Theoretical and experimental justification for the Schrödinger equation
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The theoretical and experimental justification for the Schrödinger equation motivates the discovery of the
Schrödinger equation The Schrödinger equation is a linear partial differential equation that governs the wave function of a quantum-mechanical system. It is a key result in quantum mechanics, and its discovery was a significant landmark in the development of the ...
, the equation that describes the dynamics of nonrelativistic particles. The motivation uses
photon A photon () is an elementary particle that is a quantum of the electromagnetic field, including electromagnetic radiation such as light and radio waves, and the force carrier for the electromagnetic force. Photons are massless, so they always ...
s, which are
relativistic particle A relativistic particle is a particle which moves with a relativistic speed; that is, a speed comparable to the speed of light. This is achieved by photons to the extent that effects described by special relativity are able to describe those of su ...
s with dynamics described by
Maxwell's equations Maxwell's equations, or Maxwell–Heaviside equations, are a set of coupled partial differential equations that, together with the Lorentz force law, form the foundation of classical electromagnetism, classical optics, and electric circuits. ...
, as an analogue for all types of particles.


Classical electromagnetic waves


Nature of light

The
quantum In physics, a quantum (plural quanta) is the minimum amount of any physical entity (physical property) involved in an interaction. The fundamental notion that a physical property can be "quantized" is referred to as "the hypothesis of quantizati ...
particle of light is called a
photon A photon () is an elementary particle that is a quantum of the electromagnetic field, including electromagnetic radiation such as light and radio waves, and the force carrier for the electromagnetic force. Photons are massless, so they always ...
. Light has both a wave-like and a
particle In the Outline of physical science, physical sciences, a particle (or corpuscule in older texts) is a small wikt:local, localized physical body, object which can be described by several physical property, physical or chemical property, chemical ...
-like nature. In other words, light can appear to be made of photons (particles) in some experiments and light can act like waves in other experiments. The dynamics of classical electromagnetic waves are completely described by
Maxwell's equations Maxwell's equations, or Maxwell–Heaviside equations, are a set of coupled partial differential equations that, together with the Lorentz force law, form the foundation of classical electromagnetism, classical optics, and electric circuits. ...
, the classical description of electrodynamics. In the absence of sources, Maxwell's equations can be written as
wave equation The (two-way) wave equation is a second-order linear partial differential equation for the description of waves or standing wave fields — as they occur in classical physics — such as mechanical waves (e.g. water waves, sound waves and s ...
s in the electric and
magnetic field A magnetic field is a vector field that describes the magnetic influence on moving electric charges, electric currents, and magnetic materials. A moving charge in a magnetic field experiences a force perpendicular to its own velocity and to ...
vectors. Maxwell's equations thus describe, among other things, the wave-like properties of light. When "classical" (coherent or thermal) light is incident on a photographic plate or CCD, the average number of "hits", "dots", or "clicks" per unit time that result is approximately proportional to the square of the electromagnetic fields of the light. By ''formal analogy'', the wavefunction of a material particle can be used to find the probability density by taking its absolute-value squared. Unlike electromagnetic fields, quantum-mechanical wavefunctions are complex. (Often in the case of EM fields complex notation is used for convenience, but it is understood that in fact the fields are real. However, wavefunctions are genuinely complex.) Maxwell's equations were completely known by the latter part of the nineteenth century. The dynamical equations for light were, therefore, well-known long before the discovery of the photon. This is not true for other particles such as the
electron The electron ( or ) is a subatomic particle with a negative one elementary electric charge. Electrons belong to the first generation of the lepton particle family, and are generally thought to be elementary particles because they have no kn ...
. It was surmised from the interaction of light with atoms that electrons also had both a particle-like and a wave-like nature.
Newtonian mechanics Newton's laws of motion are three basic laws of classical mechanics that describe the relationship between the motion of an object and the forces acting on it. These laws can be paraphrased as follows: # A body remains at rest, or in motion ...
, a description of the particle-like behavior of macroscopic objects, failed to describe very small objects such as electrons.
Abductive reasoning Abductive reasoning (also called abduction,For example: abductive inference, or retroduction) is a form of logical inference formulated and advanced by American philosopher Charles Sanders Peirce beginning in the last third of the 19th century ...
was performed to obtain the dynamics of massive objects (particles with
mass Mass is an intrinsic property of a body. It was traditionally believed to be related to the quantity of matter in a physical body, until the discovery of the atom and particle physics. It was found that different atoms and different elementar ...
) such as electrons. The
electromagnetic wave equation The electromagnetic wave equation is a second-order partial differential equation that describes the propagation of electromagnetic waves through a medium or in a vacuum. It is a three-dimensional form of the wave equation. The homogeneous form ...
, the equation that described the dynamics of light, was used as a prototype for discovering the
Schrödinger equation The Schrödinger equation is a linear partial differential equation that governs the wave function of a quantum-mechanical system. It is a key result in quantum mechanics, and its discovery was a significant landmark in the development of the ...
, the equation that describes the wave-like and particle-like dynamics of nonrelativistic massive particles.


