First observation of the Greisen-Zatsepin-Kuzmin suppression.

By R. Abbasi, T. Abu-Zayyad, M. Allen, J. Amman, G. Archbold, K. Belov, J. Belz, S. Zvi, D. Bergman, S. Blake and 50 more. Physical Review Letters, 2008

658 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/9d9985b0535ca5c73b1ae78603b9091a6d2e28e8

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. Kohta Murase
2. Angela V. Olinto
3. Kumiko Kotera
4. F. Oikonomou
5. Ralph Engel
6. S. Nagataki
7. P. Simakachorn
8. Y. Gouttenoire

In Nuclear and High Energy Physics

1. Kumiko Kotera
2. Angela V. Olinto
3. Kohta Murase
4. M. Unger
5. F. Oikonomou
6. Ralph Engel
7. S. Nagataki
8. K. Kampert

Citations in the corpus

• Beyond the Standard Models with cosmic strings (2019, background): “Therefore, CS have been pointed [258–261] as a possible candidate for the detection of ultra-high energy cosmic rays [262] above the Greisen-Zatsepin-Kuzmin (GZK) cut-off, around 10 eV [263–265], even though the expected flux at earth is generally too small to be detected [266–268].”
• INDICATIONS OF INTERMEDIATE-SCALE ANISOTROPY OF COSMIC RAYS WITH ENERGY GREATER THAN 57 EeV IN THE NORTHERN SKY MEASURED WITH THE SURFACE DETECTOR OF THE TELESCOPE ARRAY EXPERIMENT (2014, result): “The High Resolution Fly’s Eye (HiRes) collaboration was first to observe a suppression of cosmic rays above∼60 EeV (Abbasi et al. 2008), which is consistent with expectation from the GZK cutoff.”
• The Astrophysics of Ultrahigh-Energy Cosmic Rays (2011, background): “Due to different reconstruction methods, the HiRes measurement of fluctuations is not easily displayed in Figure 6, but their data trend remains closer to light primaries up to around 50 EeV.”