# Glossary

- Page ID
- 29441

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Words (or words that have the same definition) | The definition is case sensitive | (Optional) Image to display with the definition [Not displayed in Glossary, only in pop-up on pages] | (Optional) Caption for Image | (Optional) External or Internal Link | (Optional) Source for Definition |
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(Eg. "Genetic, Hereditary, DNA ...") | (Eg. "Relating to genes or heredity") | The infamous double helix | https://bio.libretexts.org/ | CC-BY-SA; Delmar Larsen |

Word(s) |
Definition |
Image | Caption | Link | Source |
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width of the central peak | angle between the minimum for \(\displaystyle m=1\) and \(\displaystyle m=−1\) | OpenStax | |||

two-slit diffraction pattern | diffraction pattern of two slits of width a that are separated by a distance d is the interference pattern of two point sources separated by d multiplied by the diffraction pattern of a slit of width a |
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resolution | ability, or limit thereof, to distinguish small details in images | OpenStax | |||

Rayleigh criterion | two images are just-resolvable when the center of the diffraction pattern of one is directly over the first minimum of the diffraction pattern of the other | OpenStax | |||

missing order | interference maximum that is not seen because it coincides with a diffraction minimum | OpenStax | |||

holography | process of producing holograms with the use of lasers | OpenStax | |||

hologram | three-dimensional image recorded on film by lasers; the word hologram means entire picture (from the Greek word holo, as in holistic) | OpenStax | |||

diffraction limit | fundamental limit to resolution due to diffraction | OpenStax | |||

diffraction grating | large number of evenly spaced parallel slits | OpenStax | |||

diffraction | bending of a wave around the edges of an opening or an obstacle | OpenStax | |||

destructive interference for a single slit | occurs when the width of the slit is comparable to the wavelength of light illuminating it | OpenStax | |||

Bragg planes | families of planes within crystals that can give rise to X-ray diffraction | OpenStax | |||

coherent waves | waves are in phase or have a definite phase relationship | OpenStax | |||

fringes | bright and dark patterns of interference | OpenStax | |||

incoherent | waves have random phase relationships | OpenStax | |||

interferometer | instrument that uses interference of waves to make measurements | OpenStax | |||

monochromatic | light composed of one wavelength only | OpenStax | |||

Newton’s rings | circular interference pattern created by interference between the light reflected off two surfaces as a result of a slight gap between them | OpenStax | |||

order | integer m used in the equations for constructive and destructive interference for a double slit | OpenStax | |||

principal maximum | brightest interference fringes seen with multiple slits | OpenStax | |||

secondary maximum | bright interference fringes of intensity lower than the principal maxima | OpenStax | |||

aberration | distortion in an image caused by departures from the small-angle approximation | OpenStax | |||

accommodation | use of the ciliary muscles to adjust the shape of the eye lens for focusing on near or far objects | OpenStax | |||

angular magnification | ratio of the angle subtended by an object observed with a magnifier to that observed by the naked eye | OpenStax | |||

apparent depth | depth at which an object is perceived to be located with respect to an interface between two media | OpenStax | |||

Cassegrain design | arrangement of an objective and eyepiece such that the light-gathering concave mirror has a hole in the middle, and light then is incident on an eyepiece lens | OpenStax | |||

charge-coupled device (CCD) | semiconductor chip that converts a light image into tiny pixels that can be converted into electronic signals of color and intensity | OpenStax | |||

coma | similar to spherical aberration, but arises when the incoming rays are not parallel to the optical axis | OpenStax | |||

compound microscope | microscope constructed from two convex lenses, the first serving as the eyepiece and the second serving as the objective lens | OpenStax | |||

concave mirror | spherical mirror with its reflecting surface on the inner side of the sphere; the mirror forms a “cave” | OpenStax | |||

converging (or convex) lens | lens in which light rays that enter it parallel converge into a single point on the opposite side | OpenStax | |||

