4–14 Jul 2022
Europe/Paris timezone

Session

Morning session

4 Jul 2022, 09:00

Conveners

Morning session: Dark Matter Galactic Center

  • Carlo Luciano Bianco (ICRANet)

Morning session: Dark Matter Galactic Center

  • Aldo Treves (Università Insubria)

Morning session: Dark Matter Galactic Center

  • Piero Rosati

Morning session: AGNs

  • Gregory Vereshchagin (ICRANet)

Morning session: Fronteer

  • She-Sheng Xue (ICRANet, Physics Department, Sapienza University of Rome)

Morning session: Cocoon and BdHN model

  • Yerlan Aimuratov (Fesenkov Astrophysical Institute / al-Farabi Kazakh National University)

Morning session: Cocoon and BdHN Model

  • Liang Li (ICRANet, Piazza della Repubblica 10, I-65122 Pescara, Italy)

Morning session: Supernovae

  • Maria Dainotti (National Astronomical Observatory of Japan)

Morning session: GRB 171205A and GRB 220101

  • Carlos Raúl Argüelles (Universidad Nacional de La Plata)

Presentation materials

There are no materials yet.

  1. Carlo Luciano Bianco (ICRANet)
    04/07/2022, 09:00
  2. Alessandro Spagna
    04/07/2022, 09:45

    The Galactic stellar populations can be used to test the predictions made by the Cold Dark Matter (CDM) model and compared with the observations at high redshift. Thanks to the modern astrometric, photometric and spectroscopic stellar surveys we can identify the «building blocks» of the Milky Way. Studies based on the Gaia DR’s and ground based spectroscopic surveys have already identified a...

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  3. Re Fiorentin Paola
    04/07/2022, 10:07

    The Galactic stellar populations can be used to test the predictions made by the Cold Dark Matter (CDM) model and compared with the observations at high redshift. Thanks to the modern astrometric, photometric and spectroscopic stellar surveys we can identify the «building blocks» of the Milky Way. Studies based on the Gaia DR’s and ground based spectroscopic surveys have already identified a...

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  4. Florian Peissker
    04/07/2022, 10:30
  5. Prof. Matteo Viel
    04/07/2022, 11:30

    I will review the use of the Intergalactic Medium as a probe of fundamental physics.

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  6. Federico Re
    05/07/2022, 09:00

    The inconclusive results in the search for a dark matter particle have led many to investigate primordial black holes as a possible alternative candidate. In my talk I will first review the basic theory of primordial black holes,
    their potential role in the dark matter problem, and the observational constraints already in place in this regard. In the second part of my talk I will explore...

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  7. Stefano Bondani (University of Insubria)
    05/07/2022, 09:45
  8. Felix Mirabel (IAFE-Argentina)
    05/07/2022, 10:30
  9. Carlos Raúl Argüelles (La Plata National University & ICRANet)
    05/07/2022, 11:30
  10. Daniele Gregoris (danielegregoris@libero.it)
    06/07/2022, 09:00

    Pioneered with the Christodoulou-Ruffini irreducible mass and subsequently reformulated with the Hawking-Bekenstein entropy, it can be shown that the area of the horizon of a black hole cannot decrease. Partly motivated by the arrow of time problem in cosmology and the Weyl curvature hypothesis, previous works in the literature have proposed - among other possibilities - the square of the...

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  11. Carlos Raúl Argüelles (Universidad Nacional de La Plata)
    06/07/2022, 09:45
  12. Carlos Raúl Argüelles (La Plata National University & ICRANet), Carlos Raúl Argüelles (Universidad Nacional de La Plata)
    06/07/2022, 10:30
  13. Piero Rosati
    06/07/2022, 11:30

    I will show how high-precision strong lensing models of galaxy clusters based on high-quality HST imaging and spectroscopic VLT data can constrain the inner dark matter mass distribution of clusters and compared with cosmological simulations. The same lens models enable competitive time-delay cosmography and the study of high-redshift magnified star-forming galaxies.

