Effect of Spectral Broadening and Electron-Hole Scattering on Carrier

Total Page:16

File Type:pdf, Size:1020Kb

Effect of Spectral Broadening and Electron-Hole Scattering on Carrier Effect of spectral broadening and electron-hole scattering on carrier relaxat!on in GaAs quantum dots lgor Vurgaftman and Jasprit Singh Solid State Electronics Laboratory, Department of Electrical Engineering and Computer Science, The University of Michigan, Ann Arbol; Michigan 48109-2122 (Received 13 August 1993; accepted for publication 2 November 1993) Luminescence efficiency in quantum dots has been a matter of some controversy recently. Theoretically, poor efficiency has been predicted owing to the phonon bottleneck in carrier relaxation, while slightly enhanced luminescence has been reported in several experiments. The approach of this letter differs from previous theoretical work in that the scattering rates are computed self-consistently accounting for the spectral broadening of the electronic spectra due to a finite energy level lifetime. Scattering of electrons and holes confined in the dot is found to be responsible for breaking the phonon bottleneck in electron relaxation reducing the relaxation time from several ns to several hundred ps. Results of a Monte Carlo simulation also including confined and interface polar optical phonon and acoustic phonon scattering for a range of quantum dot dimensions and temperatures are presented. These results may provide an explanation of the absence of a significant reduction in quantum dot luminescence compared with that from quantum wells. The optoelectronic properties of quasi-one-dimensional In this letter, we present a theoretical analysis of electron electronic systems have been investigated recently for poten- relaxation in GaAs/Alo,sGao.,As quantum dots based on a tial applications in ultralow threshold semiconductor lasers’ Monte Carlo simulation of the equilibration process with the and with regard to the predicted enhancement in optical inclusion of self-consistently calculated electron-phonon and nonlinearities.2 The realization is growing, however, that al- electron-hole scattering processes. An idealized flat-band po- though the discrete eigenvalue spectrum in quantum dots re- tential profile is assumed, i.e., no attempt is made to describe sults in a greatly increased oscillator strength for optical tran- the band-bending properties of the GaAs/AlGaAs system re- sitions, coupling of electrons to polar optical phonons (POP) sulting from a particular fabrication process. The electronic may be drastically reduced in small dots, and as a result, spectrum is found by solving the Schriidinger equation in the relaxation of electrons to the ground state may be hindered. effective mass approximation, and the hole states are derived Phonon scattering rates in quantum dots have been studied by diagonalizing the four-band Kohn-Luttinger Ham& by Bockelmann and Bastard? They pointed out that unless tonian, in which the standard prescription for calculating the electron states are separated by the energy of the optical quantum confined states [k, --+ - i( d/h), etc.] is used. In phonon, the mechanism for POP scattering in quantum dots order to estimate the electron-hole scattering rate, for the is different from that in bulk semiconductors. Electron relax- sake of computational simplicity, the off-diagonal coupling ation may occur as a result of phonon renormalization, terms in the Hamiltonian are set to zero. The eigenenergies broadening of the electron and phonon spectrum, emission of and eigenfunctions are found by discretizing the volume of short-wavelength acoustic phonons, or higher order phonon the dot on a uniform spatial mesh terminated far away from scattering processes. Considering electron relaxation by the dot interfaces, approximating derivatives as finite differ- emission of acoustic phonons, Benisty et aL4 have predicted ences, and solving the resulting matrix equation iteratively. poor radiative efficiency in quantum dots with lateral dimen- The macroscopic electrostatic model has proved useful sions less than 500 A in consequence of the electron relax- in approximating the spatial structure and dispersion rela- ation times being comparable to nonradiative recombination tions for phonon models in quantum wells and wires.” We times (a few ns). Although a number of experiments have assume that the confined phonon modes are given by linear been reported which appear to substantiate this combinations of products of sines and cosines, whose wave conclusion,5-7 several workers have observed luminescence in very small quantum dots, in which the effect of the pho- vector is fixed at multiples of wfLi, where i=x,y,z, by im- non bottleneck should become noticeable.