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Cosmic Neutrinos and Multi-messenger Workshop "CosNuMM2019"

27–30 Nov 2019
Tsung-Dao Lee Institute (East wing of Pao Yue-Kong Library)
Asia/Shanghai timezone

Wen Wang 汪雯

Contribution List

48 out of 48 displayed
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  1. 10. Greetings
    Prof. Donglian Xu (T D Lee Institute), Prof. Wei Ku (TDLI)
    28/11/2019, 08:30

    Welcome & brief introduction of TDLI

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  2. 11. Massive neutrinos decree beyond the standard theory
    Prof. Tsutomu Yanagida (Tsung-Dao Lee Institute)
    28/11/2019, 08:40
  3. 12. Supernova & compact object neutrinos
    Prof. Mengru Wu (Academia Sinica)
    28/11/2019, 09:05
  4. 22. Supernova neutrino observables
    Prof. Shun Zhou
    28/11/2019, 09:40
  5. 23. Status of JUNO
    Prof. Liang Zhan (IHEP)
    28/11/2019, 10:30
  6. 24. Combined sensitivity to the neutrino mass ordering with JUNO and the IceCube Upgrade/PINGU
    Mr Jan Weldert (JGU Mainz)
    28/11/2019, 10:55
  7. 25. Solar neutrino detection and China's plan
    Prof. Shaomin Chen (Tsinghua)
    28/11/2019, 11:20
  8. 26. Atmospheric neutrino flux calculation at low energies
    Jie Cheng (IHEP)
    28/11/2019, 11:45
  9. 27. Observing supernova neutrinos with IceCube
    Prof. Segev BenZvi (University of Rochester )
    28/11/2019, 14:00
  10. 28. Potential sensitivity of supernova neutrino detection at PandaX-4T liquid xenon detector
    Ning Zhou (Shanghai Jiao Tong University)
    28/11/2019, 14:25
  11. 29. Early warning from pre-SN neutrinos in future large LS detectors
    Huiling Li
    28/11/2019, 14:50
  12. 30. Multi-messenger trigger system of JUNO
    Dr Ziping Ye (T. D. Lee Institute)
    28/11/2019, 15:05
  13. 58. KM3NeT online framework for neutrino alerts
    Dr Feifei Huang (CPPM)
    28/11/2019, 15:20
  14. 31. Origin of neutrino mass
    Prof. Goran Senjanovic (ICTP)
    28/11/2019, 16:00
  15. 32. How effectively can we test Quantum Gravity with JUNO?
    Prof. Antonino Marciano (Fudan University)
    28/11/2019, 16:25
  16. 33. Testing spin statistics at Gran Sasso underground laboratory
    Dr Kristian Piscicchia
    28/11/2019, 16:50
  17. 34. Brace for supernova neutrino burst by waveform compression
    Benda Xu
    28/11/2019, 17:05
  18. 35. Realtime and Multi-Messenger Astrophysics with IceCube
    Mr Raamis Hussain (UW-Madison)
    29/11/2019, 08:30
  19. 36. Status of KM3NeT/Antares and its multi-messenger program
    Prof. Pascal Coyle (CPPM)
    29/11/2019, 08:55
  20. 37. Status of Baikal-GVD and its multi-messenger program
    Prof. Olga Suvorova (INR of RAS)
    29/11/2019, 09:20
  21. 38. P-ONE and prospects towards a global neutrino telescope network
    Mr Matthias Huber (TUM)
    29/11/2019, 09:45
  22. 39. Open Universe and dissecting TXS0506+056
    Prof. Paolo Giommi (ASI)
    29/11/2019, 10:30
  23. 41. Prospects for multi-wavelength searches of neutrino sources
    Marcos Santander
    29/11/2019, 10:55
  24. 40. Finding more TeV neutrino sources
    Anatoli Fedynitch (Institute of Cosmic Ray Research)
    29/11/2019, 11:20
  25. 42. Two-zone models for the multi-messenger emission from the blazar TXS0506+056
    Ruoyu Liu (Nanjing University)
    29/11/2019, 11:45
  26. 43. On the astrophysical sources of high-energy neutrinos
    Prof. Xiangyu Wang (Nanjing U)
    29/11/2019, 14:00
  27. 44. Constraints on diffuse high energy neutrino flux from star-forming galaxies
    Mr Tianqi Huang (Peking U)
    29/11/2019, 14:25
  28. 45. Status of LHAASO and its multi-messenger program
    Dr Yi Zhang (IHEP)
    29/11/2019, 14:40
  29. 46. Latest results from DAMPE
    Qiang Yuan (Purple Mountain Observatory)
    29/11/2019, 15:05
  30. 47. Insight-HXMT in Multi-Messenger Astronomy Era
    Prof. Lian Tao (IHEP)
    29/11/2019, 16:00
  31. 48. FAST & Its Multi-messenger Program
    Dr Lei Qian (NAOC)
    29/11/2019, 16:25
  32. 49. A Bayesian approach to multi-messenger astronomy
    Prof. Xilong Fan (Wuhan U)
    29/11/2019, 16:50
  33. 50. Science program and status of GRAND
    Hao Zhou
    29/11/2019, 17:15
  34. 51. Overview of dark matter physics and the importance of “neutrino” experiments in dark matter searches
    Prof. Shigeki Matsumoto (IPMU)
    30/11/2019, 08:30
  35. 52. PTOLEMY:cosmic relic neutrino detection
    Prof. Christopher Tully (Princeton U)
    30/11/2019, 08:55
  36. 53. Gravitational waves, dark energy, and massive neutrinos
    Prof. Xin Zhang
    30/11/2019, 09:20
  37. 54. First results from KamLAND-ZEN (800kg)
    Prof. Kunio Inoue (IPMU)
    30/11/2019, 10:15
  38. 55. Neutrinoless Double Beta Decay Searches with PandaX
    Ke Han (SJTU)
    30/11/2019, 10:40
  39. 56. Probing fundamental laws of physics from multi-messenger astronomy
    Andrea Addazi (Sichuan University)
    30/11/2019, 11:05
  40. 57. Subleading corrections to heavy Higgsino and Wino direct detection
    Qing Chen (University of Kentucky)
    30/11/2019, 11:20
  41. 2. Atmospheric neutrino flux calculation at low energies
    Ms Jie Cheng (IHEP)

