On ionization energy losses of relativistic particles created in matter

2000 ◽  
Vol 164-165 ◽  
pp. 180-185 ◽  
Author(s):  
N.F. Shul'ga ◽  
V.V. Syshchenko
Keyword(s):  
Ionization Energy ◽  
Energy Losses ◽  
Relativistic Particles

A method for the direct measurement of small energy losses of relativistic particles

1965 ◽  
Vol 86 (3) ◽  
pp. 674-676
Author(s):  
D K Aitken ◽  
R E Jennings ◽  
R N F Walker
Keyword(s):  
Direct Measurement ◽  
Energy Losses ◽  
Small Energy ◽  
Relativistic Particles

The energy spectrum of the component of the cosmic radiation

1968 ◽  
Vol 46 (10) ◽  
pp. S578-S582 ◽  
Author(s):  
P. S. Freier ◽  
C. J. Waddington
Keyword(s):  
Energy Spectrum ◽  
Ionization Energy ◽  
Cosmic Radiation ◽  
Integral Intensity ◽  
Cosmic Ray ◽  
Energy Losses ◽  
Ionization Energy Loss ◽  
Maximum Value ◽  
Source Spectra ◽  
Acceleration Term

Three large stacks of nuclear emulsions were exposed during 1964–66 on high-altitude balloons launched from Fort Churchill, Canada; Texas, U.S.A.; and Hyderabad, India. These stacks have been used to study the energy spectrum of the cosmic-ray nuclei of calcium and heavier (the so-called VH nuclei). These measurements result in integral intensity values for energies greater than 7.1, 1.58, and 1.00 GeV per nucleon, together with differential intensities over the range [Formula: see text] MeV per nucleon. Differential intensities were also found for lighter nuclei over varying energy ranges. The differential spectrum observed has a maximum value of about 1.6 × 10−3 nuclei/m2 sr s MeV per nucleon around [Formula: see text] MeV per nucleon and falls off at both higher and lower energies. These values are based on the observation of a total of some 1 600 VH nuclei. The energy spectrum has been compared with that observed at similar times for the helium nuclei in order to study the influences of ionization energy losses during propagation of these high-Z nuclei. These observations are interpreted as implying that if the source spectra of the VH nuclei and the helium nuclei are similar, then the VH nuclei have traversed less than 1 g/cm2 of matter while ionization energy loss has been the dominant acceleration term.

Ionization energy losses of relativistic positrons passing through a silicon single crystal and electron emission

1983 ◽  
Vol 71 (3-4) ◽  
pp. 185-189
Author(s):  
D. I. Adejshvili ◽  
G. L. Bochek ◽  
V. I. Vit'Ko ◽  
V. G. Gorbenko ◽  
I. A. Grishaev ◽  
...  
Keyword(s):  
Single Crystal ◽  
Electron Emission ◽  
Ionization Energy ◽  
Silicon Single Crystal ◽  
Energy Losses

Ionization Energy Losses of RelativisticμMesons in Gases

1953 ◽  
Vol 91 (5) ◽  
pp. 1186-1191 ◽  
Author(s):  
J. E. Kupperian ◽  
E. D. Palmatier
Keyword(s):  
Ionization Energy ◽  
Energy Losses

Ionization energy losses and ranges of alpha particles in ionic crystals

1976 ◽  
Vol 40 (4) ◽  
pp. 418-420
Author(s):  
G. N. Potetyunko ◽  
E. T. Shipatov
Keyword(s):  
Ionization Energy ◽  
Alpha Particles ◽  
Energy Losses ◽  
Ionic Crystals

Influence of the ionization-energy losses of high-energy bismuth ions on the development of helium blisters in silicon

2015 ◽  
Vol 49 (10) ◽  
pp. 1290-1293
Author(s):  
V. F. Reutov ◽  
S. N. Dmitriev ◽  
A. S. Sohatsky ◽  
A. G. Zaluzhnyi
Keyword(s):  
Ionization Energy ◽  
High Energy ◽  
Energy Losses

scholarly journals The quirk signal at FASER and FASER 2

2021 ◽  
Vol 2021 (12) ◽  
Author(s):  
Jinmian Li ◽  
Junle Pei ◽  
Long jie Ran ◽  
Wenxing Zhang
Keyword(s):  
Ionization Energy ◽  
Energy Losses ◽  
Interaction Point ◽  
Quantum Numbers ◽  
Integrated Luminosity

Abstract We study FASER and FASER 2 sensitivities to the quirk signal by simulating the motions of quirks that are travelling through several infrastructures from the ATLAS interaction point to the FASER (2) detector. The ionization energy losses for a charged quirk travelling in different materials are treated carefully. We calculate the expected numbers of quirk events that can reach the FASER (2) detector for an integrated luminosity of 150 (3000) fb−1. Scenarios for quirks with four different quantum numbers, and different masses and confinement scales are studied.

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