“,’ Recently en- posing the boundary condition that the phonon mode vanish hanced luminescence has been observed in 35-nm InGaAs/ near the interface with a material with a different resonant GaAs quantum dots defined by a combination of electron vibration frequency. Since the nonepitaxial dimensions beam epitaxy, dry etching, and molecular beam epitaxial greater than 20 nm are examined in this letter, we assume regrowth,” although fabrication-induced changes in the po- quantum well interface phonon modes varying as hyperbolic tential profile in those structures may be substantial. In ex- sines and cosines with the dispersion relation derivable from perimentally realizable quantum dots, nomadiative recombi- the boundary condition.” The interface phonon energies lie nation may be enhanced by controllable defects as well as by in the Reststrahlen region between the transverse (tio,=33 the relaxation bottleneck; therefore, the issue of electron re- meV in GaAs) and longitudinal (fiwLo=36 meV) optical laxation in quantum dots cannot be considered well under- phonon energies. stood at present. The confined POP scattering rate is calculated using the 232 Appl. Phys. Lett. 64 (2), 10 January 1994 0003-6951/94/64(2)/232,‘3/$6.00 Q 1994 American Institute of Physics Friihlich form of the interaction Hamiltonian from the Fermi 0.18 Without SHS Epilibqium Golden Rule: ____.________.......__ ,.. ,.,....,,.., . @P=gl!~,*g;p (; -$) , , Y 2 x[(f)2+( y i’+(Ei ’]-’ 1; 1 1 x rz(OLO)f~ 2)-z MyyZ,m,n) 2 1 )I I x a(Ef-Ei+hwJJo), (1) 0.0 200.0 400.0 600.0 800.0 1000.0 where Iif is the overlap integral for the cell periodic parts of TIME AFTER INJECTION (PS) the electron wave function, presumed unity in this work, and the rest of the symbols have their usual meaning. The upper FIG. 1. The mean electron energy as a function of time after injection for sign corresponds to phonon emission, the lower sign to ab- the 50 AX250 AX250 A GaAs/Al,,ZGao,,As quantum dot at 300 K. The sorption. Taking an arbitrary vertex of the box as origin, the horizontal line represents the equilibrium mean energy. The averaging is overlap integral for the envelope parts of the wave function over 5000 carriers. can be written down simply as POP modes. Due to the weaker coupling of acoustic phonons M~(l,m,n)= d”rcp;(r)sin rT)Sin(y)Sin(z- F) cpi(r). to electrons, the broadening linewidth is also much smaller than that for POP. (2) The Pauli exclusion principle has to be considered in the The delta function in Eq. (1) is replaced by a Gaussian line occupation of discrete quantum dot levels. However, because shape function: of the small size of dots under study, it is permissible to assume that only one electron is injected in any one quantum qq-.E,+fio& + &XP ( -(?;4;;?o)2). (3) dot. With this assumption, the electron-electron interaction and screening can be ignored. Previous treatments of elec- An iterative self-consistent calculation of the scattering rates tron relaxation mechanisms in quantum dots have not in- and the linewidth (~=li/r, where r is taken to be the recipro- cluded electron-hole (EH) scattering. Since the hole confine- cal of the scattering rate, is necessary to determine Wp ment energy is much smaller than that for the electron, the from Eqs. (l)-(3). The scattering rates have also been calcu- hole distribution can be assumed to be in thermal equilibrium lated for interface phonon modes and have been found to be with the lattice. Therefore, the electron may lose energy by lower by two orders of magnitude than the rates for confined interacting with a thermalized hole in the valence band. The bulklike phonons. Consequently, even for phonon energies in matrix element can be computed in the Born approximation: the range between 33 and 36 meV, confined phonon scatter- ing dominates, with the energy difference made up by the d3q, 2 ipi*‘(r,)~fh~‘~rk); broadening of the electronic spectrum. By assumption, the v=l lattice is maintained at a constant temperature. In quantum wires, acoustic phonon (AP) scattering is one of the mechanisms responsible for electron relaxation for quantum wires of cross sections less than 100 AX 100 A-l2 In where the sum runs over the 13/2,-t3/2) and 13/2,+1/2) an- quantum dots, the AP scattering rate can be calculated using gular momentum statesThe scattering rate is calculated by the Fermi Golden Rule and the deformation potential theory: applying the Fermi Golden Rule with the broadening found in an iterative fashion as described above. y‘y= 7r c f=(n(mq)+; 2;) Given the relevant scattering rates, electron relaxation P-wyL q wq can be modeled by a Monte Carlo simulation. Electrons are 2 injected at the top of the potential barrier in a thermal distri- X d3r (pT(r)e’g”qi(r) S(Ef-Eikfi~~), (4) bution, and their evolution is followed in energy and time. II An averaging over a large number of electrons (and equiva- where p is the mass density of GaAs, DA is the acoustic lently, dots) is necessary in order to produce statistically re- deformation potential, and q is the phonon wave vector with liable results. In Fig. 1 the evolution of the mean energy of a continuous spectrum. We include acoustic phonon scatter- the electron distribution in the 50 AX250 AX250 A ing in our Monte Carlo simulation, although in small quan- GaAs/Al,,Gao,,As quantum dot at 300 K is shown.
