THE MEASUREMENT OF EXTRA HARD X-RAYS AND GAMMA RAYS IN ROENTGENS

1937 ◽  
Vol 15a (5) ◽  
pp. 67-78 ◽  
Author(s):  
G. C. Laurence

The intensity in roentgens per second of X-rays or γ-rays harder than 0.03 Å may be measured with a small thimble chamber with homogeneous walls of elements below atomic number 13 and thick enough to be impermeable to the fastest secondary β-rays. The ionization current measured under saturation conditions at standard temperature and pressure is divided by BV, and correction is made for the apparent absorption of the X-rays m the walls. V is the volume of the chamber and B is given by[Formula: see text]A table (Table IV) of the values of 2 loge (Zw/Za) for different wall materials is given, and J, K, and L are plotted (Fig. 2) as functions of the quality of the radiation.The absolute intensity of radiation in quanta per square centimetre per second may be obtained from[Formula: see text]in which c is the ionization current per unit volume in the chamber, at standard temperature and pressure, produced by one quantum per square centimetre per second.The intensity of the radiation from one milligram of radium in equilibrium, and covered by platinum of wall thickness t, at one centimetre distance is (8.98 − 1.17 mm.−1 × t) roentgens per hour approximately, it t is not less than 0.3 mm.

Parasitology ◽  
1966 ◽  
Vol 56 (4) ◽  
pp. 651-656 ◽  
Author(s):  
T. Kassai ◽  
B. Fitzpatrick ◽  
W. Mulligan

A comparison has been made of the attenuating effect on N. brasiliensis larvae of X-rays (HVL, 8 mm Al) and γ-rays from 60Co over the range 10–80 kr. In the dose range where attenuation was manifested as a decrease in total worm burden the γ-rays had an RBE (relative biological effect) of 0-7 relative to the X-rays as unity.Because of the enhancement of infectivity occurring at low radiation doses, attenuation in this region is better assessed in terms of alteration to the sex-ratio of the parasite rather than effect on total population.This work was supported by grants from the Agricultural Research Council and the Horse Race Betting Levy Board, and was carried out during the tenure by one of the authors (T. Kassai) of a British Council exchange scholarship.Thanks are due to Dr T. Martin Young and Mr J. S. Orr of the Radiotherapy Department, Western Infirmary, Glasgow, for access to radiation sources and helpful advice.


2011 ◽  
Vol 7 (S279) ◽  
pp. 274-281 ◽  
Author(s):  
Boaz Katz ◽  
Nir Sapir ◽  
Eli Waxman

AbstractSome of the observed bursts of X-rays/Gamma-rays associated with supernovae (SNe) as well as very luminous SNe may result from the breakout of the SN shock from an optically thick wind surrounding the progenitor. We show that in such scenarios a collisionless shock necessarily forms during the shock breakout. An intense non-thermal flash of ≲1 MeV gamma rays, hard X-rays and multi-TeV neutrinos is produced simultaneously with and following the typical soft X-ray breakout emission, carrying similar or larger energy than the soft emission. The non-thermal flash is detectable by current X-ray telescopes and may be detectable out to 10's of Mpc by km-scale neutrino telescopes.


2021 ◽  
pp. 219-222
Author(s):  
Rubina Rubina ◽  
Baig M.Q ◽  
Kumar Dev

Many years after the discovery of X-ray's and gamma rays. They have been used empirically in medicine, later on realized that this approach was dangerous mainly in radiotherapy and up to some extent in diagnostic radiology. Thus Means of measuring x-ray/γ-rays had to be found in terms of unit of x-rays quantity dened and accepted. The magnitude of the biological effect desirable in case therapy and undesirable in case of diagnosis. It depends upon how much radiation energy is absorbed by irradiated material. X-ray dosimetry is the measurement of energy absorbed in any material particularly in different tissues of the body.


1953 ◽  
Vol 31 (12) ◽  
pp. 1164-1172 ◽  
Author(s):  
G. R. Freeman ◽  
A. B. Van Cleave ◽  
J. W. T. Spinks

The production of acid by irradiation of 1 M chloral hydrate solutions is proportional to the dose at a given dose rate. The specific yield is the same for Co60 γ-rays as for 23 Mev. peak energy X rays and is a linear function of the inverse of the square root of the close rate. The reaction is apparently a chain reaction.


1994 ◽  
Vol 159 ◽  
pp. 379-379
Author(s):  
Andrzej Maciołek-Niedźwiecki ◽  
Andrzej A. Zdziarski ◽  
Alan P. Lightman

We show that the recent observations of the Seyfert galaxy NGC 4151 in hard X-rays and soft γ-rays by the OSSE and SIGMA detectors onboard CGRO and GRANAT, respectively, are well explained by a nonthermal model with acceleration of relativistic electrons at an efficiency of ≲50% and with the remaining power dissipated thermally in the source (the standard nonthermal e± pair model assumed 100% efficiency). Such an acceleration efficiency is generally expected on physical grounds. The resulting model unifies previously proposed purely thermal and purely nonthermal models. The pure nonthermal model for NGC 4151 appears to be ruled out. The pure thermal model gives a worse fit to the data than our hybrid nonthermal/thermal model. Our results are presented in Zdziarski, Lightman, & Maciołek-Niedźwiecki (1993).


2010 ◽  
Vol 6 (S275) ◽  
pp. 305-306
Author(s):  
Włodek Bednarek

AbstractDense wind of a massive star can be partially captured by a companion neutron star (NS) creating a very turbulent and magnetized transition region at some distance from the NS surface. We consider the consequences of electron and hadron acceleration at such a transition region. Electrons lose energy on the synchrotron process and the inverse Compton (IC) scattering of thermal radiation from the NS surface and/or the massive star. We calculate the synchrotron spectra (from X-rays to soft γ-rays) and IC spectra in the case of sources accreting the matter under the accretor and propeller scenarios. It is argued that a population of accreting massive binaries, recently discovered by the INTEGRAL observatory, can be detectable by the Fermi LAT telescope. On the other hand, TeV γ-ray emission from other class of massive binaries can be interpreted in terms of a magnetar accreting matter in the propeller scenario. We also calculate the expected neutrino event rates in a km2 detector produced by relativistic hadrons accelerated in such scenario.


Author(s):  
L. H. Gray

No satisfactory formula has so far been derived theoretically for the photoelectric absorption of X-rays and γ-rays. The empirical lawhas hitherto been generally accepted as giving approximately the variation of the photoelectric absorption coefficient per electron, with atomic numberZand wave length λ for X-rays of wave length greater than 100 X.U., and the validity of this law has often been assumed for γ-rays also.


1998 ◽  
Vol 492 (1) ◽  
pp. 228-245 ◽  
Author(s):  
P. Hoflich ◽  
J. C. Wheeler ◽  
A. Khokhlov

1999 ◽  
Vol 511 (1) ◽  
pp. 204-207 ◽  
Author(s):  
Vincent Tatischeff ◽  
Reuven Ramaty
Keyword(s):  

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