convex mirror | spherical mirror with its reflecting surface on the outer side of the sphere | OpenStax | |||

curved mirror | mirror formed by a curved surface, such as spherical, elliptical, or parabolic | OpenStax | |||

diverging (or concave) lens | lens that causes light rays to bend away from its optical axis | OpenStax | |||

eyepiece | lens or combination of lenses in an optical instrument nearest to the eye of the observer | OpenStax | |||

far point | furthest point an eye can see in focus | OpenStax | |||

farsightedness (or hyperopia) | visual defect in which near objects appear blurred because their images are focused behind the retina rather than on the retina; a farsighted person can see far objects clearly but near objects appear blurred | OpenStax | |||

first focus or object focus | object located at this point will result in an image created at infinity on the opposite side of a spherical interface between two media | OpenStax | |||

focal length | distance along the optical axis from the focal point to the optical element that focuses the light rays | OpenStax | |||

focal plane | plane that contains the focal point and is perpendicular to the optical axis | OpenStax | |||

focal point | for a converging lens or mirror, the point at which converging light rays cross; for a diverging lens or mirror, the point from which diverging light rays appear to originate | OpenStax | |||

image distance | distance of the image from the central axis of the optical element that produces the image | OpenStax | |||

linear magnification | ratio of image height to object height | OpenStax | |||

magnification | ratio of image size to object size | OpenStax | |||

near point | closest point an eye can see in focus | OpenStax | |||

nearsightedness (or myopia) | visual defect in which far objects appear blurred because their images are focused in front of the retina rather than on the retina; a nearsighted person can see near objects clearly but far objects appear blurred | OpenStax | |||

net magnification | (MnetMnet) of the compound microscope is the product of the linear magnification of the objective and the angular magnification of the eyepiece | OpenStax | |||

Newtonian design | arrangement of an objective and eyepiece such that the focused light from the concave mirror was reflected to one side of the tube into an eyepiece | OpenStax | |||

object distance |
distance of the object from the central axis of the optical element that produces its image |
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objective | lens nearest to the object being examined. | OpenStax | |||

optical axis | axis about which the mirror is rotationally symmetric; you can rotate the mirror about this axis without changing anything | OpenStax | |||

optical power | (P) inverse of the focal length of a lens, with the focal length expressed in meters. The optical power P of a lens is expressed in units of diopters D; that is, \(\displaystyle 1D=1/m=1m^{−1}\) | OpenStax | |||

plane mirror | plane (flat) reflecting surface | OpenStax | |||

ray tracing | technique that uses geometric constructions to find and characterize the image formed by an optical system | OpenStax | |||

real image | image that can be projected onto a screen because the rays physically go through the image | OpenStax | |||

second focus or image focus | for a converging interface, the point where a bundle of parallel rays refracting at a spherical interface; for a diverging interface, the point at which the backward continuation of the refracted rays will converge between two media will focus | OpenStax | |||

simple magnifier (or magnifying glass) | converging lens that produces a virtual image of an object that is within the focal length of the lens | OpenStax | |||

small-angle approximation | approximation that is valid when the size of a spherical mirror is significantly smaller than the mirror’s radius; in this approximation, spherical aberration is negligible and the mirror has a well-defined focal point | OpenStax | |||

spherical aberration | distortion in the image formed by a spherical mirror when rays are not all focused at the same point | OpenStax | |||

thin-lens approximation | assumption that the lens is very thin compared to the first image distance | OpenStax | |||

vertex | point where the mirror’s surface intersects with the optical axis | OpenStax | |||

virtual image | image that cannot be projected on a screen because the rays do not physically go through the image, they only appear to originate from the image | OpenStax | |||

birefringent | refers to crystals that split an unpolarized beam of light into two beams | OpenStax | |||

Brewster’s angle | angle of incidence at which the reflected light is completely polarized | OpenStax | |||