Plane sinusoidal waves


Electromagnetic wave equation

The electromagnetic wave equation describes the propagation of electromagnetic waves through a
medium Medium may refer to: Science and technology Aviation *Medium bomber, a class of war plane * Tecma Medium, a French hang glider design Communication * Media (communication), tools used to store and deliver information or data * Medium of ...
or in a
vacuum A vacuum is a space devoid of matter. The word is derived from the Latin adjective ''vacuus'' for "vacant" or "void". An approximation to such vacuum is a region with a gaseous pressure much less than atmospheric pressure. Physicists often dis ...
. The
homogeneous Homogeneity and heterogeneity are concepts often used in the sciences and statistics relating to the uniformity of a substance or organism. A material or image that is homogeneous is uniform in composition or character (i.e. color, shape, siz ...
form of the equation, written in terms of either the
electric field An electric field (sometimes E-field) is the physical field that surrounds electrically charged particles and exerts force on all other charged particles in the field, either attracting or repelling them. It also refers to the physical field fo ...
E or the
magnetic field A magnetic field is a vector field that describes the magnetic influence on moving electric charges, electric currents, and magnetic materials. A moving charge in a magnetic field experiences a force perpendicular to its own velocity and to ...
B, takes the form: : \nabla^2 \mathbf \ - \ \ \ = \ \ 0 : \nabla^2 \mathbf \ - \ \ \ = \ \ 0 where ''c'' is the
speed of light The speed of light in vacuum, commonly denoted , is a universal physical constant that is important in many areas of physics. The speed of light is exactly equal to ). According to the special theory of relativity, is the upper limit ...
in the medium. In a vacuum, c = 2.998 × 108 meters per second, which is the speed of light in
free space A vacuum is a space devoid of matter. The word is derived from the Latin adjective ''vacuus'' for "vacant" or "void". An approximation to such vacuum is a region with a gaseous pressure much less than atmospheric pressure. Physicists often dis ...
. The magnetic field is related to the electric field through Faraday's law ( cgs units) : \nabla \times \mathbf = - \frac .


Plane wave solution of the electromagnetic wave equation

The plane
sinusoidal A sine wave, sinusoidal wave, or just sinusoid is a mathematical curve defined in terms of the '' sine'' trigonometric function, of which it is the graph. It is a type of continuous wave and also a smooth periodic function. It occurs often in m ...
solution for an
electromagnetic wave In physics, electromagnetic radiation (EMR) consists of waves of the electromagnetic (EM) field, which propagate through space and carry momentum and electromagnetic radiant energy. It includes radio waves, microwaves, infrared, (visib ...
traveling in the z direction is ( cgs units and
SI units The International System of Units, known by the international abbreviation SI in all languages and sometimes Pleonasm#Acronyms and initialisms, pleonastically as the SI system, is the modern form of the metric system and the world's most wid ...
) \mathbf ( \mathbf , t ) = \left, \mathbf \ \operatorname \left \ \equiv \left, \mathbf \ \operatorname \left \ for the electric field and \mathbf ( \mathbf , t ) = \hat \times \mathbf ( \mathbf , t ) for the magnetic field, where ''k'' is the
wavenumber In the physical sciences, the wavenumber (also wave number or repetency) is the ''spatial frequency'' of a wave, measured in cycles per unit distance (ordinary wavenumber) or radians per unit distance (angular wavenumber). It is analogous to temp ...
, \omega = c k is the
angular frequency In physics, angular frequency "''ω''" (also referred to by the terms angular speed, circular frequency, orbital frequency, radian frequency, and pulsatance) is a scalar measure of rotation rate. It refers to the angular displacement per unit tim ...
of the wave, and c is the
speed of light The speed of light in vacuum, commonly denoted , is a universal physical constant that is important in many areas of physics. The speed of light is exactly equal to ). According to the special theory of relativity, is the upper limit ...
. The hats on the vectors indicate unit vectors in the x, y, and z directions. In complex notation, the quantity , \mathbf , is the
amplitude The amplitude of a periodic variable is a measure of its change in a single period (such as time or spatial period). The amplitude of a non-periodic signal is its magnitude compared with a reference value. There are various definitions of amplit ...
of the wave. Here , \zeta \rangle \equiv \begin \zeta_x \\ \zeta_y \end = \begin \cos(\theta) e^ \\ \sin(\theta) e^ \end is the
Jones vector In optics, polarized light can be described using the Jones calculus, discovered by R. C. Jones in 1941. Polarized light is represented by a Jones vector, and linear optical elements are represented by ''Jones matrices''. When light crosses an op ...
in the x-y plane. The notation for this vector is the
bra–ket notation In quantum mechanics, bra–ket notation, or Dirac notation, is used ubiquitously to denote quantum states. The notation uses angle brackets, and , and a vertical bar , to construct "bras" and "kets". A ket is of the form , v \rangle. Mathema ...
of
Dirac Distributed Research using Advanced Computing (DiRAC) is an integrated supercomputing facility used for research in particle physics, astronomy and cosmology in the United Kingdom. DiRAC makes use of multi-core processors and provides a variety of ...
, which is normally used in a quantum context. The quantum notation is used here in anticipation of the interpretation of the Jones vector as a quantum state vector. The angles \theta,\; \alpha_x,\; \text \; \alpha_y are the angle the electric field makes with the x axis and the two initial phases of the wave, respectively. The quantity , \phi \rangle = e^ , \zeta \rangle is the state vector of the wave. It describes the polarization of the wave and the spatial and temporal functionality of the wave. For a
coherent state In physics, specifically in quantum mechanics, a coherent state is the specific quantum state of the quantum harmonic oscillator, often described as a state which has dynamics most closely resembling the oscillatory behavior of a classical harmo ...
light beam so dim that its average photon number is much less than 1, this is approximately equivalent to the quantum state of a single photon.


