Межа Ваксмана — Бакала

Межа Ваксмана—Бакала — це обчислена верхня межа спостережуваного потоку нейтрино високих енергій на основі спостережуваного потоку космічних променів високих енергій. Оскільки найбільш високоенергійні нейтрино утворюються в тих самих взаємодіях, що й космічні промені, спостережувана швидкість створення останніх накладає обмеження на перші. Межа названа на честь Елі Ваксмана та Джона Бакала[1].

Література

  • Alemany, R.; Burrage, C.; et al. "(2019). Summary Report of Physics Beyond Colliders at CERN".[2]
    • Gives a sense of the colliders at CERN that can help with this data set
  • Bradascio, F.. (2019). "Search for high-energy neutrinos from AGN cores". Proceedings of Science. [3]
    • Another peer reviewed article, this source allows for further information into parts of AGN that is included in the initial article.
  • Kachelriess, M.. (2022). "Extragalactic cosmic rays". FOS: Physical Science [4]
    • A journal reviewed article describing extra-galactic cosmic rays
  • Kachelriess, M.; Semikoz, D.V. (2019). "Cosmic ray models". Progress in Particle and Nuclear Physics, 109, 103710. [5]
    • Peer reviewed journal that gives a broad understanding of cosmic ray models and different experiments
  • Kajita T. Atmospheric neutrinos and discovery of neutrino oscillations. Proc Jpn Acad Ser B Phys Biol Sci.[6]
    • Gives information about neutrinos - journal reviewed document
  • Kimura, S.. (2022). "Neutrinos from Gamma-ray Bursts". FOS: Physical Sciences.[7]
    • The peer reviewed journal article above works to give a further insight in to high energy neutrinos from GRB's, which is discussed in the original article by Bahcall and Waxman and gives a further insight into the paper
  • Letessier-Selvon, A. (2001). "Establishing the GZK cutoff with ultra high energy tau neutrinos". AIP Conference Proceedings.[8]
    • This is a peer reviewed source, and it works to add details about other factors and components necessary for our analysis
  • Piran, T. (1999). Gamma-ray bursts and the fireball model. Physics Reports, 314(6), 575–667.[9]
    • journal reviewed article that gives a brief insight into how the fireball method works.
  • Kronberg, P. (2003). "Intergalactic Magnetic Fields". Physics Today, 55 [10]
    • The journal reviewed article above gives more information on the intergalactic magnetic fields mentioned above in the paper
  • Waxman, E; Bahcall, J (1998). "High energy neutrinos from astrophysical sources: An upper bound". Physical Review D, 59(2). [1]
    • This paper is a peer reviewed paper made by the authors Waxman and Bachall and gives a good overview of the overall topic chosen

Посилання

  1. ↑ а б Waxman, Eli; Bahcall, John (1999). High energy neutrinos from astrophysical sources: An upper bound. Physical Review D (англ.). 59 (2): 023002. arXiv:hep-ph/9807282. Bibcode:1998PhRvD..59b3002W. doi:10.1103/PhysRevD.59.023002.
  2. ↑ Alemany, R. (2019). Summary Report of Physics Beyond Colliders at CERN. arXiv:1902.00260.
  3. ↑ Bradascio, Federica (2019). Search for high-energy neutrinos from AGN cores. 36th International Cosmic Ray Conference (ICRC2019). Т. 36. с. 845. arXiv:1908.05170. Bibcode:2019ICRC...36..845B.
  4. ↑ Kachelriess, M. (2022). Extragalactic cosmic rays. 37th International Cosmic Ray Conference. 12-23 July 2021. Berlin. с. 18. arXiv:2201.04535. Bibcode:2022icrc.confE..18K.
  5. ↑ Kachelrieß, M.; Semikoz, D.V. (November 2019). Cosmic ray models. Progress in Particle and Nuclear Physics (англ.). 109: 103710. arXiv:1904.08160. Bibcode:2019PrPNP.10903710K. doi:10.1016/j.ppnp.2019.07.002.
  6. ↑ Kajita, Takaaki (2010). Atmospheric neutrinos and discovery of neutrino oscillations. Proceedings of the Japan Academy, Series B. 86 (4): 303—321. Bibcode:2010PJAB...86..303K. doi:10.2183/pjab.86.303. PMC 3417797. PMID 20431258.
  7. ↑ Kimura, Shigeo S. (2022). Neutrinos from Gamma-ray Bursts. arXiv:2202.06480.
  8. ↑ Letessier-Selvon, A. (2001). Establishing the GZK cutoff with ultra high energy tau neutrinos. AIP Conference Proceedings (англ.). 566: 157—171. arXiv:astro-ph/0009444. Bibcode:2001AIPC..566..157L. doi:10.1063/1.1378629.
  9. ↑ Piran, Tsvi (1999). Gamma-Ray Bursts and the Fireball Model. Physics Reports. 314 (6): 575—667. arXiv:astro-ph/9810256. Bibcode:1999PhR...314..575P. doi:10.1016/S0370-1573(98)00127-6.
  10. ↑ Kronberg, Philipp P. (1 грудня 2002). Intergalactic Magnetic Fields. Physics Today. 55 (12): 40—46. Bibcode:2002PhT....55l..40K. doi:10.1063/1.1537911.