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  14. Martin Mestre
    06/07/2022, 12:15
  15. Kuantay Boshkayev (Kazakh National University)
    07/07/2022, 09:00
  16. She-Sheng Xue (ICRANet, Physics Department, Sapienza University of Rome)
    07/07/2022, 09:45

    The recent high-precision measurement of the $W$ mass by the CDF collaboration is in $7.0~\sigma$ tension with the Standard Model (SM) expectation. This tension can be relieved if the $W$ boson possesses a non-trivial right-handed gauge coupling at high energies. Such a right-handed gauge coupling induces by the SM gauge symmetric four-fermion interactions at TeV scales, where SM fermions...

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  17. Narek Sahakyan (ICRANet-Armenia)
    07/07/2022, 10:30
  18. Razmik Mirzoyan (Max-Planck-Institute for Physics)
    07/07/2022, 11:30
  19. Costantino Sigismondi (ICRA Sapienza and ICRANET Pescara)
    07/07/2022, 12:15

    The measurement of the sunrise azimuth on the sea horizon of Pescara is made in the season 1-march to 4-july (and more) by using a fixed reference point in the foreground, and the coordinates y to the horizon level and x towards left (+) or right (-). The parabola obtained in this way will be analyzed with modern tools now available in many spreadsheets softwares. The comparison with the...

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  20. Di Li (National Astronomical Observatories, China)
    08/07/2022, 09:00
  21. Lang Xie
    08/07/2022, 09:45
  22. Zhi-Peng Jin
    08/07/2022, 10:10
  23. Wentao Luo (USTC)
    08/07/2022, 10:30
  24. Mimoza Hafizi (University of Tirana)
    08/07/2022, 11:30
  25. Francesco Longo (University of Trieste and INFN, Trieste)
    08/07/2022, 12:15

    The lecture will review the path that led to the observation of GRBs at High and Very High Energies.

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  26. Maria Dainotti (National Astronomical Observatory of Japan)
    11/07/2022, 09:00
  27. Lorenzo Amati (INAF - OAS Bologna)
    11/07/2022, 09:45
  28. Ehud Nakar
    11/07/2022, 10:30

    During my classes I will describe the main physical processes that govern the propagation of a relativistic jet in dense media and the cocoon that develops during this propagation. Then I will discuss the emission that is released during the shock breakout from the surface of the media and the following cocoon expansion.

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  29. Gregory Vereshchagin (ICRANet)
    11/07/2022, 11:30
  30. Dafne Guetta
    11/07/2022, 12:15
  31. Ehud Nakar
    12/07/2022, 09:00

    During my classes I will describe the main physical processes that govern the propagation of a relativistic jet in dense media and the cocoon that develops during this propagation. Then I will discuss the emission that is released during the shock breakout from the surface of the media and the following cocoon expansion.

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  32. Tsvi Piran (The Hebrew University)
    12/07/2022, 09:45
  33. Mariateresa Crosta (INAF-OATo)
    12/07/2022, 10:30
  34. Petr Kotlarik
    12/07/2022, 11:30
  35. Astesiano Davide
    12/07/2022, 12:15

    I will review exact solutions to Einstein’s field equations coupled to dust and discuss their application to galaxies’ dynamic.

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  36. Massimo Della Valle
    13/07/2022, 09:00
  37. Rahim Moradi (ICRANet and ICRA-Sapienza)
    13/07/2022, 09:45
  38. Luca Izzo (University of Copenhagen)
    13/07/2022, 10:30
  39. Eli Wazman
    13/07/2022, 11:30

    ULTRASAT is a scientific satellite, that is planned to be launched to a geo-stationary orbit in Q2/Q3 2025. It will carry a telescope with an unprecedentedly large field of view (200 squared degrees) and UV (230-290nm) sensitivity. These unique properties will enable us to detect and systematically study transient astronomical events within an extra-Galactic volume, that is hundreds of time...

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  40. Yerlan Aimuratov (Fesenkov Astrophysical Institute / al-Farabi Kazakh National University)
    13/07/2022, 12:15
  41. Jorge Armando Rueda Hernandez (ICRANet)
    14/07/2022, 09:00
  42. Liang Li (ICRANet, Piazza della Repubblica 10, I-65122 Pescara, Italy)
    14/07/2022, 09:45
  43. Yu Wang (ICRANet, INAF)
    14/07/2022, 10:30
  44. 14/07/2022, 11:30
  45. Matteo Luca Ruggiero
  46. Da-Ming Wei
  47. Prof. Stefano Ansoldi (University of Udine)
Building timetable...