The physics of radiation detection has barely changed in a generation — yet the instruments built on it have been transformed.
Silicon photomultipliers have displaced vacuum tubes, new scintillator crystals reach resolutions once out of reach, room-temperature semiconductor detectors are now routine, a global helium-3 shortage reshaped neutron detection, and signal processing has become almost entirely digital. Anyone who learned from older references faces a widening gap between the classic foundations and the equipment actually in use — with no single, rigorous, current account that connects the two.
This comprehensive guide closes that gap. It keeps the durable physics — energy loss in matter, the statistics of counting, and the operating principles of every major detector — and rebuilds the modern technology around it, developing each result from first principles and showing the full working of every derivation and worked example.
Inside, you will:
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