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Unpulsed gamma rays from the Crab pulsar and nebulaCheung, Wai-man, 張惠民 January 1994 (has links)
published_or_final_version / Physics / Master / Master of Philosophy
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The two-gamma-ray method for determining density and moisture content of cut lumber a final project report submitted ... /Smith, J. Michael January 1964 (has links)
Thesis (M.S.)--University of Michigan, 1964.
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Investigation of SKYSHINE a Monte Carlo application /Olhoeft, Jack E. January 1958 (has links)
Thesis (M.S.)--University of Michigan, 1958.
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Gamma ray energy standards and resonance half-widthsBenedict, Donald Lee, January 1942 (has links)
Thesis (Ph. D.)--University of Wisconsin--Madison, 1942. / Typescript. Vita. eContent provider-neutral record in process. Description based on print version record. Includes bibliographical references.
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Gamma ray anisotropies in antiferromagnetic crystals of MnSiF₆.6H₂0 and CoC1₂.6H₂0Griffiths, David J. January 1960 (has links)
By the technique of adiabatic demagnetization, paramagnetic
salts may be cooled to temperatures less than .1°K. By good thermal contact between crystals and paramagnetic salts, the antiferromagnetics MnSiF₆.6H₂0 and CoC1₂.6H₂0 were cooled to temperatures at which the
hyperfine interaction energy of an introduced Mn⁵⁴ impurity was comparable to kT. This resulted in a preferential
population distribution of the available energy states. The alignment of nuclear spin, induced by the crystalline field present at the active Mn⁵⁴ impurity, was measured by the anisotropic distribution of the ƴ-rays given off by the radioactive Mn⁵⁴. This data led to a determination of the crystalline field acting on the impurity ion in MnSiF₆.6H₂0 and to verification
of theoretical calculations representing the anisotropy of ƴ-emission as a function of absolute temperature. Also by means of such data, a determination was made of the axes of alignment in the antiferromagnetic, CoC1₂.6H₂0 . / Science, Faculty of / Physics and Astronomy, Department of / Graduate
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Gamma radiations from the bombardment of boron ten with protons and deuteronsChadwick, George Brierley January 1955 (has links)
The gamma rays resulting from the bombardment of B¹⁰ with protons of energies from 0.5 to 2.0 Mev. have been observed with a sodium iodide scintillation counter. Capture radiation, of energy
E[subscript γ] = 8.81 ± 0.05 + 10/11 E[subscript p] Mev.,
showed a broad resonance at E[subscript p] = 1135 ± 15 kev. At this energy, the radiation had an angular distribution of the form 1 + (0.5 ± 0.05)cos²θ and a total cross section (3.5 ± 1.0) × 10[power -30] cm². Several lower energy radiations were also observed and assigned tentatively to cascade transitions in en.
The cross section for the 430 kev. radiation from the reaction B¹⁰ (p, αγ)Be⁷ was measured to be 0.21 ± 0.05 bn. at E[subscript p] = 1.52 Mev. This radiation was found to be isotropic.
A three crystal scintillation counter pair spectometer has been constructed and used to observe the gamma radiations from the bombardment of B¹⁰ with deuterons of energies from 0.6 to 2.0 Mev. The spectrometer incorporated a selection of those pulses in the side counters representing 0.5 Mev. energy release before they entered a triple coincidence circuit, responding to coincidence between the three counters. The improved energy resolution and background rejection allowed the complex gamma ray spectra from B¹⁰ + d to be resolved and interpreted. / Science, Faculty of / Physics and Astronomy, Department of / Graduate
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A single crystal sodium iodide scintillation spectrometer for the investigation of gamma-ray spectraAzuma, Richard Ernest January 1953 (has links)
A single crystal sodium iodide spectrometer has been developed for the investigation of gamma-ray spectra. The spectrometer was tested with the gamma-rays from the sources Eu¹⁵⁵,RaD, Na²², Zn⁶⁵, Co⁶⁰, and RdTh. The spectra from these sources have been obtained by analyzing the pulse height distribution from the scintillation counter with a single channel differential discriminator.
A crystal mounting technique is described in which the crystals are mounted dry with a layer of magnesium oxide powder surrounding them to provide diffuse reflecting surfaces. With mountings of this type, 7% energy resolution has been achieved for gamma-ray energies of approximately 1 MeV.
The expected pulse height distributions have been calculated and compared with the experimental distributions. The effect of multiple scattering events on the shape of the distributions is discussed,2and the effect of crystal dimensions on the resolution has been studied. It has been found that for the energy region 0.5 to 2.5 MeV the best resolution is obtained with small crystals.
A search has been made for the presence of low energy gamma-rays in the decay of tritium, and it was found that within the accuracy of the experiment no gamma-rays were present.
