Compton Scattering

Compton Scattering

Compton Scattering MIT Department of Physics (Dated: August 27, 2013) You will observe the scattering of 661.6 keV photons by electrons and measure the energies of the scattered gamma rays as well as the energies of the recoil electrons. The results can be compared with the formulas for Compton scattering, considering the quantized photon like a particle. PREPARATORY QUESTIONS an intense collimated beam of monochromatic molybde- num Kα X-rays and using an ionization chamber as the Please visit the Compton Scattering chapter on the detector in his spectrometer, Compton found that the 8.13x website at mitx.mit.edu to review the background spectrum of scattered X-rays had two distinct spectral material for this experiment. Answer all questions found lines, one at the wavelength of the incident X-rays and in the chapter. Work out the solutions in your laboratory another at a wavelength that was longer by an amount notebook; submit your answers on the web site. that depends on the angle of scattering. The scatter- ing without a wavelength shift was readily explained by the classical theory of coherent scattering of electro- SUGGESTED SCHEDULE magnetic waves from electrons bound in atoms. How- ever, the classical theory provided no explanation of the • Day 1: Familiarize yourself with the equipment and wavelength-shifting \incoherent" scattering process. The do Section III.1. phenomenon of Bragg reflection used in Compton's mea- surements was a clear demonstration of the wavelike char- • Day 2: Repeat Section III.1 and do Section III.2. acter of the X-rays. Nevertheless, Compton put forward By the end of this session you should have verified the apparently contradictory idea that X-rays, known to that Escat + Erecoil ≈ 662 keV for at least two be electromagnetic radiation of very short wavelength, angular positions. interact with electrons like particles of zero rest mass so that their energy E = hν = hc/λ and momentum p are • Day 3: Perform Section III.3. related by the relativistic equation for particles of zero rest mass, namely p = E=c. He calculated according • Day 4: Repeat portions of the experiment that need to relativistic mechanics the relations between the initial improvement. and final energies and momenta of an X-ray quantum and a free electron involved, like billiard balls, in an elas- I. INTRODUCTION tic collision. In this way he arrived at the formula for the \Compton shift" in the wavelength of incoherently scattered X-rays, namely (see [2], AppendixA) By 1920 the successes of the quantum theories of black- body spectra (Planck, 1901), the photoelectric effect h ∆λ = (1 − cos θ); (1) (Einstein, 1905) and the hydrogen spectrum (Bohr, 1913) mc had established the idea that interactions between elec- tromagnetic radiation of frequency ν and matter occur where m is the mass of the electron and θ is the an- through the emission or absorption of discrete quanta of gle between the trajectories of the incident and scattered energy E = hν. The next crucial step in the development photon. of the modern concept of the photon as the particle of The agreement between Compton's experimental re- electromagnetic radiation was taken by Arthur Compton sults confronted physicists and philosophers with the con- in the interpretation of experiments he initiated in 1920 ceptual dilemma of the particle-wave duality of electro- to measure with precision the wavelengths of X-rays scat- magnetic radiation. In particular, how was one to un- tered from electrons in materials of (low atomic number) derstand how each particle of light in a Young interfer- [1,3]. The phenomena of X-ray scattering had already ence experiment goes simultaneously through two slits? been studied intensively. It was known that the penetrat- The dilemma was further compounded when, in 1924, ing power of X-rays decreases with increasing wavelength de Broglie put forward the idea that material particles and that X-rays are less penetrating after being scattered (i.e. electrons, protons, atoms, etc.) should exhibit wave- than before, which indicated that the scattering process like properties characterized by a wavelength λ related to somehow increases their wavelength. their momentum p by the same formula as that for light Compton's idea was to use the recently developed tech- quanta, namely λ = h=p. In 1927 the wave-like properties nique of high-resolution X-ray spectrometry, based on of electrons were discovered by Davisson and Germer in measurement of the angle of Bragg reflection of X-rays experiments on the reflection of electrons from crystals. from crystals, to measure precisely the wavelengths of A particularly interesting account of these developments the scattered X-rays [4]. Irradiating a carbon target with is given by Compton and Allison in their classic treatise [5]. Id: 01.compton.tex,v 1.63 2013/08/27 19:20:55 spatrick Exp Id: 01.compton.tex,v 1.63 2013/08/27 19:20:55 spatrick Exp 2 I.1. Experimental Goals 1. Kinematics and theory of Compton scattering; 2. Properties of 137Cs; In this experiment you will measure: 3. Scintillation counters and the interpretation of 1. the energies of Compton-scattered gamma-ray pho- pulse height spectra (see preparatory question 3); tons and recoil electrons, 4. Radiation safety; 2. the frequency of scattering as a function of angle θ, and 5. Parameter and error estimation [6]. 