Cosmic Neutrinos and Multi-messenger Workshop "CosNuMM2019"

Session

Cosmic neutrinos and multi-messenger

29 Nov 2019, 14:00

Tsung-Dao Lee Institute (East wing of Pao Yue-Kong Library)

Conveners

Cosmic neutrinos and multi-messenger

• Anatoli Fedynitch (Institute of Cosmic Ray Research)

43. On the astrophysical sources of high-energy neutrinos

Prof. Xiangyu Wang (Nanjing U)

29/11/2019, 14:00

44. Constraints on diffuse high energy neutrino flux from star-forming galaxies

Mr Tianqi Huang (Peking U)

29/11/2019, 14:25

45. Status of LHAASO and its multi-messenger program

Dr Yi Zhang (IHEP)

29/11/2019, 14:40

46. Latest results from DAMPE

Qiang Yuan (Purple Mountain Observatory)

29/11/2019, 15:05

9. Constraints on diffuse high energy neutrino flux from Star-forming Galaxies

Mr Tianqi Huang (Peking University)

If star-forming galaxies could accelerate cosmic ray to very high energies, high energy neutrinos and gamma-ray photons will be produced during cosmic ray propagation. Considering the gamma-ray point sources below the detection threshold, the source count distribution above 50 GeV places an upper limit on non-blazar component of the EGB measured by Fermi-LAT. Keith Bechtol et al. found a...