Zobrazeno 1 - 10
of 25
pro vyhledávání: '"Rasmus S. L. Hansen"'
Publikováno v:
Hansen, R S L, Shalgar, S M & Tamborra, I 2022, ' Enhancement or damping of fast neutrino flavor conversions due to collisions ', Physical Review D, vol. 105, no. 12, 123003 . https://doi.org/10.1103/PhysRevD.105.123003
Fast neutrino flavor conversion can occur in core-collapse supernovae or compact binary merger remnants when non-forward collisions are also at play, and neutrinos are not fully decoupled from matter. This work aims to shed light on the conditions un
Publikováno v:
Dansk Universitetspædagogisk Tidsskrift. 15:70-86
Denne undersøgelse belyser de udfordringer, som studerende oplever i overgangen til universitetet. Undersøgelsen bygger på en empirinær kodning af 557 Arts-studerendes besvarelser på spørgsmål om udfordringer i overgangen til universitetet og
Publikováno v:
Phys.Rev.D
Phys.Rev.D, 2022, 105 (2), pp.023011. ⟨10.1103/PhysRevD.105.023011⟩
Sarfati, L, Hansen, R S L & Tamborra, I 2022, ' Triangulating black hole forming stellar collapses through neutrinos ', Physical Review D, vol. 105, no. 02, 023011 . https://doi.org/10.1103/PhysRevD.105.023011
Physical Review D
Phys.Rev.D, 2022, 105 (2), pp.023011. ⟨10.1103/PhysRevD.105.023011⟩
Sarfati, L, Hansen, R S L & Tamborra, I 2022, ' Triangulating black hole forming stellar collapses through neutrinos ', Physical Review D, vol. 105, no. 02, 023011 . https://doi.org/10.1103/PhysRevD.105.023011
Physical Review D
In the event of a black hole (BH) forming stellar collapse, the neutrino signal should terminate abruptly at the moment of BH formation, after a phase of steady accretion. Since neutrinos are expected to reach Earth hours before the electromagnetic s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ad165ddd82921db30c7e1878ffa5e7b1
https://hal.archives-ouvertes.fr/hal-03380571
https://hal.archives-ouvertes.fr/hal-03380571
Autor:
Rasmus S. L. Hansen
Parallel Contributed Talk at the "XIX International Workshop on Neutrino Telescopes" on line - 18-26 February, 2021
in collaboration with Shashank Shalgar and Irene Tamborra based on 2012.03948 Co-financed by the Connecting Europe Facility of th
in collaboration with Shashank Shalgar and Irene Tamborra based on 2012.03948 Co-financed by the Connecting Europe Facility of th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2cd3bbfe9aef3a8d4ed27e54d4b31f38
Publikováno v:
Hansen, R S L, Lindner, M & Scholer, O 2020, ' Timing the neutrino signal of a Galactic supernova ', Physical Review D, vol. 101, no. 12, 123018 . https://doi.org/10.1103/PhysRevD.101.123018
Physical Review
Physical Review
We study several methods for timing the neutrino signal of a Galactic supernova (SN) for different detectors via Monte Carlo simulations. We find that, for the methods we studied, at a distance of $10\,$kpc both Hyper-Kamiokande and IceCube can reach
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a0c011c1a3647229c2b9190377394bfb
https://pure.au.dk/ws/files/223683887/PhysRevD.101.123018.pdf
https://pure.au.dk/ws/files/223683887/PhysRevD.101.123018.pdf
Autor:
Kazunori Kohri, Thomas Tram, Rasmus S. L. Hansen, Steen Hannestad, Takuya Hasegawa, Nagisa Hiroshima
Publikováno v:
Hasegawa, T, Hiroshima, N, Kohri, K, Hansen, R S L, Tram, T & Hannestad, S 2020, ' MeV-scale reheating temperature and cosmological production of light sterile neutrinos ', Journal of Cosmology and Astroparticle Physics, vol. 2020, no. 8, 015 . https://doi.org/10.1088/1475-7516/2020/08/015
We investigate how sterile neutrinos with a range of masses influence cosmology in MeV-scale reheating temperature scenarios. By computing the production of sterile neutrinos through the combination of mixing and scattering in the early Universe, we
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d48ca542e9000114e75862183327edd5
http://arxiv.org/abs/2003.13302
http://arxiv.org/abs/2003.13302
Autor:
Kazunori Kohri, Thomas Tram, Steen Hannestad, Rasmus S. L. Hansen, Nagisa Hiroshima, Takuya Hasegawa
Publikováno v:
Hasegawa, T, Hiroshima, N, Kohri, K, Hansen, R S L, Tram, T & Hannestad, S 2019, ' MeV-scale reheating temperature and thermalization of oscillating neutrinos by radiative and hadronic decays of massive particles ', Journal of Cosmology and Astroparticle Physics, vol. 2019, no. 12, 012, pp. 012 . https://doi.org/10.1088/1475-7516/2019/12/012
From a theoretical point of view, there is a strong motivation to consider an MeV-scale reheating temperature induced by long-lived massive particles with masses around the weak scale, decaying only through gravitational interaction. In this study, w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9080039e7ab67247415adb67c3fe2057
http://arxiv.org/abs/1908.10189
http://arxiv.org/abs/1908.10189
Autor:
Rasmus S. L. Hansen
Publikováno v:
Proceedings of Neutrino Oscillation Workshop — PoS(NOW2018).
The neutrino flavour evolution in a supernova can be described either in terms of neutrino fields or as the evolution of individual neutrinos. There is no reason to think that the two approaches should give contradicting results, and both have their
Publikováno v:
Hansen, R S L & Smirnov, A Y 2019, ' Effect of extended ν production region on collective oscillations in supernovae ', Journal of Cosmology and Astroparticle Physics, vol. 2019, no. 10, 027 . https://doi.org/10.1088/1475-7516/2019/10/027
Journal of Cosmology and Astroparticle Physics
Journal of Cosmology and Astroparticle Physics
In supernovae neutrinos are emitted from a region with a width $r_{\rm eff}$ of a few kilometers (rather than from a surface of infinitesimal width). We study the effect of integration (averaging) over such an extended emission region on collective o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7861378729260f7b0cb75efcc7be0c29
Autor:
Rasmus S. L. Hansen, Vedran Brdar
Motivated by the discovery of the first high-energy astrophysical neutrino source, the blazar TXS 0506+056, we revisit the IceCube flavor ratio analysis. Assuming large statistics from identified blazars, collected in the forthcoming years by the Ice
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6a866a6ac06b4ac36c0b064950f60ffd
http://arxiv.org/abs/1812.05541
http://arxiv.org/abs/1812.05541