3. the total cross section of electrons for Compton scattering. II. EXPERIMENTAL ARRANGEMENT The results of the energy measurements will be compared with the predictions of Compton kinematics. The re- The experimental arrangement for the Compton ex- sults of the scattering rate and cross section measure- periment is shown schematically in Figure1. The 2"x2" ments will be compared with the predictions of the clas- cylindrical \recoil electron" or \target" scintillator de- sical (Thomson) theory of X-ray scattering and with the tector (Canberra model 802-3/2007), is irradiated by a Klein-Nishina formula derived from relativistic quantum beam of 661.6 keV photons emitted by about 100 µCi theory. (≈ 1 microgram!) of 137Cs located at the end of a hole in The experimental setup employs a radioactive source a large lead brick which acts as a gamma-ray \howitzer". of 661.6 keV photons from 137Cs, and two NaI scintilla- If a photon entering the target scintillator scatters from tion counters. One counter serves as the scattering target a loosely bound, effectively free, electron, the resulting and measures the energy of the recoil electrons; the other recoil electron may lose all of its energy in the target, counter detects the scattered photons and measures the causing a scintillation pulse with an amplitude propor- energy they deposit. Both the target and scatter coun- tional to the energy of the recoil electron. If the scattered ters have a scintillator consisting of a 2"×2" cylinder of photon emerges from the target scintillator without fur- Thallium-activated sodium iodide optically coupled to a ther interaction, and if its trajectory passes through the photomultiplier. A 661.6 keV photon traversing sodium NaI crystal of the \scattered photon" detector, it will iodide has about equal probability of undergoing photo- have a substantial probability of depositing all of its en- electric absorption and Compton scattering. A photo- ergy by a single photoelectric interaction or by a sequence electric absorption event is a quantum mechanical tran- of Compton scatterings and photoelectric interactions. sition from an initial state consisting of an incident pho- This will produce a scintillation pulse that contributes ton of energy E and a neutral atom to a final state. This to the \photopeak" of the pulse height spectrum. The event therefore consists of an excited ion with a vacancy median channel of the photopeak in the multichannel an- in one of its inner shells where the electron that was for- alyzer (MCA) display is a good measure of the median merly bound and a free \photoelectron" with kinetic en- energy of the detected photons. If the scattered photon ergy E−W , where W is the binding energy of the electron undergoes a Compton scattering in the scatter scintilla- in the neutral atom. The energetic photoelectron loses its tor and then escapes from the scintillator, the resulting energy within a small fraction of a microsecond by multi- pulse, with a size proportional to the energy of the Comp- ple Coulomb interactions with electrons and nuclei in the ton recoil electron, will be registered in the Compton re- sodium iodide crystal, and a certain fraction of the lost coil continuum of the spectrum. Several experimental energy is converted into scintillation light. Meanwhile, details are considered in [7{11]. the ion from which the photoelectron was ejected loses In the experimental arrangement described by [2] (pg. its energy of excitation through a cascade of transitions 256) the target is inert material (not a detector). The that fill the vacancy in its electronic structure and give scatter counter suffers background due to gamma-ray rise to lower energy photons or electrons that, in turn, photons leaking through the lead from the 137Cs source, lose their energy in the crystal and generate additional cosmic rays, and radioactive isotopes in the environ- scintillation light. ment which is suppressed by the use of very heavy The total amount of scintillation light produced is (≈ 200 lb) lead shielding around the source and the scat- closely proportional to the total amount of energy dissi- ter counter. Without such shielding and without any pated in all these processes. As a consequence, the pulse electronic tricks the pulses produced by Compton scat- height spectrum of a NaI scintillation counter exposed to tered photons would be buried in the background.

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