Recommended publications
  • Glossary Physics (I-Introduction)
    1 Glossary Physics (I-introduction) - Efficiency: The percent of the work put into a machine that is converted into useful work output; = work done / energy used [-]. = eta In machines: The work output of any machine cannot exceed the work input (<=100%); in an ideal machine, where no energy is transformed into heat: work(input) = work(output), =100%. Energy: The property of a system that enables it to do work. Conservation o. E.: Energy cannot be created or destroyed; it may be transformed from one form into another, but the total amount of energy never changes. Equilibrium: The state of an object when not acted upon by a net force or net torque; an object in equilibrium may be at rest or moving at uniform velocity - not accelerating. Mechanical E.: The state of an object or system of objects for which any impressed forces cancels to zero and no acceleration occurs. Dynamic E.: Object is moving without experiencing acceleration. Static E.: Object is at rest.F Force: The influence that can cause an object to be accelerated or retarded; is always in the direction of the net force, hence a vector quantity; the four elementary forces are: Electromagnetic F.: Is an attraction or repulsion G, gravit. const.6.672E-11[Nm2/kg2] between electric charges: d, distance [m] 2 2 2 2 F = 1/(40) (q1q2/d ) [(CC/m )(Nm /C )] = [N] m,M, mass [kg] Gravitational F.: Is a mutual attraction between all masses: q, charge [As] [C] 2 2 2 2 F = GmM/d [Nm /kg kg 1/m ] = [N] 0, dielectric constant Strong F.: (nuclear force) Acts within the nuclei of atoms: 8.854E-12 [C2/Nm2] [F/m] 2 2 2 2 2 F = 1/(40) (e /d ) [(CC/m )(Nm /C )] = [N] , 3.14 [-] Weak F.: Manifests itself in special reactions among elementary e, 1.60210 E-19 [As] [C] particles, such as the reaction that occur in radioactive decay.
    [Show full text]
  • Or Continuous Spectrum and Not to the Line Spectra. in the X-Ray Region, In
    662 PHYSICS: W. D UA NE PROC. N. A. S. intensity is greatest close to -80 and that it falls off regularly as the angle departs therefrom. We conclude, therefore, that the momentum of the electron in its orbit uithin the atom does not affect the direction of ejection in the way denanded by the theory of Auger and Perrin. While this does not constitute definite evidence against the physical reality of electronic orbits, it is a serious difficulty for the conception. A detailed discussion of the general question here raised in the light of new experimental results will be published elsewhere. 1 Auger, P., J. Physique Rad., 8, 1927 (85-92). 2 Loughridge, D. H., in press. 3 Bothe, W., Zs. Physik, 26, 1924 (59-73). 4 Auger, P., and Perrin, F., J. Physique Rad., 8, 1927 (93-111). 6 Bothe, W., Zs. Physik, 26,1924 (74-84). 6 Watson, E. C., in press. THE CHARACTER OF THE GENERAL, OR CONTINUOUS SPEC- TRUM RADIA TION By WILLIAM DuANX, DJPARTMSNT OF PHysIcs, HARVARD UNIVERSITY Communicated August 6, 1927 The impacts of electrons against atoms produce two different kinds of radiation-the general, or continuous spectrum and the line spectra. By far the greatest amount of energy radiated belongs to the general, or continuous spectrum and not to the line spectra. In the X-ray region, in particular, the continuous, or general radiation spectrum carries most of the radiated energy. In spite of this, and because the line spectra have an important bearing on atomic structure, the general radiation has received much less attention than the line spectra in the recent de- velopment of fundamental ideas in physical science.