Energy, momentum, and angular momentum of electromagnetic waves


Energy density of classical electromagnetic waves


Energy in a plane wave

The energy per unit volume in classical electromagnetic fields is (cgs units) : \mathcal_c = \frac \left \mathbf^2( \mathbf , t ) + \mathbf^2( \mathbf , t ) \right . For a plane wave, converting to complex notation (and hence dividing by a factor of 2), this becomes : \mathcal_c = \frac where the energy has been averaged over a wavelength of the wave.


Fraction of energy in each component

The fraction of energy in the x component of the plane wave (assuming linear polarization) is : f_x = \frac = \phi_x^*\phi_x with a similar expression for the y component. The fraction in both components is : \phi_x^*\phi_x + \phi_y^*\phi_y = \langle \phi , \phi\rangle = 1 .


Momentum density of classical electromagnetic waves

The momentum density is given by the
Poynting vector In physics, the Poynting vector (or Umov–Poynting vector) represents the directional energy flux (the energy transfer per unit area per unit time) or '' power flow'' of an electromagnetic field. The SI unit of the Poynting vector is the watt ...
: \boldsymbol = \mathbf( \mathbf, t ) \times \mathbf( \mathbf, t ) . For a sinusoidal plane wave traveling in the z direction, the momentum is in the z direction and is related to the energy density: : \mathcal c = \mathcal_c . The momentum density has been averaged over a wavelength.


Angular momentum density of classical electromagnetic waves

The angular momentum density is : \boldsymbol = \mathbf \times \boldsymbol = \mathbf \times \left \mathbf( \mathbf, t ) \times \mathbf( \mathbf, t ) \right . For a sinusoidal plane wave the angular momentum is in the z direction and is given by (going over to complex notation) : \mathcal = \left ( \mid \langle R , \phi\rangle \mid^2 - \mid \langle L , \phi\rangle \mid^2 \right ) = \mathcal_c \left ( \mid \phi_R \mid^2 - \mid \phi_L \mid^2 \right ) where again the density is averaged over a wavelength. Here right and left circularly polarized unit vectors are defined as : , R\rangle \equiv \begin 1 \\ i \end and : , L\rangle \equiv \begin 1 \\ -i \end .