Brewster’s law | \(\displaystyle tanθ_b=\frac{n_2}{n_1}\), where \(\displaystyle n_1\) is the medium in which the incident and reflected light travel and \(\displaystyle n_2\) is the index of refraction of the medium that forms the interface that reflects the light | OpenStax | |||

corner reflector | object consisting of two (or three) mutually perpendicular reflecting surfaces, so that the light that enters is reflected back exactly parallel to the direction from which it came | OpenStax | |||

critical angle | incident angle that produces an angle of refraction of 90° | OpenStax | |||

direction of polarization | direction parallel to the electric field for EM waves | OpenStax | |||

dispersion | spreading of light into its spectrum of wavelengths | OpenStax | |||

geometric optics | part of optics dealing with the ray aspect of light | OpenStax | |||

horizontally polarized | oscillations are in a horizontal plane | OpenStax | |||

Huygens’s principle | every point on a wave front is a source of wavelets that spread out in the forward direction at the same speed as the wave itself; the new wave front is a plane tangent to all of the wavelets | OpenStax | |||

index of refraction | for a material, the ratio of the speed of light in a vacuum to that in a material | OpenStax | |||

law of reflection | angle of reflection equals the angle of incidence | OpenStax | |||

law of refraction | when a light ray crosses from one medium to another, it changes direction by an amount that depends on the index of refraction of each medium and the sines of the angle of incidence and angle of refraction | OpenStax | |||

Malus’s law | where \(\displaystyle I_0\) is the intensity of the polarized wave before passing through the filter | OpenStax | |||

optically active | substances that rotate the plane of polarization of light passing through them | OpenStax | |||

polarization | attribute that wave oscillations have a definite direction relative to the direction of propagation of the wave | OpenStax | |||

polarized | refers to waves having the electric and magnetic field oscillations in a definite direction | OpenStax | |||

ray | straight line that originates at some point | OpenStax | |||

refraction | changing of a light ray’s direction when it passes through variations in matter | OpenStax | |||

total internal reflection | phenomenon at the boundary between two media such that all the light is reflected and no refraction occurs | OpenStax | |||

unpolarized | refers to waves that are randomly polarized | OpenStax | |||

vertically polarized | oscillations are in a vertical plane | OpenStax | |||

wave optics | part of optics dealing with the wave aspect of light | OpenStax | |||

classical (Galilean) velocity addition | method of adding velocities when \(\displaystyle v<<c\); velocities add like regular numbers in one-dimensional motion: \(\displaystyle u=v+u'\), where v is the velocity between two observers, u is the velocity of an object relative to one observer, and \(\displaystyle u'\) is the velocity relative to the other observer | OpenStax | |||

event | occurrence in space and time specified by its position and time coordinates (x, y, z, t) measured relative to a frame of reference | OpenStax | |||

first postulate of special relativity | laws of physics are the same in all inertial frames of reference | OpenStax | |||

Galilean relativity | if an observer measures a velocity in one frame of reference, and that frame of reference is moving with a velocity past a second reference frame, an observer in the second frame measures the original velocity as the vector sum of these velocities | OpenStax | |||

Galilean transformation | relation between position and time coordinates of the same events as seen in different reference frames, according to classical mechanics | OpenStax | |||

inertial frame of reference | reference frame in which a body at rest remains at rest and a body in motion moves at a constant speed in a straight line unless acted on by an outside force | OpenStax | |||

length contraction | decrease in observed length of an object from its proper length \(\displaystyle L_0\) to length L when its length is observed in a reference frame where it is traveling at speed v | OpenStax | |||

Lorentz transformation | relation between position and time coordinates of the same events as seen in different reference frames, according to the special theory of relativity | OpenStax | |||