    [Show full text]
  • Discrete-Continuous and Classical-Quantum
    Under consideration for publication in Math. Struct. in Comp. Science Discrete-continuous and classical-quantum T. Paul C.N.R.S., D.M.A., Ecole Normale Sup´erieure Received 21 November 2006 Abstract A discussion concerning the opposition between discretness and continuum in quantum mechanics is presented. In particular this duality is shown to be present not only in the early days of the theory, but remains actual, featuring different aspects of discretization. In particular discreteness of quantum mechanics is a key-stone for quantum information and quantum computation. A conclusion involving a concept of completeness linking dis- creteness and continuum is proposed. 1. Discrete-continuous in the old quantum theory Discretness is obviously a fundamental aspect of Quantum Mechanics. When you send white light, that is a continuous spectrum of colors, on a mono-atomic gas, you get back precise line spectra and only Quantum Mechanics can explain this phenomenon. In fact the birth of quantum physics involves more discretization than discretness : in the famous Max Planck’s paper of 1900, and even more explicitly in the 1905 paper by Einstein about the photo-electric effect, what is really done is what a computer does: an integral is replaced by a discrete sum. And the discretization length is given by the Planck’s constant. This idea will be later on applied by Niels Bohr during the years 1910’s to the atomic model. Already one has to notice that during that time another form of discretization had appeared : the atomic model. It is astonishing to notice how long it took to accept the atomic hypothesis (Perrin 1905).
    [Show full text]
  • Spectrum (Functional Analysis) - Wikipedia, the Free Encyclopedia
    Spectrum (functional analysis) - Wikipedia, the free encyclopedia http://en.wikipedia.org/wiki/Spectrum_(functional_analysis) Spectrum (functional analysis) From Wikipedia, the free encyclopedia In functional analysis, the concept of the spectrum of a bounded operator is a generalisation of the concept of eigenvalues for matrices. Specifically, a complex number λ is said to be in the spectrum of a bounded linear operator T if λI − T is not invertible, where I is the identity operator. The study of spectra and related properties is known as spectral theory, which has numerous applications, most notably the mathematical formulation of quantum mechanics. The spectrum of an operator on a finite-dimensional vector space is precisely the set of eigenvalues. However an operator on an infinite-dimensional space may have additional elements in its spectrum, and may have no eigenvalues. For example, consider the right shift operator R on the Hilbert space ℓ2, This has no eigenvalues, since if Rx=λx then by expanding this expression we see that x1=0, x2=0, etc. On the other hand 0 is in the spectrum because the operator R − 0 (i.e. R itself) is not invertible: it is not surjective since any vector with non-zero first component is not in its range. In fact every bounded linear operator on a complex Banach space must have a non-empty spectrum. The notion of spectrum extends to densely-defined unbounded operators. In this case a complex number λ is said to be in the spectrum of such an operator T:D→X (where D is dense in X) if there is no bounded inverse (λI − T)−1:X→D.