Unitary operators and energy conservation

A wave can be transformed by, for example, passing through a
birefringent crystal Birefringence is the optical property of a material having a refractive index that depends on the polarization and propagation direction of light. These optically anisotropic materials are said to be birefringent (or birefractive). The birefring ...
or through slits in a
diffraction grating In optics, a diffraction grating is an optical component with a periodic structure that diffracts light into several beams travelling in different directions (i.e., different diffraction angles). The emerging coloration is a form of structura ...
. We can define the transformation of the state from the state at time t to the state at time (t + \tau) as : , \phi (t + \tau) \rangle = \hat(\tau) , \phi (t) \rangle . To conserve energy in the wave we require : \langle \phi (t + \tau), \phi (t + \tau) \rangle = \langle \phi(t) , \hat^(\tau) \hat(\tau) , \phi(t) \rangle = \langle \phi(t) , \phi(t) \rangle = 1 where U^ is the adjoint of U, the complex conjugate transpose of the matrix. This implies that a transformation that conserves energy must obey : \hat^ \hat = I where I is the identity operator and U is called a
unitary operator In functional analysis, a unitary operator is a surjective bounded operator on a Hilbert space that preserves the inner product. Unitary operators are usually taken as operating ''on'' a Hilbert space, but the same notion serves to define the con ...
. The unitary property is necessary to ensure
energy conservation Energy conservation is the effort to reduce wasteful energy consumption by using fewer energy services. This can be done by using energy more effectively (using less energy for continuous service) or changing one's behavior to use less service (f ...
in state transformations.


Hermitian operators and energy conservation

If \tau is an infinitesimal real quantity dt , then the unitary transformation is very close to the identity matrix (the final state is very close to the initial state) and can be written : \hat \approx I - i\hat\tau and the adjoint by : \hat^ \approx I + i\hat^\tau. The factor of ''i'' is introduced for convenience. With this convention, it will be shown that energy conservation requires H to be a Hermitian operator and that H is related to the energy of a particle. Energy conservation requires : I = \hat^ \hat \approx \left ( I + i\hat^\tau \right ) \left ( I - i\hat\tau \right ) \approx I + i\hat^\tau - i\hat\tau + \hat^\dagger \hat \tau^2 . Since \tau is infinitesimal, which means that \tau^2 may be neglected with respect to \tau, the last term can be omitted. Further, if ''H'' is equal to its adjoint: : \hat = \hat^ , it follows that (for infinitesimal translations in time \tau= dt\, ) : \hat^ \hat = I , so that, indeed, energy is conserved. Operators that are equal to their adjoints are called Hermitian or self-adjoint. The infinitesimal translation of the polarization state is : , \phi (t+dt) \rangle - , \phi (t) \rangle = -i\hat dt , \phi (t)\rangle . Thus, energy conservation requires that infinitesimal transformations of a polarization state occur through the action of a Hermitian operator. While this derivation is classical, the concept of a Hermitian operator generating energy-conserving infinitesimal transformations forms an important basis for quantum mechanics. The derivation of the Schrödinger equation follows directly from this concept.


Quantum analogy of classical electrodynamics

The treatment to this point has been classical. However, the quantum mechanical treatment of particles follows along lines ''formally analogous'' however, to
Maxwell's equations Maxwell's equations, or Maxwell–Heaviside equations, are a set of coupled partial differential equations that, together with the Lorentz force law, form the foundation of classical electromagnetism, classical optics, and electric circuits. ...
for electrodynamics. The analog of the classical "state vectors" \vert \phi \rangle in the classical description is quantum state vectors in the description of photons.


Energy, momentum, and angular momentum of photons


Energy

The early interpretation is based on the experiments of Max Planck and the interpretation of those experiments by
Albert Einstein Albert Einstein ( ; ; 14 March 1879 – 18 April 1955) was a German-born theoretical physicist, widely acknowledged to be one of the greatest and most influential physicists of all time. Einstein is best known for developing the theory ...
, which was that electromagnetic radiation is composed of irreducible packets of energy, known as
photon A photon () is an elementary particle that is a quantum of the electromagnetic field, including electromagnetic radiation such as light and radio waves, and the force carrier for the electromagnetic force. Photons are massless, so they always ...
s. The energy of each packet is related to the angular frequency of the wave by the relation \epsilon = \hbar \omega where \hbar is an experimentally determined quantity known as the reduced Planck's constant. If there are N photons in a box of volume V , the energy (neglecting
zero point energy Zero-point energy (ZPE) is the lowest possible energy that a quantum mechanical system may have. Unlike in classical mechanics, quantum systems constantly fluctuate in their lowest energy state as described by the Heisenberg uncertainty pr ...
) in the electromagnetic field is N \hbar \omega and the energy density is . The energy of a photon can be related to classical fields through the
correspondence principle In physics, the correspondence principle states that the behavior of systems described by the theory of quantum mechanics (or by the old quantum theory) reproduces classical physics in the limit of large quantum numbers. In other words, it says t ...
which states that for a large number of photons, the quantum and classical treatments must agree. Thus, for very large N , the quantum energy density must be the same as the classical energy density = \mathcal_c = \frac. The average number of photons in the box in a coherent state is then N = \frac \left, \mathbf \^2 .


Momentum

The correspondence principle also determines the momentum and angular momentum of the photon. For momentum \mathcal_c = = which implies that the momentum of a photon is \hbar k (or equivalently h \over \lambda ).


