The high-energy spectrum of Cygnus X-1 revisited

1993 ◽  
Vol 411 ◽  
pp. L95 ◽  
Author(s):  
F. Haardt ◽  
C. Done ◽  
G. Matt ◽  
A. C. Fabian
Keyword(s):  
Energy Spectrum ◽  
High Energy

Energy spectrum and mass composition of high-energy cosmic rays

2003 ◽  
Vol 66 (7) ◽  
pp. 1145-1206 ◽  
Author(s):  
Andreas Haungs ◽  
Heinigerd Rebel ◽  
Markus Roth
Keyword(s):  
Energy Spectrum ◽  
Cosmic Rays ◽  
High Energy ◽  
Mass Composition ◽  
High Energy Cosmic Rays

ULTRA HIGH ENERGY COSMIC RAYS WITH THE PIERRE AUGER OBSERVATORY

2012 ◽  
Vol 18 ◽  
pp. 221-229
Author(s):  
◽  
J. R. T. DE MELLO NETO
Keyword(s):  
Energy Spectrum ◽  
Cosmic Rays ◽  
Cross Section ◽  
High Energy ◽  
Pierre Auger Observatory ◽  
Mass Composition ◽  
Ultra High Energy ◽  
High Energy Cosmic Rays ◽  
The Status ◽  
Shower Maximum

We present the status and the recent measurements from the Pierre Auger Observatory. The energy spectrum is described and its features discussed. We report searches for anisotropy of cosmic rays arrival directions in large scales and through correlation with catalogues of celestial objects. The measurement of the cross section proton-air is discussed. Finally, the mass composition is addressed with the measurements of the variation of the depth of shower maximum with energy and with the muon density at ground.

Probing by transport the single-particle energy spectrum up to high energy of one quantum dot with the ground state of an adjacent weakly coupled quantum dot

2007 ◽  
Vol 204 (2) ◽  
pp. 508-512 ◽  
Author(s):  
D. G. Austing ◽  
G. Yu ◽  
C. Payette ◽  
J. A. Gupta ◽  
M. Korkusinski ◽  
...  
Keyword(s):  
Energy Spectrum ◽  
Quantum Dot ◽  
Single Particle ◽  
Ground State ◽  
High Energy ◽  
Particle Energy ◽  
Single Particle Energy ◽  
Weakly Coupled

Energy spectrum optimization in high-energy flash X-ray radiography

2010 ◽  
Vol 22 (3) ◽  
pp. 655-658 ◽  
Author(s):  
陈楠 Chen Nan ◽  
戴文华 Dai Wenhua ◽  
王敏鸿 Wang Minhong ◽  
周智 Zhou Zhi ◽  
王利鸣 Wang Liming ◽  
...  
Keyword(s):  
Energy Spectrum ◽  
High Energy ◽  
X Ray ◽  
Spectrum Optimization

Analysis of the hadronic energy spectrum in high-energy cosmic-ray families detected by emulsion chambers

1993 ◽  
Author(s):  
J. Bellandi ◽  
C. G. S. Costa ◽  
R. J. M. Covolan ◽  
C. Dobrigkeit ◽  
M. M. Guzzo ◽  
...  
Keyword(s):  
Energy Spectrum ◽  
Cosmic Ray ◽  
High Energy ◽  
Hadronic Energy

Decays of the Three Top Contributors to the Reactor V¯e High-Energy Spectrum, 92Rb, 96gsY, and 142Cs, Studied with Total Absorption Spectroscopy

2017 ◽  
Author(s):  
B. C. Rasco ◽  
M. Wolińska-Cichocka ◽  
A. Fijałkowska ◽  
K. P. Rykaczewski ◽  
M. Karny ◽  
...  
Keyword(s):  
Energy Spectrum ◽  
Absorption Spectroscopy ◽  
High Energy ◽  
Total Absorption

scholarly journals The Pierre Auger Observatory: Review of Latest Results and Perspectives

Universe ◽  
2018 ◽  
Vol 4 (11) ◽  
pp. 128 ◽  
Author(s):  
Dariusz Góra ◽  
Keyword(s):  
Energy Spectrum ◽  
Cosmic Rays ◽  
Detection System ◽  
Cosmic Ray ◽  
High Energy ◽  
Pierre Auger Observatory ◽  
Mass Composition ◽  
Ultra High Energy ◽  
Energy Limitation ◽  
Arrival Directions

The Pierre Auger Observatory is the world’s largest operating detection system for the observation of ultra high energy cosmic rays (UHECRs), with energies above 10 17 eV. The detector allows detailed measurements of the energy spectrum, mass composition and arrival directions of primary cosmic rays in the energy range above 10 17 eV. The data collected at the Auger Observatory over the last decade show the suppression of the cosmic ray flux at energies above 4 × 10 19 eV. However, it is still unclear if this suppression is caused by the energy limitation of their sources or by the Greisen–Zatsepin–Kuzmin (GZK) cut-off. In such a case, UHECRs would interact with the microwave background (CMB), so that particles traveling long intergalactic distances could not have energies greater than 5 × 10 19 eV. The other puzzle is the origin of UHECRs. Some clues can be drawn from studying the distribution of their arrival directions. The recently observed dipole anisotropy has an orientation that indicates an extragalactic origin of UHECRs. The Auger surface detector array is also sensitive to showers due to ultra high energy neutrinos of all flavors and photons, and recent neutrino and photon limits provided by the Auger Observatory can constrain models of the cosmogenic neutrino production and exotic scenarios of the UHECRs origin, such as the decays of super heavy, non-standard-model particles. In this paper, the recent results on measurements of the energy spectrum, mass composition and arrival directions of cosmic rays, as well as future prospects are presented.

Cyclotron absorption in the high energy spectrum of Her X-1

1994 ◽  
Author(s):  
M. Kunz ◽  
R. Staubert ◽  
D. E. Gruber ◽  
W. Pietsch ◽  
J. Trümper ◽  
...  
Keyword(s):  
Energy Spectrum ◽  
High Energy ◽  
Cyclotron Absorption
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