    [Show full text]
  • Continuous Spectrum—Kirchoff's First
    Continuous Spectrum—Kirchoff’s First Law • A hot opaque substance (solid, liquid or gas) gives off a continuous spectrum, that is, a spectrum containing energy at all wavelengths. • Examples where a continuous spectrum will be found: • An incandescent bulb. • A pool of molten iron • Lava flowing from a volcano. • A hot, ionized, opaque gas (such as below the Sun’s atmosphere). • A continuous spectrum approximates a black body spectrum, the spectrum observed from a perfectly black substance heated to a high temperature. No real spectrum is a perfect black body spectrum, but many are good approximations to it. AST 303: Chapter 13 1 Black-body (Continuous) Spectrum • The energy distribution of a black body spectrum looks like this: 1000 Visible 100 10 UV Infrared Intensity (arbitrary units) 1 1000 3000 10000 30000 100000 Wavelength (Ångstroms) AST 303: Chapter 13 2 Wien’s Law—Temperature Dependence (1) • We are familiar with the fact that the color of a heated object changes as its temperature changes. As we heat a substance, it first glows a dull red; then a bright red, then orange, yellow, white, and finally bluish-white. This happens because the distribution of energy with wavelength shifts to predominantly shorter and shorter wavelengths as the temperature rises. • Mathematically, we can calculate the wavelength of maximum emission: 3 !107 Wavelength of Maximum = Å T where T is the temperature in degrees Kelvin. AST 303: Chapter 13 3 How Color Varies with Temperature AST 303: Chapter 13 4 Emission Spectra—Kirchoff’s Second Law • When a transparent gas is heated to a high temperature, one sees an emission spectrum, also known as a bright-line spectrum.
    [Show full text]
  • Continuous Spectrum X-Rays from Thin Targets
    RP 60 CONTINUOUS SPECTRUM X RAYS FROM THIN TARGETS * By Warren W. Nicholas 2 Technique is described for the use of thin metal foils as anticathodes in X-ray- tubes. The continuous radiation from these foils is analyzed by a crystal, the intensities being measured by a photographic comparison method. It is indicated that the high-frequency limit of the continuous spectrum from an infinitely thin target consists of a finite discontinuity. (The corresponding thick target spectrum has only a discontinuity of slope.) The energy distributions on a frequency scale are approximately horizontal, for gold and for aluminum, and for ^=40°, 90°, and 140°, where \I/ is the angle between measured X rays and cathode stream; this agrees with Kramer's, but not with Wentzel's, theory. The intensities for these values of \p are roughly 3:2:1, respectively; theories have not yet been constructed for the variation with \p of resolved energy, but it is pointed out that the observations do not support a supposed quantum process in which a single cathode ray, losing energy hv by interaction with a nucleus, radiates a single frequency v in the continuous spectrum. The observations do not support the "absorption" process assumed by Lenard, in which cathode rays, in penetrating a metal, suffered large losses of speed not accompanied by radiation. The manner in which thick target spectra are synthesized from thin is discussed, and empirical laws are formulated describing the dependence on of thick target continuous spectrum energy. A structure for the moving \f/ electron is proposed which explains classically X ray continuous spectrum phenomena, and seems to have application in other fields as well.
    [Show full text]
  • X-Ray Emission Spectrum
    X-ray Emission Spectrum Dr. Ahmed Alsharef Farah Dr. Ahmed Alsharef Farah 1 • X-ray photons produced by an X-ray tube are heterogeneous in energy. • The energy spectrum shows a continuous distribution of energies for the bremsstrahlung photons superimposed by characteristic radiation of discrete energies. Dr. Ahmed Alsharef Farah 2 There are two types of X-ray spectrum: 1. Bremsstrahlung or continuous spectrum. 2. Characteristic spectrum. Dr. Ahmed Alsharef Farah 3 • A bremsstrahlung spectrum consists of X- ray photons of all energies up to maximum in a continuous fashion, which is also known as white radiation, because of its similarity to white light. • A characteristic spectrum consists of X-ray photons of few energy, which is also called as line spectrum. • The position of the characteristic radiation depends upon the atomic number of the target. Dr. Ahmed Alsharef Farah 4 Dr. Ahmed Alsharef Farah 5 Characteristic X-ray Spectrum: • The discrete energies of characteristic x- rays are characteristic of the differences between electron binding energies in a particular element. • A characteristic x-ray from tungsten, for example, can have 1 of 15 different energies and no others. Dr. Ahmed Alsharef Farah 6 Characteristic X-rays of Tungsten and Their Effective Energies (keV). Dr. Ahmed Alsharef Farah 7 Characteristic x-ray emission spectrum for tungsten contains 15 different x-ray energies. Dr. Ahmed Alsharef Farah 8 • Such a plot is called the characteristic x-ray emission spectrum. • Five vertical lines representing K x-rays and four vertical lines representing L x-rays are included. • The lower energy lines represent characteristic emissions from the outer electron shells.
