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Detection of Light 3rd Revised edition [Kõva köide]

(University of Arizona)
  • Formaat: Hardback, 450 pages, kõrgus x laius x paksus: 175x250x25 mm, kaal: 830 g
  • Ilmumisaeg: 13-May-2021
  • Kirjastus: Cambridge University Press
  • ISBN-10: 110712414X
  • ISBN-13: 9781107124141
  • Formaat: Hardback, 450 pages, kõrgus x laius x paksus: 175x250x25 mm, kaal: 830 g
  • Ilmumisaeg: 13-May-2021
  • Kirjastus: Cambridge University Press
  • ISBN-10: 110712414X
  • ISBN-13: 9781107124141
The invention and development of advanced methods to detect light underlies much of modern technology. This fully updated and restructured third edition is unique amongst the literature, providing a comprehensive, uniform discussion of a broad range of detection approaches. The material is accessible to a broad range of readers rather than just highly trained specialists, beginning with first principles and developing the relevant physics as it goes. The book emphasizes physical understanding of detector operation, without being a catalog of current examples. It is self-contained but also provides a bridge to more specialized works on specific approaches; each chapter points readers toward the relevant literature. This will provide a broad and lasting understanding of the methods for detecting light that underpin so much of our technology. The book is suitable for advanced undergraduate and graduate students, and will provide a valuable reference for professionals across physics and engineering disciplines.

Fully restructured and updated, Detection of Light introduces the whole range of photon detectors from first principles to an audience with a modest background in physics. These devices are central to much of our technology, making this an ideal resource for students and professionals in many technical areas.

Arvustused

'The book introduces the detection of light and is designed to be accessible to a broad range of readers rather than just highly trained specialists is an ideal read for master's and Ph.D. students in astronomical instrumentation.' Silvano Donati, Optics & Photonics News 'The book is increased in breadth from earlier editions, and now covers the vast majority of the electromagnetic spectrum, from millimetre wavelengths to X-rays it is undoubtedly authoritative, as expected from a leading practising expert in the field underlying physics is explained at just the right depth required to understand each type of detector [ and] it gets beyond simplistic, generic descriptions to explain how and why real-world detectors have been refined in design, clarifying the strengths and weaknesses of each modification or increased layer of sophistication the book could be usefully purchased as 'technical backup' by those involved in teaching, say, observational astronomy. It is also pitched at just the right level for masterslevel or postgraduate students pursuing work involving the development of astronomical instrumentation, or indeed any area of physics involving photon detection.' James S. Dunlop, The Observatory

Muu info

Comprehensive, accessible, and physically based description of the approaches currently used to detect light, from X-ray to mm-wave.
Preface ix
1 Introduction
1(23)
1.1 Radiometry
1(8)
1.2 Detector Types
9(1)
1.3 Performance Characteristics
10(9)
1.4 Radiometry Example
19(2)
1.5 Problems
21(1)
1.6 Note
22(1)
1.7 Further Reading
23(1)
2 Photodetector Basics
24(34)
2.1 Solid State Physics
24(8)
2.2 Intrinsic Photoconductors
32(16)
2.3 Extrinsic Photoconductors
48(6)
2.4 Example: Design of a Photoconductor
54(1)
2.5 Problems
55(2)
2.6 Further Reading
57(1)
3 Infrared (and Optical) Photodetectors
58(41)
3.1 Photodiodes
58(26)
3.2 Extrinsic Doped Silicon Detectors
84(8)
3.3 Problems
92(2)
3.4 Note
94(3)
3.5 Further Reading
97(2)
4 Amplifiers, Readouts, and Arrays
99(35)
4.1 Building Blocks
99(3)
4.2 Load Resistor and Amplifier
102(1)
4.3 Transimpedance Amplifier (TIA)
103(6)
4.4 Integrating Amplifiers
109(11)
4.5 Detector Arrays
120(7)
4.6 X-ray Detection with DEPFETs
127(2)
4.7 High Energy X-ray Detectors
129(1)
4.8 Example: Readout Performance
130(2)
4.9 Problems
132(1)
4.10 Further Reading
133(1)
5 Charge Coupled Devices
134(40)
5.1 Basic Operation
134(5)
5.2 CCD Performance at Faint Light Levels
139(15)
5.3 Quantum Efficiency and Spectral Range
154(8)
5.4 Optical/Infrared Detector Test Procedures
162(8)
5.5 Example
170(2)
5.6 Problems
172(1)
5.7 Further Reading
173(1)
6 Other Photodetectors
174(41)
6.1 Photography
174(6)
6.2 Photoemissive Detectors
180(25)
6.3 Example
205(1)
6.4 Quantum Well Detectors
206(7)
6.5 Energy-Resolving Detectors
213(1)
6.6 Problems
213(1)
6.7 Further Reading
214(1)
7 Superconducting Detectors
215(30)
7.1 Superconductivity
215(7)
7.2 Superconducting Electronics
222(1)
7.3 Microwave Kinetic Inductance Detectors (MKIDs)
223(12)
7.4 Other Superconducting Detectors
235(7)
7.5 Problems
242(2)
7.6 Further Reading
244(1)
8 Bolometers
245(34)
8.1 Basic Operation
245(2)
8.2 Room Temperature Thermal Detectors
247(3)
8.3 Cryogenic Semiconductor Bolometers
250(10)
8.4 Superconducting Bolometers
260(4)
8.5 Bolometer Construction Components
264(4)
8.6 Examples of Bolometer Construction
268(3)
8.7 Other Thermal Detectors
271(4)
8.8 Example: Design of a Bolometer
275(2)
8.9 Problems
277(1)
8.10 Further Reading
277(2)
9 Visible and Infrared Coherent Receivers
279(24)
9.1 Basic Operation
279(4)
9.2 Visible and Infrared Heterodyne
283(10)
9.3 Heterodyne Performance Attributes
293(8)
9.4 Problems
301(1)
9.5 Further Reading
302(1)
10 Submillimeter- and Millimeter-Wave Heterodyne Receivers
303(43)
10.1 Basic Operation
303(5)
10.2 Mixers
308(16)
10.3 Local Oscillators
324(6)
10.4 Backends
330(1)
10.5 Performance Characteristics
331(5)
10.6 Improvements in Receiver Capabilities
336(1)
10.7 Performance Comparison
337(2)
10.8 Example
339(1)
10.9 Problems
340(1)
10.10 Note
341(4)
10.11 Further Reading
345(1)
Appendix A Useful Constants and Conversions 346(1)
Appendix B Answers to Selected Problems 347(3)
References 350(16)
Index 366
George H. Rieke is Regents Professor of Astronomy and Planetary Sciences at the University of Arizona. He switched from TeV gamma rays to the infrared just in time to enjoy its growth from primitive beginnings, to culminate with the launch of JWST. He has contributed to many scientific and technical topics along the way, gaining the background for this broad-ranging book. His other books include The Last of the Great Observatories (2006) and Measuring the Universe (Cambridge, 2017), which won the American Astronomical Society's Chambliss Astronomical Writing Award.