Michelson-Morley experiment | investigation performed in 1887 that showed that the speed of light in a vacuum is the same in all frames of reference from which it is viewed | OpenStax | |||

proper length | \(\displaystyle L_0\); the distance between two points measured by an observer who is at rest relative to both of the points; for example, earthbound observers measure proper length when measuring the distance between two points that are stationary relative to Earth | OpenStax | |||

proper time | \(\displaystyle Δτ\) is the time interval measured by an observer who sees the beginning and end of the process that the time interval measures occur at the same location | OpenStax | |||

relativistic kinetic energy | kinetic energy of an object moving at relativistic speeds | OpenStax | |||

relativistic momentum | \(\displaystyle \vec{p}\), the momentum of an object moving at relativistic velocity; \(\displaystyle \vec{p}=γm\vec{u}\) | OpenStax | |||

lativistic velocity addition | method of adding velocities of an object moving at a relativistic speeds | OpenStax | |||

rest energy | energy stored in an object at rest: \(\displaystyle E_0=mc^2\) | OpenStax | |||

rest frame | frame of reference in which the observer is at rest | OpenStax | |||

rest mass | mass of an object as measured by an observer at rest relative to the object | OpenStax | |||

second postulate of special relativity | light travels in a vacuum with the same speed c in any direction in all inertial frames | OpenStax | |||

special theory of relativity | theory that Albert Einstein proposed in 1905 that assumes all the laws of physics have the same form in every inertial frame of reference, and that the speed of light is the same within all inertial frames | OpenStax | |||

speed of light | ultimate speed limit for any particle having mass | OpenStax | |||

time dilation | lengthening of the time interval between two events when seen in a moving inertial frame rather than the rest frame of the events (in which the events occur at the same location) | OpenStax | |||

total energy | sum of all energies for a particle, including rest energy and kinetic energy, given for a particle of mass m and speed u by \(\displaystyle E=γmc^2\), where \(\displaystyle γ=\frac{1}{\sqrt{1−\frac{u^2}{c^2}}}\) | OpenStax | |||

world line | path through space-time | OpenStax | |||

absorber | any object that absorbs radiation | OpenStax | |||

absorption spectrum | wavelengths of absorbed radiation by atoms and molecules | OpenStax | |||

Balmer formula | describes the emission spectrum of a hydrogen atom in the visible-light range | OpenStax | |||

Balmer series | spectral lines corresponding to electron transitions to/from the \(\displaystyle n=2\) state of the hydrogen atom, described by the Balmer formula | OpenStax | |||

blackbody | perfect absorber/emitter | OpenStax | |||

blackbody radiation | radiation emitted by a blackbody | OpenStax | |||

Bohr radius of hydrogen | radius of the first Bohr’s orbit | OpenStax | |||

Bohr’s model of the hydrogen atom | first quantum model to explain emission spectra of hydrogen | OpenStax | |||

Brackett series | spectral lines corresponding to electron transitions to/from the \(\displaystyle n=4\) state | OpenStax | |||

Compton effect | the change in wavelength when an X-ray is scattered by its interaction with some materials | OpenStax | |||

Compton shift | difference between the wavelengths of the incident X-ray and the scattered X-ray | OpenStax | |||

Compton wavelength | physical constant with the value \(\displaystyle λ_c=2.43pm\) | OpenStax | |||

cut-off frequency | frequency of incident light below which the photoelectric effect does not occur | OpenStax | |||

cut-off wavelength | wavelength of incident light that corresponds to cut-off frequency | OpenStax | |||

Davisson–Germer experiment | historically first electron-diffraction experiment that revealed electron waves | OpenStax | |||

de Broglie wave | matter wave associated with any object that has mass and momentum | OpenStax | |||

de Broglie’s hypothesis of matter waves | particles of matter can behave like waves | OpenStax | |||

double-slit interference experiment | Young’s double-slit experiment, which shows the interference of waves | OpenStax | |||

electron microscopy | microscopy that uses electron waves to “see” fine details of nano-size objects | OpenStax | |||

emission spectrum | wavelengths of emitted radiation by atoms and molecules | OpenStax | |||

emitter | any object that emits radiation | OpenStax | |||

energy of a photon | quantum of radiant energy, depends only on a photon’s frequency | OpenStax | |||

energy spectrum of hydrogen | set of allowed discrete energies of an electron in a hydrogen atom | OpenStax | |||

excited energy states of the H atom | energy state other than the ground state | OpenStax | |||