    [Show full text]
  • Flexible Learning Approach to Physics (FLAP)
    ATOMIC SPECTRA AND THE HYDROGEN ATOM MODULE P8.2 F PAGE P8.2.1 Module P8.2 Atomic spectra and the hydrogen atom 1 Opening items 1 Ready to study? 2 The production of atomic spectra 3 Study comment To study this module you will need to understand the following terms: 2.1 Characteristic emission spectra 3 absolute temperature, angular momentum, angular frequency, atom, Boltzmann’s constant, 2.2 Continuous emission spectra; the centripetal force, circular motion, Coulomb’s law, diffraction grating, dispersion, electric black-body spectrum 4 potential energy, electromagnetic radiation, electromagnetic spectrum (including ultraviolet 2.3 Absorption spectra 4 and infrared), electronvolt, energy conservation, force, frequency the grating relation 2.4 Summary of Section 2 5 λ2 2 1 1θ (n = d sin n), kinetic energy, molecule momentum, momentum conservation, Newton’s 3 The emission spectrum of laws of motion, orders of diffraction, wavelength. In addition, some familiarity with the use atomic hydrogen 5 of basic algebra, exponentials, graph plotting, logarithms and trigonometric functions will 3.1 The visible spectrum of atomic be assumed. If you are uncertain about any of these terms, review them now by reference to hydrogen; Balmer’s formula 6 the Glossary, which will also indicate where in FLAP they are developed. 3.2 The ultraviolet and infrared series of lines for hydrogen 6 Module summary 3.3 Summary of Section 3 7 1 The spectrum of a sample of electromagnetic radiation shows the way in which 4 Bohr’s model for the hydrogen atom 7 the energy carried by that radiation is distributed with respect to wavelength 4.1 The four postulates 7 (or frequency).
    [Show full text]
  • Electromagnetic Radiation Production of Light
    Electromagnetic Radiation Production of Light Full window version (looks a little nicer). Click <Back> button to get back to small framed version with content indexes. This material (and images) is copyrighted!. See my copyright notice for fair use practices. When light is passed through a prism or a diffraction grating to produce a spectrum, the type of spectrum you will see depends on what kind of object is producing the light: is it a thick or thin gas, is it hot or cool, is it a gas or a solid? There are two basic types of spectra: continuous spectrum (energy at all wavelengths) and discrete spectrum (energy at only certain wavelengths). Astronomers usually refer to the two types of discrete spectra: emission lines (bright lines) and absorption lines (dark lines in an otherwise continuous spectrum) as different types of spectra. Continuous Spectrum A rainbow is an example of a continuous spectrum. Most continuous spectra are from hot, dense objects like stars, planets, or moons. The continuous spectrum from these kinds of objects is also called a thermal spectrum, because hot, dense objects will emit electromagnetic radiation at all wavelengths or colors. Any solid, liquid and dense (thick) gas at a temperature above absolute zero will produce a thermal spectrum. A thermal spectrum is the simplest type of spectrum because its shape depends on only the temperature. A discrete spectrum is more complex because it depends on temperature and other things like the chemical composition of the object, the gas density, surface gravity, speed, etc. Exotic objects like neutron stars and black holes can produce another type of continuous spectrum called ``synchrotron spectrum'' from charged particles swirling around magnetic fields, but I will discuss them in another chapter later on.