Angular momentum and spin

Similarly for the angular momentum \mathcal = \mathcal_c \left ( \left, \psi_R \^2 - \left, \psi_L \^2 \right ) = \left ( \left, \psi_R \^2 - \left, \psi_L \^2 \right ) which implies that the angular momentum of the photon is l_z = \hbar \left ( \left, \psi_R \^2 - \left, \psi_L \^2 \right ) . the quantum interpretation of this expression is that the photon has a probability of \left, \psi_R \^2 of having an angular momentum of \hbar and a probability of \left, \psi_L \^2 of having an angular momentum of -\hbar . We can therefore think of the angular momentum of the photon being quantized as well as the energy. This has indeed been experimentally verified. Photons have only been observed to have angular momenta of \pm \hbar .


=Spin operator

= The
spin Spin or spinning most often refers to: * Spinning (textiles), the creation of yarn or thread by twisting fibers together, traditionally by hand spinning * Spin, the rotation of an object around a central axis * Spin (propaganda), an intentionally b ...
of the photon is defined as the coefficient of \hbar in the angular momentum calculation. A photon has spin 1 if it is in the , R \rangle state and -1 if it is in the , L \rangle state. The spin operator is defined as the
outer product In linear algebra, the outer product of two coordinate vector In linear algebra, a coordinate vector is a representation of a vector as an ordered list of numbers (a tuple) that describes the vector in terms of a particular ordered basis. An ea ...
\hat \equiv , R\rangle \langle R , - , L\rangle \langle L , = \begin 0 & -i \\ i & 0 \end. The eigenvectors of the spin operator are , R\rangle and , L\rangle with
eigenvalue In linear algebra, an eigenvector () or characteristic vector of a linear transformation is a nonzero vector that changes at most by a scalar factor when that linear transformation is applied to it. The corresponding eigenvalue, often denoted b ...
s 1 and -1, respectively. The expected value of a spin measurement on a photon is then \langle \psi , \hat , \psi\rangle = \left, \psi_R \^2 - \left, \psi_L \^2. An operator S has been associated with an observable quantity, the angular momentum. The eigenvalues of the operator are the allowed observable values. This has been demonstrated for angular momentum, but it is in general true for any observable quantity.


Probability for a single photon

There are two ways in which probability can be applied to the behavior of photons; probability can be used to calculate the probable number of photons in a particular state, or probability can be used to calculate the likelihood of a single photon to be in a particular state. The former interpretation is applicable to thermal or to coherent light (see Quantum optics). The latter interpretation is the option for a single-photon Fock state. Dirac explains this This explanation is in some sense antiquated or even obsolete, as we now know that the concept of a single-photon wavefunction is disputed
/sup>, that in a
coherent state In physics, specifically in quantum mechanics, a coherent state is the specific quantum state of the quantum harmonic oscillator, often described as a state which has dynamics most closely resembling the oscillatory behavior of a classical harmo ...
one indeed deals with the probable number of photons, given by coherent-state Poissonian statistics, and that different photons can indeed interfere
/sup>.
in the context of the
double-slit experiment In modern physics, the double-slit experiment is a demonstration that light and matter can display characteristics of both classically defined waves and particles; moreover, it displays the fundamentally probabilistic nature of quantum mechanics ...
:


Probability amplitudes

The probability for a photon to be in a particular polarization state depends on the probability distribution over the fields as calculated by the classical Maxwell's equations (in the Glauber-Sudarshan P-representation of a one-photon Fock state.) The expectation value of the photon number in a coherent state in a limited region of space is quadratic in the fields. In quantum mechanics, by analogy, the state or probability amplitude of a single particle contains the basic probability information. In general, the rules for combining probability amplitudes look very much like the classical rules for composition of probabilities: (The following quote is from Baym, Chapter 1)
# The probability amplitude for two successive probabilities is the product of amplitudes for the individual possibilities. ... # The amplitude for a process that can take place in one of several indistinguishable ways is the sum of amplitudes for each of the individual ways. ... # The total probability for the process to occur is the absolute value squared of the total amplitude calculated by 1 and 2.


de Broglie waves

In 1923 Louis de Broglie addressed the question of whether all particles can have both a wave and a particle nature similar to the photon. Photons differ from many other particles in that they are massless and travel at the speed of light. Specifically de Broglie asked the question of whether a particle that has both a wave and a particle associated with it is consistent with Einstein's two great 1905 contributions, the
special theory of relativity In physics, the special theory of relativity, or special relativity for short, is a scientific theory regarding the relationship between Spacetime, space and time. In Albert Einstein's original treatment, the theory is based on two Postulates of ...
and the quantization of energy and momentum. The answer turned out to be positive. The wave and particle nature of electrons was experimentally observed in 1927, two years after the discovery of the Schrödinger equation.


de Broglie hypothesis

De Broglie supposed that every particle was associated with both a particle and a wave. The angular frequency \omega and wavenumber k of the wave was related to the energy E and momentum p of the particle by E = \hbar \omega and p = \hbar k . The question reduces to whether every observer in every inertial reference frame can agree on the phase of the wave. If so, then a wave-like description of particles may be consistent with special relativity.