A preliminary report is presented on the investigation of possible scintillation produced in air by alpha particles. The effect has been shown to exist but no systematic study has been made. / Science, Faculty of / Physics and Astronomy, Department of / Graduate
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Gamma radiation from the proton bombardment of lithium sixAlexander, Thomas Kennedy January 1955 (has links)
The reaction Li⁶(p,γ)Be⁷ has been investigated using 0.4 to 1 Mev. energy protons incident on isotopically separated Li⁶ targets. Capture gamma radiation to the ground state and the 430 Kev. state in Be⁷ has been observed; some 62% of the transitions go to the ground state. The ratio of intensities does not change significantly with energy, nor with angle of observation at Ep = 750 Kev. The differential cross section with the counter at 90° to the proton beam and Ep = 750 Kev; is about 2 x 10⁻³²cm²/steradian. The combined angular distribution of the two gamma rays is 1 + (1.05 ± 0.15)cos²θ at Ep = 750 Kev. The Q value for the reaction is 5.66 ± 0.03 Mev. in fair agreement with that calculated from mass values. / Science, Faculty of / Physics and Astronomy, Department of / Graduate
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Lifetimes of gamma-ray transitions by delayed-coincidence measurementsMacKenzie, Innes Keith January 1953 (has links)
An apparatus for the measurement of the lifetimes of gamma-ray transitions between nuclear excited states has been designed and constructed. With this apparatus, lifetimes as short as 1.5 x 10⁻¹⁰ seconds may be determined. This lower limit is shown to be inherent in the scintillation detectors available and not in the electronic circuits which are themselves capable of much better performance. Measurements have been carried out on several radioactive nuclei and have yielded the following results:
(1) The two excited states of Ni⁶⁰ have half-lives less than 1.6 x 10⁻¹⁰ seconds.
(2) The three excited states of Co⁵⁹ have half-lives less than 2 x 10⁻¹⁰ seconds.
(3) No detectable half-life is found in the decay of Eu¹⁵²,¹⁵⁴.
(4) An excited state with a half-life of 1.1 x 10⁻⁹ seconds is present in W¹⁸². We identify this transition as magnetic quadrupole.
(5) A half-life.of 2.3 x 10⁻¹⁰ seconds is found for the .607 Mev transition in Te¹²⁴ which has previously been classified as electric quadrupole. / Science, Faculty of / Physics and Astronomy, Department of / Graduate
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Scintillation counters for gamma-ray measurements and a study of the gamma-rays from the D (p.Y) He[3] reactionGriffiths, George Motley January 1953 (has links)
The development of scintillation counters for measurements of Ƴ-ray energies and fluxes is described, with particular emphasis on Y-rays in the energy range 2 to 20 Mev. A comparison has been made between the experimentally observed and theoretically predicted properties of these counters.
A three-crystal pair spectrometer has been developed which measures only those Ƴ-rays which interact with the detector crystal by producing electron-positron pairs. This device has proved useful for investigating the pair production process for Ƴ-rays with energies only 150 Kev. above the pair production threshold, as well as for the investigation of the complex Ƴ-ray spectrum produced by the F¹⁹(p,αƳ)0¹⁶ reaction.
A detailed study of the D(p,Ƴ)He³ reaction has been made. The Ƴ-ray energy indicates that the transition goes to the ground state of He³. The shift in Ƴ-energy with changing proton, energy was, observed, and fits the following relation:
E[subscript] Ƴ = (5.50 ± 0.03) + ⅔ E[subscript]p Mev.
The Doppler shift of the Ƴ-ray energy (frequency) as a function of the angle between the directions of the incident protons and emitted Ƴ-rays has been measured. The observed shift has the full value expected, assuming that the Ƴ-rays are emitted in a time short compared to the slowing down time of the intermediate He³ nucleus in the target. From these results an upper limit of 2 x 10¹³sec. can be placed on the half-life for the Ƴ-ray transition. The cross section for the reaction for incident protons of 1 Mev. is estimated to be 6 x 10⁻³⁰ cm² (± 50%). The excitation function has been measured from 250 Kev. to 1.8 Mev. and the angular distribution of the Ƴ-rays has the form (Sin² θ + b) where b = 0.046 ± 0.005 for 1 Mev. protons and b = 0.025 ±0.006 for 1.75 Mev. protons. These results, when compared with recent theory, indicate that the reaction is due to direct radiative capture of the protons.
Preliminary measurements have been made on the T(p,Ƴ)He⁴ reaction. The Ƴ-ray energy measured relative to the Ƴ rays from the Li⁷(p,Ƴ)Be⁸ reaction is 20.3 ± 0.4 Mev. for 800 Kev. incident protons, indicating that the transition goes directly to the ground state of the helium nucleus. The angular distribution of, the Ƴ-rays measured in a plane containing the incident proton beam direction is predominantly Sin² θ with the addition of a small isotropic component. The present approximate measurements show a greater isotropic component than that obtained at higher proton energy by other workers. / Science, Faculty of / Physics and Astronomy, Department of / Graduate
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