Fraunhofer lines | dark absorption lines in the continuum solar emission spectrum | OpenStax | |||

ground state energy of the hydrogen atom | energy of an electron in the first Bohr orbit of the hydrogen atom | OpenStax | |||

group velocity | velocity of a wave, energy travels with the group velocity | OpenStax | |||

Heisenberg uncertainty principle | sets the limits on precision in simultaneous measurements of momentum and position of a particle | OpenStax | |||

Humphreys series | spectral lines corresponding to electron transitions to/from the \(\displaystyle n=6\) state | OpenStax | |||

hydrogen-like atom | ionized atom with one electron remaining and nucleus with charge \(\displaystyle +Ze\) | OpenStax | |||

inelastic scattering | scattering effect where kinetic energy is not conserved but the total energy is conserved | OpenStax | |||

ionization energy | energy needed to remove an electron from an atom | OpenStax | |||

ionization limit of the hydrogen atom | ionization energy needed to remove an electron from the first Bohr orbit | OpenStax | |||

Lyman series | spectral lines corresponding to electron transitions to/from the ground state | OpenStax | |||

nuclear model of the atom | heavy positively charged nucleus at the center is surrounded by electrons, proposed by Rutherford | OpenStax | |||

Paschen series | spectral lines corresponding to electron transitions to/from the \(\displaystyle n=3\) state | OpenStax | |||

Pfund series | spectral lines corresponding to electron transitions to/from the \(\displaystyle n=5\) state | OpenStax | |||

photocurrent | in a circuit, current that flows when a photoelectrode is illuminated | OpenStax | |||

photoelectric effect | emission of electrons from a metal surface exposed to electromagnetic radiation of the proper frequency | OpenStax | |||

photoelectrode | in a circuit, an electrode that emits photoelectrons | OpenStax | |||

photoelectron | electron emitted from a metal surface in the presence of incident radiation | OpenStax | |||

photon | particle of light | OpenStax | |||

Planck’s hypothesis of energy quanta | energy exchanges between the radiation and the walls take place only in the form of discrete energy quanta | OpenStax | |||

postulates of Bohr’s model | three assumptions that set a frame for Bohr’s model | OpenStax | |||

power intensity | energy that passes through a unit surface per unit time | OpenStax | |||

propagation vector | vector with magnitude \(\displaystyle 2π/λ\) that has the direction of the photon’s linear momentum | OpenStax | |||

quantized energies | discrete energies; not continuous | OpenStax | |||

quantum number | index that enumerates energy levels | OpenStax | |||

quantum phenomenon | in interaction with matter, photon transfers either all its energy or nothing | OpenStax | |||

quantum state of a Planck’s oscillator | any mode of vibration of Planck’s oscillator, enumerated by quantum number | OpenStax | |||

reduced Planck’s constant | Planck’s constant divided by \(\displaystyle 2π\) | OpenStax | |||

Rutherford’s gold foil experiment | first experiment to demonstrate the existence of the atomic nucleus | OpenStax | |||

Rydberg constant for hydrogen | physical constant in the Balmer formula | OpenStax | |||

Rydberg formula | experimentally found positions of spectral lines of hydrogen atom | OpenStax | |||

scattering angle | angle between the direction of the scattered beam and the direction of the incident beam | OpenStax | |||

Stefan–Boltzmann constant | physical constant in Stefan’s law | OpenStax | |||

stopping potential | in a circuit, potential difference that stops photocurrent | OpenStax | |||

wave number | magnitude of the propagation vector | OpenStax | |||

wave quantum mechanics | theory that explains the physics of atoms and subatomic particles | OpenStax | |||

wave-particle duality | particles can behave as waves and radiation can behave as particles | OpenStax | |||

work function | energy needed to detach photoelectron from the metal surface | OpenStax | |||