Rest frame

First consider the rest frame of the particle. In that case the frequency and wavenumber of the wave are related to the energy and momentum of the particles properties by E_0 = mc^2 = \hbar \omega_0 and p_0 = 0 = \hbar k_0 where ''m'' is the rest mass of the particle. This describes a wave of infinite wavelength and infinite
phase velocity The phase velocity of a wave is the rate at which the wave propagates in any medium. This is the velocity at which the phase of any one frequency component of the wave travels. For such a component, any given phase of the wave (for example, ...
v_ = . The wave may be written as proportional to \cos(\omega_0 t) . This, however, is also the solution for a
simple harmonic oscillator In mechanics and physics, simple harmonic motion (sometimes abbreviated ) is a special type of periodic motion of a body resulting from a dynamic equilibrium between an inertial force, proportional to the acceleration of the body away from the ...
, which can be thought of as a clock in the rest frame of the particle. We can imagine a clock ticking at the same frequency as the wave is oscillating. The phases of the wave and the clock can be synchronized.


Frame of the observer

It is shown that the phase of the wave in an observer frame is the same as the phase of the wave in a particle frame, and also the same as clocks in the two frames. There is, therefore, consistency of both a wave-like and a particle-like picture in special relativity.


=Phase of the observer clock

= In the frame of an observer moving at relative speed v with respect to the particle, the particle clock is observed to tick at a frequency \omega_c = where \gamma = is a Lorentz factor that describes time dilation of the particle clock as observed by the observer. The phase of the observer clock is \omega_c t = ( \gamma t_0 ) = \omega_0 t_0 where t_0 is time measured in the particle frame. Both the observer clock and the particle clock agree on the phase.


=Phase of the observer wave

= The frequency and wavenumber of the wave in the observer frame is given by E = \gamma m_o c^2 = \hbar \omega = \gamma \hbar \omega_o and \vec = \gamma m_o \vec = \hbar \vec = \frac with a phase velocity v_ = = = . The phase of the wave in the observer frame is \omega t - k x = \omega t - vt = \omega t \left ( 1- \right ) = = (\gamma t_o ) = \omega_o t_o = \omega_c t. The phase of the wave in the observer frame is the same as the phase in the particle frame, as the clock in the particle frame, and the clock in the observer frame. A wave-like picture of particles is thus consistent with special relativity. In fact, we now know that these relations can be succinctly written using special relativistic
4-vector In special relativity, a four-vector (or 4-vector) is an object with four components, which transform in a specific way under Lorentz transformations. Specifically, a four-vector is an element of a four-dimensional vector space considered as a ...
notation: The relevant four-vectors are: *
Four-position In special relativity, a four-vector (or 4-vector) is an object with four components, which transform in a specific way under Lorentz transformations. Specifically, a four-vector is an element of a four-dimensional vector space considered as a r ...
\mathbf = (ct,\vec) * Four-velocity \mathbf = \gamma (c,\vec) *
Four-momentum In special relativity, four-momentum (also called momentum-energy or momenergy ) is the generalization of the classical three-dimensional momentum to four-dimensional spacetime. Momentum is a vector in three dimensions; similarly four-momentum is ...
\mathbf = \left(\frac,\vec\right) * Four-wavevector \mathbf = \left(\frac,\vec\right) = \left(\frac, \frac \hat\right) The relations between the four-vectors are as follows: * \mathbf = \frac * \mathbf = \hbar \mathbf = m_o \mathbf *\mathbf = \left(\frac\right) \mathbf = \left(\frac\right)\mathbf The phase of the wave is the relativistic invariant: \mathbf \cdot \mathbf = \omega t - \vec \cdot \vec = \omega_o t_o = \omega_o \tau


