Development of liquid xenon detectors for gamma ray astronomy
The application of liquid xenon in high resolution detectors for gamma ray astronomy is being investigated. Initial results from a pulse shape analysis of ionization signals in a liquid xenon gridded chamber indicate that we are able to achieve the necessary liquid purity for the transport of free electrons with simple techniques. The energy resolution has been measured as a function of applied electric field, using electrons and ..gamma..-rays from a /sup 207/Bi source. At a field of 12 kV/cm the noise subtracted energy resolution of the dominant 569 keV ..gamma..-ray line is 34 keV FWHM. This value, which is the best reported to date in liquid xenon at similar field strengths, is mostly determined by recombination of electron-ion pairs on delta-electron tracks.
- Research Organization:
- Physics Dept. and Astrophysics Lab., Columbia Univ., New York, NY (US)
- OSTI ID:
- 6415634
- Report Number(s):
- CONF-881103-; TRN: 89-009905
- Journal Information:
- IEEE Trans. Nucl. Sci.; (United States), Vol. 36:1; Conference: IEEE nuclear science symposium, Orlando, FL, USA, 9 Nov 1988
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
GAMMA ASTRONOMY
GAS SCINTILLATION DETECTORS
PERFORMANCE
XENON
BISMUTH 207
ELECTRIC FIELDS
ELECTRON TRANSFER
ION SOURCES
RECOMBINATION
ASTRONOMY
BETA DECAY RADIOISOTOPES
BETA-PLUS DECAY RADIOISOTOPES
BISMUTH ISOTOPES
ELECTRON CAPTURE RADIOISOTOPES
ELEMENTS
FLUIDS
GASES
HEAVY NUCLEI
ISOTOPES
MEASURING INSTRUMENTS
NONMETALS
NUCLEI
ODD-EVEN NUCLEI
RADIATION DETECTORS
RADIOISOTOPES
RARE GASES
SCINTILLATION COUNTERS
YEARS LIVING RADIOISOTOPES
440104* - Radiation Instrumentation- High Energy Physics Instrumentation
640100 - Astrophysics & Cosmology