α-particle | doubly ionized helium atom | OpenStax | |||

α-ray | beam of \(\displaystyle α\)-particles (alpha-particles) | OpenStax | |||

β-ray | beam of electrons | OpenStax | |||

γ-ray | beam of highly energetic photons | OpenStax | |||

anti-symmetric function | odd function | OpenStax | |||

Born interpretation | states that the square of a wave function is the probability density | OpenStax | |||

complex function | function containing both real and imaginary parts | OpenStax | |||

Copenhagen interpretation | states that when an observer is not looking or when a measurement is not being made, the particle has many values of measurable quantities, such as position | OpenStax | |||

correspondence principle | in the limit of large energies, the predictions of quantum mechanics agree with the predictions of classical mechanics | OpenStax | |||

energy levels | states of definite energy, often represented by horizontal lines in an energy “ladder” diagram | OpenStax | |||

energy quantum number | index that labels the allowed energy states | OpenStax | |||

energy-time uncertainty principle | energy-time relation for uncertainties in the simultaneous measurements of the energy of a quantum state and of its lifetime | OpenStax | |||

even function | in one dimension, a function symmetric with the origin of the coordinate system | OpenStax | |||

expectation value | average value of the physical quantity assuming a large number of particles with the same wave function | OpenStax | |||

field emission | electron emission from conductor surfaces when a strong external electric field is applied in normal direction to conductor’s surface | OpenStax | |||

ground state energy | lowest energy state in the energy spectrum | OpenStax | |||

Heisenberg’s uncertainty principle | places limits on what can be known from a simultaneous measurements of position and momentum; states that if the uncertainty on position is small then the uncertainty on momentum is large, and vice versa | OpenStax | |||

infinite square well | potential function that is zero in a fixed range and infinitely beyond this range | OpenStax | |||

momentum operator | operator that corresponds to the momentum of a particle | OpenStax | |||

nanotechnology | technology that is based on manipulation of nanostructures such as molecules or individual atoms to produce nano-devices such as integrated circuits | OpenStax | |||

normalization condition | requires that the probability density integrated over the entire physical space results in the number one | OpenStax | |||

odd function | in one dimension, a function antisymmetric with the origin of the coordinate system | OpenStax | |||

position operator | operator that corresponds to the position of a particle | OpenStax | |||

potential barrier | potential function that rises and falls with increasing values of position | OpenStax | |||

principal quantum number | energy quantum number | OpenStax | |||

probability density | square of the particle’s wave function | OpenStax | |||

quantum dot | small region of a semiconductor nanocrystal embedded in another semiconductor nanocrystal, acting as a potential well for electrons | OpenStax | |||

quantum tunneling | phenomenon where particles penetrate through a potential energy barrier with a height greater than the total energy of the particles | OpenStax | |||

resonant tunneling | tunneling of electrons through a finite-height potential well that occurs only when electron energies match an energy level in the well, occurs in quantum dots | OpenStax | |||

resonant-tunneling diode | quantum dot with an applied voltage bias across it | OpenStax | |||

scanning tunneling microscope (STM) | device that utilizes quantum-tunneling phenomenon at metallic surfaces to obtain images of nanoscale structures | OpenStax | |||

Schrӧdinger’s time-dependent equation | equation in space and time that allows us to determine wave functions of a quantum particle | OpenStax | |||