    The precise calculation of atmospheric neutrino fluxes in the low-energy range at JUNO is presented, where the calculating scheme is based on the method in Honda et al. Phys. Rev. D 92, 023004 (2015), but with more precise local information on the geomagnetic field, air density and mountain profile. To reduce the associated flux uncertainties, a careful consideration of the muon decay and...

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  42. 3. Brace for supernova neutrino burst by waveform compression
    Benda Xu

    The observation of neutrino burst from SN1987A provided invaluable insights on star evolution and essence of neutrinos. Because of the establishment of SuperNova Early Warning System(SNEWS), a global network of observatories has been formed for the next galactic supernova. Nevertheless, it remains a big challenge to transfer and store the complete data stream from PMT and FADC systems of...

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  43. 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...

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  44. 8. Multi-Messenger Trigger System of JUNO
    Dr Ziping Ye (T. D. Lee Institute)

    The Jiangmen Underground Neutrino Observatory (JUNO) is a 20 kton liquid scintillator detector aiming to measure neutrino mass hierarchy. With its large target mass, low threshold and excellent energy resolution, JUNO can be a powerful neutrino telescope. To fully exploit its ability of observing astrophysical neutrinos, we are developing a multi-messenger trigger system for JUNO, trying to...

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  45. 4. Pre-supernova neutrino observation in JUNO
    Huiling Li

    Jiangmen Underground Neutrino Observatory (JUNO) is one of the next-generation neutrino experiments under construction, designed with a 20 kt large liquid scintillator detector. Prior to the core-collapse of the massive stars with mass larger than 8 solar mass, the increasing sub-MeV neutrinos produced through thermal and weak nuclear processes enables their observation in JUNO. In this talk,...

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  46. 5. Probing fundamental laws of physics from Multi-Messenger astronomy
    Prof. Andrea Addazi (Sichuan University)

    New high energy astro-particle physics experiments will provide a new whole avenue towards innovative explorations of new physics beyond the Standard Model and Quantum Gravity. In this talk, we will discuss several exotic phenomena which can be probed from next generation of experiments such as LHAASO and JUNO and further other cosmic rays facilities, in a multi-messenger strategy. The most...

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  47. 7. Subleading Corrections to Heavy Higgsino and Wino Direct Detection
    Qing Chen (University of Kentucky)

    In the heavy WIMP limit, the cross sections for Higgsino-like particles scattering on nucleons is severely suppressed by an amplitude level cancellation, making it important to assess the impact of formally subleading effects. The power correction of order $m_W/M$ to the heavy WIMP limit is computed for general electroweak doublet dark matter candidates, and a model of nuclear modifications...

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  48. 6. Two-zone models for the multi-messenger emission from the blazar TXS 0506+056
    Dr Ruoyu Liu (NJU)

    A high-energy muon neutrino event, IceCube-170922A, was recently discovered in both spatial and temporal coincidence with a gamma-ray flare of the blazar TXS 0506+056. We propose the multi-messenger emission of the blazar flare can be well explained in two-zone models, with an inner blob inside of or close to the broad-line region (BLR) and an outer one well beyond the BLR. We compare our...

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