Bohr atom


Inconsistency of observation with classical physics

The de Broglie hypothesis helped resolve outstanding issues in atomic physics.
Classical physics Classical physics is a group of physics theories that predate modern, more complete, or more widely applicable theories. If a currently accepted theory is considered to be modern, and its introduction represented a major paradigm shift, then the ...
was unable to explain the observed behaviour of electrons in atoms. Specifically, accelerating electrons emit electromagnetic radiation according to the
Larmor formula In electrodynamics, the Larmor formula is used to calculate the total power radiated by a nonrelativistic point charge as it accelerates. It was first derived by J. J. Larmor in 1897, in the context of the wave theory of light. When any charged ...
. Electrons orbiting a nucleus should lose energy to radiation and eventually spiral into the nucleus. This is not observed. Atoms are stable on timescales much longer than predicted by the classical Larmor formula. Also, it was noted that excited atoms emit radiation with discrete frequencies. Einstein used this fact to interpret discrete energy packets of light as, in fact, real particles. If these real particles are emitted from atoms in discrete energy packets, however, must the emitters, the electrons, also change energy in discrete energy packets? There is nothing in
Newtonian mechanics Newton's laws of motion are three basic laws of classical mechanics that describe the relationship between the motion of an object and the forces acting on it. These laws can be paraphrased as follows: # A body remains at rest, or in motion ...
that explains this. The de Broglie hypothesis helped explain these phenomena by noting that the only allowed states for an electron orbiting an atom are those that allow for standing waves associated with each electron.


Balmer series

The Balmer series identifies those frequencies of light that can be emitted from an excited hydrogen atom: : \hbar \omega_n = R \left(\frac - \frac\right) \quad n=3,4,5,\dots where R is known as the Rydberg constant and is equal to 13.6 electron volts.


Assumptions of the Bohr model

The Bohr model, introduced in 1913, was an attempt to provide a theoretical basis for the Balmer series. The assumptions of the model are: # The orbiting electrons existed in circular orbits that had discrete quantized energies. That is, not every orbit is possible but only certain specific ones. # The laws of
classical mechanics Classical mechanics is a physical theory describing the motion of macroscopic objects, from projectiles to parts of machinery, and astronomical objects, such as spacecraft, planets, stars, and galaxies. For objects governed by classical ...
do not apply when electrons make the jump from one allowed orbit to another. # When an electron makes a jump from one orbit to another the energy difference is carried off (or supplied) by a single quantum of light (called a
photon A photon () is an elementary particle that is a quantum of the electromagnetic field, including electromagnetic radiation such as light and radio waves, and the force carrier for the electromagnetic force. Photons are massless, so they always ...
) which has an energy equal to the energy difference between the two orbitals. # The allowed orbits depend on quantized (discrete) values of orbital
angular momentum In physics, angular momentum (rarely, moment of momentum or rotational momentum) is the rotational analog of linear momentum. It is an important physical quantity because it is a conserved quantity—the total angular momentum of a closed syst ...
, ''L'' according to the equation L = n \hbar where ''n'' = 1,2,3,... and is called the principal quantum number.


Implications of the Bohr model

In a circular orbit the
centrifugal force In Newtonian mechanics, the centrifugal force is an inertial force (also called a "fictitious" or "pseudo" force) that appears to act on all objects when viewed in a rotating frame of reference. It is directed away from an axis which is paralle ...
balances the attractive force of the electron : = where m is the mass of the electron, v is the speed of the electron, r is the radius of the orbit and : = where e is the charge on the electron or proton. The energy of the orbiting electron is : E = m v^2 - = - which follows from the centrifugal force expression. The angular momentum assumption of the Bohr model implies : L = mvr = n \hbar which implies that, when combined with the centrifugal force equation, the radius of the orbit is given by : r= . This implies, from the energy equation, : E_n = - = - \left ( \right ) . The difference between energy levels recovers the Balmer series.


De Broglie's contribution to the Bohr model

The Bohr assumptions recover the observed Balmer series. The Bohr assumptions themselves, however, are not based on any more general theory. Why, for instance, should the allowed orbits depend on the angular momentum? The de Broglie hypothesis provides some insight. If we assume that the electron has a momentum given by : p = mv = \hbar k as postulated by the de Broglie hypothesis, then the angular momentum is given by : L = mvr = \hbar k r = \hbar \left ( \right ) r where \lambda is the wavelength of the electron wave. If only standing electron waves are permitted in the atom then only orbits with perimeters equal to integral numbers of wavelengths are allowed: : \lambda = . This implies that allowed orbits have angular momentum : L = n\hbar which is Bohr's fourth assumption. Assumptions one and two immediately follow. Assumption three follows from energy conservation, which de Broglie showed was consistent with the wave interpretation of particles.


Need for dynamical equations

The problem with the de Broglie hypothesis as applied to the Bohr atom is that we have forced a plane wave solution valid in empty space to a situation in which there is a strong attractive potential. We have not yet discovered the general dynamic equation for the evolution of electron waves. The Schrödinger equation is the immediate generalization of the de Broglie hypothesis and the dynamics of the photon.


