Shunsaku Horiuchi
Measuring the solar neutrino flux over gigayear timescales could provide a new window to inform the Solar Standard Model as well as studies of the Earth's long-term climate.
High Energy Physics - Phenomenology High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics Solar and Stellar Astrophysics High Energy Physics - Experiment
1 code implementation • 1 Jul 2019 • Hirokazu Sasaki, Tomoya Takiwaki, Shio Kawagoe, Shunsaku Horiuchi, Koji Ishidoshiro
We also show that if the spectrum of $\bar{\nu}_e$ in HK becomes softer due to CNO, the spectrum of $\nu_e$ in DUNE becomes harder, and vice versa.
High Energy Astrophysical Phenomena High Energy Physics - Phenomenology