    [Show full text]
  • Characteristic and Continuous X-Rays Jitender Singh| October 18, 2019
    Characteristic and Continuous X-rays Jitender Singh| www.concepts-of-physics.com October 18, 2019 1 Introduction HV • • The x-rays are produced in a Coolidge tube when a high energy −+ electron interacts with a heavy metal target. Anode e− +−• Cathode • The high energy electrons get decelerated by Coulomb’s in- LV teraction with the target atom. These decelerating electrons emit con- tinuous X-rays (or bremsstrahlung). When an electron loses its en- X-ray tire energy in a single Coulomb’s interaction then X-rays of minimum Figure 1: In Coolidge Tube, the intensity wavelength (cut-off wavelength) are emitted. of x-rays is controlled by the filament The cut-off wavelength of the continuous X-ray spectrum is related current/voltage (LV) and the frequency of x-rays is controlled by the accelerat- to the accelerating potential V of the Coolidge tube by ing voltage (HV). hc 12400 Target Nucleus • − lcut off = ≈ (Å/V). e eV V + Typically, accelerating voltage is a few thousand Volts and cut off • − wavelength is of the order of an Angstrom. The cut-off frequency e of continuous x-rays is given by ncut off = c/lcut off. The cutoff wave- length decreases when the accelerating potential of Coolidge tube is X-ray increased. The intensity of X-rays increases with an increase in ac- Figure 2: An electron decelerated by Coulomb’s interaction of target atom celerating potential as shown in the figure. The intensity of X-rays emits X-rays in the continuous spectrum. depends on multiple factors. Relative Intensity The high energy electrons also knock out an inner shell electron of 1.0 K a 50 kV the target atom.
    [Show full text]
  • The Spectrum of Atomic Hydrogen
    The Spectrum of Atomic Hydrogen For almost a century light emitted by the simplest of atoms has been the chief experimental basis for theories of the structure of matter. Exploration of the hydrogen spectrum continues, now aided by lasers by Theodor W. Hansch, Arthur L. Schawlow and George W. Series he spectrum of the hydrogen atom sorbed. glvmg rise to dark lines on a that he could account for the positions has proved to be the Rosetta stone bright background. of all the known lines by applying a sim­ Tof modern physics: once this pat­ Hydrogen is the simplest of atoms. be­ ple empirical formula. The entire set of tern of lines had been deciphered much ing made up of a single electron and a lines has since come to be known as the else could also be understood. Most no­ nucleus that consists of a single proton. Balmer series. Another group of lines. tably. it was largely the effort to explain and so it can be expected to have the the Lyman series. lies in the far ultravio­ the spectrum of light emitted by the hy­ simplest spectrum. The spectrum is not. let. and there are other series at longer drogen atom that inspired the laws of however. an easy one to record. The wavelengths. Within each series the in­ quantum mechanics. Those laws have most prominent line was detected in dividual lines are designated by Greek since been found to apply not only to 1853 by Anders Jonas Angstrom. (The letters. starting with the line of longest the hydrogen atom but also to other common unit for measuring wave­ wavelength.
    [Show full text]
  • The Formalism of Quantum Mechanics Relevant Sections in Text
    The formalism of quantum mechanics The formalism of quantum mechanics Relevant sections in text: Chapter 3 Now for some formalism::: We have now acquired a little familiarity with how quantum mechanics works via some simple examples. Our approach has been rather informal; we have not clearly stated the rules of the game. The situation is analogous to one way of studying Newtonian mechanics. In your first exposure to Newtonian mechanics you may have had the following experience. First, we introduce some basic concepts, such as vectors, force, acceleration, energy, etc. We learn, to some extent, how to use these concepts by studying some simple examples. Along the way, we state (perhaps without full generality) some of the key laws that are being used. Second, we make things a bit more systematic, e.g., by carefully stating Newton's laws. More or less, we have completed the first of the steps. Now we must complete the second step. To formulate the laws (or postulates) of quantum mechanics, we need to spend a little time giving some mathematical method to the madness we have been indulging in so far. In particular, we need to give a linear algebraic type of interpretation to the apparatus of wave functions, operators, expectation values, and so forth. We begin by developing a point of view in which states of the system are elements of a (very large) vector space. I assume that you are already familiar with the fundamentals of linear algebra (vector spaces, bases, linear transformations, eigenvalue problems, etc. ). If you need some remedial work, have a look at the first section of chapter 3 in the text.
    [Show full text]