26 August 2019 to 20 September 2019
Nordita, Stockholm
Europe/Stockholm timezone

Contribution List

58 out of 58 displayed
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  1. 26/08/2019, 10:00
  2. Dr Marek Lewicki
    26/08/2019, 10:15
    We derive efficiency factors for the production of gravitational waves through bubble collisions and plasma-related sources in strong phase transitions, and find the conditions under which the bubble collisions can contribute significantly to the signal. We illustrate our findings in two examples, the Standard Model with an extra $|H|^6$ interaction and a classically...
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  3. 26/08/2019, 13:00
  4. Alberto Roper Pol (University of Colorado. LASP)
    26/08/2019, 14:00
  5. 27/08/2019, 10:00
  6. 27/08/2019, 14:00
  7. 27/08/2019, 16:30
  8. Pierre Auclair (APC)
    28/08/2019, 10:00
  9. 28/08/2019, 13:30
    https://agenda.albanova.se/conferenceDisplay.py?confId=6809
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  10. Ramkishor Sharma (University of Delhi)
    28/08/2019, 15:30
  11. Dr Ville Vaskonen (Kings College, London)
    29/08/2019, 10:00
  12. 29/08/2019, 14:00
  13. Prof. Mairi Sakellariadou (King's College London)
    30/08/2019, 10:00
  14. Jing Liu (Institute of Theoretical Physics, Chinese Academy of Sciences)
    30/08/2019, 14:00
  15. Dr Oliver Gould (Helsinki University)
    02/09/2019, 10:00
  16. 02/09/2019, 16:30
  17. Dr Ryusuke Jinno (DESY)
    03/09/2019, 10:00
  18. Dr Stephan Huber (University of Sussex)
    03/09/2019, 14:00
  19. Dr Mark Hindmarsh (University of Sussex)
    04/09/2019, 10:00
  20. 04/09/2019, 16:30
  21. Dr Kari Rummukainen (University of Oulu)
    05/09/2019, 10:00
  22. Prof. Guenter Sigl (University of Hamburg)
    06/09/2019, 10:00
  23. Dr Igor Pikovski (University of Stockholm)
    06/09/2019, 15:30
  24. Prof. Igor Rogachevskii (Ben-Gurion University of the Negev)
    09/09/2019, 10:00
  25. Daniel Cutting (University of Sussex)
    10/09/2019, 10:00
  26. Chloe Gowling (University of Sussex)
    10/09/2019, 14:00
  27. Reuben Ares (University of Sussex)
    10/09/2019, 14:15
  28. Sayan Mandal (Carnegie Mellon University)
    10/09/2019, 14:30
  29. Alberto Roper Pol (University of Colorado. LASP)
    10/09/2019, 14:45
  30. Dr Antoine Petiteau (Laboratoire APC)
    11/09/2019, 10:00
  31. Sayan Mandal (Carnegie Mellon University)
    13/09/2019, 10:00
  32. 16/09/2019, 11:00
  33. Prof. Mairi Sakellariadou (King's College London)
    16/09/2019, 13:00
  34. Prof. Jun'ichi Yokoyama (RESCEU, University of Tokyo)
    16/09/2019, 13:45
  35. Emanuela Dimastrogiovanni (University of Sydney)
    16/09/2019, 15:00
  36. Prof. Karsten Jedamzik
    16/09/2019, 15:45
  37. 16/09/2019, 16:30
  38. Prof. Juan Garcia-Bellido
    17/09/2019, 10:00
  39. Matteo Fasiello (ICG Portsmouth)
    17/09/2019, 10:45
  40. Dr Eugene Lim (Kings College, London)
    17/09/2019, 15:00
  41. 17/09/2019, 15:45
  42. Dr Mark Hindmarsh (University of Sussex)
    18/09/2019, 10:00
  43. Prof. David Weir (University of Helsinki)
    18/09/2019, 10:45
  44. Tina Kahniashvili (Carnegie Mellon University (USA) & Ilia State University (Georgia))
    18/09/2019, 13:00
  45. Alberto Roper Pol (University of Colorado. LASP)
    18/09/2019, 13:45
  46. Axel Brandenburg (Nordita)
    18/09/2019, 15:00
  47. 18/09/2019, 15:45
  48. 18/09/2019, 17:00
  49. Dr Djuna Croon (TRIUMF)
    19/09/2019, 10:00
  50. Dr Yun Jiang (MPIK Heidelberg)
    19/09/2019, 10:45
  51. Deyan Mihaylov (Albert Einstein Institute, Potsdam)
    19/09/2019, 13:00
  52. Dr Gianmassimo Tasinato (University of Swansea)
    19/09/2019, 13:45
  53. Prof. Juan Garcia-Bellido (IFT, Autonoma de Madrid)
    19/09/2019, 15:00
    Twenty-three years ago, we predicted that massive primordial black holes (PBH) would form via the gravitational collapse of radiation and matter associated with high peaks in the spectrum of curvature fluctuations, and that they could constitute all of the dark matter (DM) today. In 2015, we predicted the clustering and broad mass distribution of PBH, which peaks at several Msun, and...
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  54. 20/09/2019, 10:00