Measurement of energy of medium-mass and heavy cosmic-ray nuclei by a specific energy deposition at the maximum of hadron showers in dense matter

2003 ◽  
Vol 66 (1) ◽  
pp. 130-134 ◽  
Author(s):  
I. D. Rapoport ◽  
A. N. Turundaevsky ◽  
V. Ya. Shestoperov
Atomic Energy ◽  
2004 ◽  
Vol 96 (4) ◽  
pp. 275-281 ◽  
Author(s):  
V. V. Vatulin ◽  
A. V. Kunin ◽  
A. A. Golubev ◽  
V. E. Luk'yashin ◽  
V. I. Turtikov ◽  
...  

2008 ◽  
Vol 396-398 ◽  
pp. 721-724 ◽  
Author(s):  
B.M. Mendes ◽  
T.P.R. Campos

Neutron brachytherapy show better results than conventional photon therapy for radioresistant tumors with hypoxic regions. Herein a comparative radiodosimetric analysis is presented considering 125I photon emitter seeds, often applied to brachytherapy, and a proposed Sol-Gel glass, synthesized with incorporated 252Cf neutron emitter, on a brain tumor implant. The proposition is to verify the viability of applying this bioceramic material. The methodology is based on the investigation of the specific energy deposition (dose) from 252Cf-Glass in deep brain interstitial implants through a stochastic computer code (MCNP5) and comparison with 125I seed’s energy deposition. 252Cf-Glass show dose per transition values higher than 125I seed’s set. RBE-isodose curves show a faster decrease of dose with the source distance increasing which can improve healthy tissue sparing.


2019 ◽  
Vol 59 (1) ◽  
pp. 29-62 ◽  
Author(s):  
Werner Hofmann ◽  
Wei Bo Li ◽  
Werner Friedland ◽  
Brian W. Miller ◽  
Balázs Madas ◽  
...  

AbstractAt the tissue level, energy deposition in cells is determined by the microdistribution of alpha-emitting radionuclides in relation to sensitive target cells. Furthermore, the highly localized energy deposition of alpha particle tracks and the limited range of alpha particles in tissue produce a highly inhomogeneous energy deposition in traversed cell nuclei. Thus, energy deposition in cell nuclei in a given tissue is characterized by the probability of alpha particle hits and, in the case of a hit, by the energy deposited there. In classical microdosimetry, the randomness of energy deposition in cellular sites is described by a stochastic quantity, the specific energy, which approximates the macroscopic dose for a sufficiently large number of energy deposition events. Typical examples of the alpha-emitting radionuclides in internal microdosimetry are radon progeny and plutonium in the lungs, plutonium and americium in bones, and radium in targeted radionuclide therapy. Several microdosimetric approaches have been proposed to relate specific energy distributions to radiobiological effects, such as hit-related concepts, LET and track length-based models, effect-specific interpretations of specific energy distributions, such as the dual radiation action theory or the hit-size effectiveness function, and finally track structure models. Since microdosimetry characterizes only the initial step of energy deposition, microdosimetric concepts are most successful in exposure situations where biological effects are dominated by energy deposition, but not by subsequently operating biological mechanisms. Indeed, the simulation of the combined action of physical and biological factors may eventually require the application of track structure models at the nanometer scale.


2020 ◽  
Vol 29 (12) ◽  
pp. 125006
Author(s):  
Yifei Zhu ◽  
Svetlana M Starikovskaia ◽  
Natalia Yu Babaeva ◽  
Mark J Kushner

1997 ◽  
Vol 14 (2) ◽  
pp. 195-199 ◽  
Author(s):  
R. W. Clay ◽  
A. G. K. Smith ◽  
J. L. Reid

AbstractCosmic radiation is capable of depositing significant quantities of energy and momentum in gravitational wave antennas at times that will generally be random with respect to gravitational signals. Such cosmic ray effects may generate noise signals at detectable levels compared to antenna design thresholds at rates of a few per year but, since antennas will not be capable of absorbing all the cosmic ray energy, it should be readily possible to construct vetoing cosmic ray detectors. For proposed interferometer antennas, a deposition of a few hundred GeV will produce a detectable noise signal and the veto will require about 100 MeV of energy deposition outside the antenna. We consider here some of the principles involved in the generation of gravitational antenna noise by cosmic ray particles and we describe a veto system to be installed at the Perth gravitational wave observatory.


2004 ◽  
Vol 42 (4) ◽  
pp. 331-337
Author(s):  
I. D. Rapoport ◽  
A. N. Turundaevskii ◽  
V. Ya. Shestoperov

2019 ◽  
Vol 17 ◽  
pp. 43
Author(s):  
I. Savvidis

A large volume (1m3) spherical proportional counter has been developed at CEA/Saclay, for low flux neutron measurements. The high voltage is applied to a small sphere 15mm in diameter, located in the center of the counter and the wall of the counter is grounded. Neutrons can be measured successfully, with high sensitivity, using 3He gas in the detector. The proton and tritium energy deposition in the drift gaseous volume, from the reaction 3He(n,p)3H, can provide the neutron spectra from thermal neutrons up to several MeV.The detector has been installed in the underground laboratory in Modane (LSM) to measure the neutron background. The sphere has been has been filled with gas mixture of Ar + 2% CH4 +3gr He-3, at 275 mbar. The thermal neutron peak is well separated from the cosmic ray and gamma background, permitting of neutron flux calculation. Other potential applications requiring large volume of about 10 m in radius are described in detail in reference


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