Schrödinger equation


Analogy with photon dynamics

The dynamics of a photon are given by : , \phi (t+dt) \rangle - , \phi (t) \rangle = - i\hat dt , \phi (t)\rangle where H is a Hermitian operator determined by Maxwell's equations. The Hermiticity of the operator ensures that energy is conserved. Erwin Schrödinger assumed that the dynamics for massive particles were of the same form as the energy-conserving photon dynamics. : , \psi (t+dt) \rangle - , \psi (t) \rangle = - i\hat dt , \psi (t)\rangle where , \psi (t) \rangle is the state vector for the particle and H is now an unknown Hermitian operator to be determined.


Particle state vector

Rather than polarization states as in the photon case, Schrödinger assumed the state of the vector depended on the position of the particle. If a particle lives in one spatial dimension, then he divided the line up into an infinite number of small bins of length \lambda and assigned a component of the state vector to each bin : , \psi (t)\rangle \equiv \begin \vdots \\ \psi_(t) \\ \psi_j(t) \\ \psi_(t) \\ \vdots \end . The subscript j identifies the bin.


Matrix form and transition amplitudes

The transition equation can be written in matrix form as : \psi_j(t+dt)^ - \psi_j(t) = -i \sum_k^ H_ \, dt \, \psi_k(t) . The Hermitian condition requires : H_ = H^*_ . Schrödinger assumed that probability could only leak into adjacent bins during the small time step dt. In other words, all components of H are zero except for transitions between neighboring bins : H_^ \ne 0 , : H_^ \ne 0 . Moreover, it is assumed that space is uniform in that all transitions to the right are equal : H_^ = H_^ \equiv H_R . The same is true for transitions to the left : H_^ = H_^ \equiv H_L . The transition equation becomes : i = H_ \psi_(t) - H_ \psi_(t) + H_ \psi_(t) - H_ \psi_(t) + H_ \psi_(t) . The first term on the right side represents the movement of probability amplitude into bin j from the right. The second term represents leakage of probability from bin j to the right. The third term represents leakage of probability into bin j from the left. The fourth term represents leakage from bin j to the left. The final term represents any change of phase in the probability amplitude in bin j. If we expand the probability amplitude to second order in the bin size \lambda and assume space is isotropic, H_R =H_L \equiv H_0 the transition equation reduces to : i = H_ + H_ \psi_(t) .


Schrödinger equation in one dimension

The transition equation must be consistent with the de Broglie hypothesis. In free space the probability amplitude for the de Broglie wave is proportional to : \exp \left i\left ( k x - \omega t \right ) \right where : E = \hbar \omega = = in the non-relativistic limit. The de Broglie solution for free space is a solution of the transition equation if we require : H_0 \lambda^2 = - and : H_^ = 0^ . The time derivative term in the transition equation can be identified with the energy of the de Broglie wave. The spatial derivative term can be identified with the kinetic energy. This suggests that the term containing H_ is proportional to the potential energy. This yields the Schrödinger equation : i\hbar = -\frac \frac + U(x) \psi (x, t) where U is the classical potential energy and : \psi (x, t) \equiv \psi_j (t) and : 1 = \int_^ \psi^* (x, t) \psi (x, t) dx .


Schrödinger equation in three dimensions

In three dimensions the Schrödinger equation becomes : -\frac + U \psi = i\hbar \psi


Hydrogen atom

The solution for the hydrogen atom describes standing waves of energy exactly given by the Balmer series. This was a spectacular validation of the Schrödinger equation and of the wave-like behaviour of matter.


See also

* Introduction to quantum mechanics *
Angular frequency In physics, angular frequency "''ω''" (also referred to by the terms angular speed, circular frequency, orbital frequency, radian frequency, and pulsatance) is a scalar measure of rotation rate. It refers to the angular displacement per unit tim ...
* Dirac equation * Path integral formulation * Photoelectric effect * Photon polarization * Quantum electrodynamics *
Relation between Schrödinger's equation and the path integral formulation of quantum mechanics This article relates the Schrödinger equation with the path integral formulation of quantum mechanics using a simple nonrelativistic one-dimensional single-particle Hamiltonian composed of kinetic and potential energy. Background Schrödinger's ...
* Stern–Gerlach experiment *
Wave–particle duality Wave–particle duality is the concept in quantum mechanics that every particle or quantum entity may be described as either a particle or a wave. It expresses the inability of the classical concepts "particle" or "wave" to fully describe the ...


Notes


References

* * * {{DEFAULTSORT:Theoretical and experimental justification for the Schrodinger equation Partial differential equations Schrödinger equation