AbstractExperimental results for the radiative energy loss of 206 and 234 GeV electrons in 5–10 μm thin Ta targets are presented. An increase in radiation emission probability at low photon energies compared to a 100 μm thick target is observed. This increase is due to the formation length of the GeV photons exceeding the thickness of the thin foils, the so-called Ternovskii–Shul'ga–Fomin (TSF) effect. The formation length of GeV photons from a multi-hundred GeV projectile is through the TSF effect shown directly to be a factor 1010 longer than their wavelength
The scope of this paper is to discuss two important questions relevant for TeV γ-ray astronomy; the ...
The scope of this paper is to discuss two important questions relevant for TeV γ-ray astronomy; the ...
Bright sources of high energy electromagnetic radiation are widely employed in fundamental research ...
AbstractExperimental results for the radiative energy loss of 206 and 234 GeV electrons in 5–10 μm t...
Experimental results for the radiative energy loss of 206 and 234 GeV electrons in 5–10 μm thin Ta t...
We report the first observation of a shoulder in the radiation spectrum from GeV electrons in a stru...
Experimental results for the radiative energy loss of 178 GeV positrons in Cu, Au, and W targets are...
AbstractWhen an ultrarelativistic electron traverses two closely spaced foils, a radiation spectrum ...
The process of emission of electromagnetic radiation does not occur instantaneously, but is “formed”...
The formation region effects in x-ray transition radiation have been experimentally investigated. Th...
Electromagnetic energy injected into the universe above a few hundred TeV is expected to pile up as ...
Electromagnetic energy injected into the universe above a few hundred TeV is expected to pile up as ...
The idea that the TeV air showers, thought to be produced by >10 TeV gamma rays from Mrk 501, can be...
The radiative return offers the unique possibility for a measurement of the cross section of electro...
The recent detection of gamma radiation from Mkn 501 at energies as high as 25 TeV suggests stringen...
The scope of this paper is to discuss two important questions relevant for TeV γ-ray astronomy; the ...
The scope of this paper is to discuss two important questions relevant for TeV γ-ray astronomy; the ...
Bright sources of high energy electromagnetic radiation are widely employed in fundamental research ...
AbstractExperimental results for the radiative energy loss of 206 and 234 GeV electrons in 5–10 μm t...
Experimental results for the radiative energy loss of 206 and 234 GeV electrons in 5–10 μm thin Ta t...
We report the first observation of a shoulder in the radiation spectrum from GeV electrons in a stru...
Experimental results for the radiative energy loss of 178 GeV positrons in Cu, Au, and W targets are...
AbstractWhen an ultrarelativistic electron traverses two closely spaced foils, a radiation spectrum ...
The process of emission of electromagnetic radiation does not occur instantaneously, but is “formed”...
The formation region effects in x-ray transition radiation have been experimentally investigated. Th...
Electromagnetic energy injected into the universe above a few hundred TeV is expected to pile up as ...
Electromagnetic energy injected into the universe above a few hundred TeV is expected to pile up as ...
The idea that the TeV air showers, thought to be produced by >10 TeV gamma rays from Mrk 501, can be...
The radiative return offers the unique possibility for a measurement of the cross section of electro...
The recent detection of gamma radiation from Mkn 501 at energies as high as 25 TeV suggests stringen...
The scope of this paper is to discuss two important questions relevant for TeV γ-ray astronomy; the ...
The scope of this paper is to discuss two important questions relevant for TeV γ-ray astronomy; the ...
Bright sources of high energy electromagnetic radiation are widely employed in fundamental research ...