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The energy spectrum of cosmic rays at the highest energies

doi: 10.1051/epjconf/20135301005 , 10.7566/jpscp.19.011003 , 10.1051/epjconf/20135301008 , 10.48550/arxiv.1306.6138 , 10.48550/arxiv.1306.4430 , 10.48550/arxiv.1306.4998 , 10.1051/epjconf/20135300001
doi: 10.1051/epjconf/20135301005 , 10.7566/jpscp.19.011003 , 10.1051/epjconf/20135301008 , 10.48550/arxiv.1306.6138 , 10.48550/arxiv.1306.4430 , 10.48550/arxiv.1306.4998 , 10.1051/epjconf/20135300001
One of several working groups established for this workshop was charged with examining results and methods associated with the UHECR energy spectrum. We summarize the results of our discussions, which include a better understanding of the analysis choices made by groups and their motivation. We find that the energy spectra determined by the larger experiments are consistent in normalization and shape after energy scaling factors are applied. Those scaling factors are within systematic uncertainties in the energy scale, and we discuss future work aimed at reducing these systematics.
Working Group report given at UHECR 2012 Symposium, CERN, Feb. 2012
- Universidade Federal do Rio de Janeiro (UFRJ) Brazil
- University of Adelaide Australia
- Université Libre de Bruxelles Belgium
- University of Paris France
- Karlsruhe Institute of Technology Germany
[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], [SDU.ASTR.HE] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], [PHYS.HPHE] Physics/High Energy Physics - Phenomenology, [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph], QC1-999, UHE [cosmic radiation], energy spectrum, FOS: Physical sciences, [PHYS.ASTR.HE] Physics/Astrophysics/High Energy Astrophysical Phenomena, 530, [SDU.ASTR.HE] Sciences of the Universe/Astrophysics/High Energy Astrophysical Phenomena, Physics and Astronomy (all), cosmic radiation: UHE, info:eu-repo/classification/ddc/530, Instrumentation and Methods for Astrophysics (astro-ph.IM), Astrophysique, High Energy Astrophysical Phenomena (astro-ph.HE), ultra-high-energy cosmic rays, cosmic radiation: energy spectrum, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Physics, ddc:530, [ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Généralités, Auger, [PHYS.HPHE] Physics [physics]/High Energy Physics - Phenomenology [hep-ph], observatory, * Automatic Keywords *, [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph], [ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph], [ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], [PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph], Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, energy spectrum [cosmic radiation], [PHYS.ASTR.HE] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]
[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], [SDU.ASTR.HE] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], [PHYS.HPHE] Physics/High Energy Physics - Phenomenology, [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph], QC1-999, UHE [cosmic radiation], energy spectrum, FOS: Physical sciences, [PHYS.ASTR.HE] Physics/Astrophysics/High Energy Astrophysical Phenomena, 530, [SDU.ASTR.HE] Sciences of the Universe/Astrophysics/High Energy Astrophysical Phenomena, Physics and Astronomy (all), cosmic radiation: UHE, info:eu-repo/classification/ddc/530, Instrumentation and Methods for Astrophysics (astro-ph.IM), Astrophysique, High Energy Astrophysical Phenomena (astro-ph.HE), ultra-high-energy cosmic rays, cosmic radiation: energy spectrum, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Physics, ddc:530, [ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Généralités, Auger, [PHYS.HPHE] Physics [physics]/High Energy Physics - Phenomenology [hep-ph], observatory, * Automatic Keywords *, [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph], [ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph], [ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], [PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph], Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, energy spectrum [cosmic radiation], [PHYS.ASTR.HE] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]
citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).33 popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.Top 10% influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).Top 10% impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.Top 10%