Schrӧdinger’s time-independent equation | equation in space that allows us to determine wave functions of a quantum particle; this wave function must be multiplied by a time-modulation factor to obtain the time-dependent wave function | OpenStax | |||

standing wave state | stationary state for which the real and imaginary parts of Ψ(x,t)Ψ(x,t) oscillate up and down like a standing wave (often modeled with sine and cosine functions) | OpenStax | |||

state reduction | hypothetical process in which an observed or detected particle “jumps into” a definite state, often described in terms of the collapse of the particle’s wave function | OpenStax | |||

stationary state | state for which the probability density function, \(\displaystyle |Ψ(x,t)|^2\), does not vary in time | OpenStax | |||

time-modulation factor | factor \(\displaystyle e^{−iωt}\) that multiplies the time-independent wave function when the potential energy of the particle is time independent | OpenStax | |||

transmission probability | also called tunneling probability, the probability that a particle will tunnel through a potential barrier | OpenStax | |||

tunnel diode | electron tunneling-junction between two different semiconductors | OpenStax | |||

tunneling probability | also called transmission probability, the probability that a particle will tunnel through a potential barrier | OpenStax | |||

wave function | function that represents the quantum state of a particle (quantum system) | OpenStax | |||

wave function collapse | equivalent to state reduction | OpenStax | |||

wave packet | superposition of many plane matter waves that can be used to represent a localized particle | OpenStax | |||

angular momentum orbital quantum number (l) | quantum number associated with the orbital angular momentum of an electron in a hydrogen atom | OpenStax | |||

angular momentum projection quantum number (m) | quantum number associated with the z-component of the orbital angular momentum of an electron in a hydrogen atom | OpenStax | |||

atomic orbital | region in space that encloses a certain percentage (usually 90%) of the electron probability | OpenStax | |||

Bohr magneton | magnetic moment of an electron, equal to \(\displaystyle 9.3×10^{−24}J/T\) or \(\displaystyle 5.8×10^{−5}eV/T\) | OpenStax | |||

braking radiation | radiation produced by targeting metal with a high-energy electron beam (or radiation produced by the acceleration of any charged particle in a material) | OpenStax | |||

chemical group | group of elements in the same column of the periodic table that possess similar chemical properties | OpenStax | |||

coherent light | light that consists of photons of the same frequency and phase | OpenStax | |||

covalent bond | chemical bond formed by the sharing of electrons between two atoms | OpenStax | |||

electron configuration | representation of the state of electrons in an atom, such as \(\displaystyle 1s^22s^1\) for lithium | OpenStax | |||

fine structure | detailed structure of atomic spectra produced by spin-orbit coupling | OpenStax | |||

fluorescence | radiation produced by the excitation and subsequent, gradual de-excitation of an electron in an atom | OpenStax | |||

hyperfine structure | detailed structure of atomic spectra produced by spin-orbit coupling | OpenStax | |||

ionic bond | chemical bond formed by the electric attraction between two oppositely charged ions | OpenStax | |||

laser | coherent light produced by a cascade of electron de-excitations | OpenStax | |||

magnetic orbital quantum number | another term for the angular momentum projection quantum number | OpenStax | |||

magnetogram | pictoral representation, or map, of the magnetic activity at the Sun’s surface | OpenStax | |||

metastable state | state in which an electron “lingers” in an excited state | OpenStax | |||

monochromatic | light that consists of photons with the same frequency | OpenStax | |||

Moseley plot | plot of the atomic number versus the square root of X-ray frequency | OpenStax | |||

Moseley’s law | relationship between the atomic number and X-ray photon frequency for X-ray production | OpenStax | |||

Orbital magnetic dipole moment | measure of the strength of the magnetic field produced by the orbital angular momentum of the electron | OpenStax | |||

Pauli’s exclusion principle | no two electrons in an atom can have the same values for all four quantum numbers \(\displaystyle (n,l,m,ms)\) | OpenStax | |||

population inversion | condition in which a majority of atoms contain electrons in a metastable state | OpenStax | |||

principal quantum number (n) | quantum number associated with the total energy of an electron in a hydrogen atom | OpenStax | |||

radial probability density function | function use to determine the probability of a electron to be found in a spatial interval in r | OpenStax | |||

selection rules | rules that determine whether atomic transitions are allowed or forbidden (rare) | OpenStax | |||

spin projection quantum number (\(\displaystyle m_s\)) | quantum number associated with the z-component of the spin angular momentum of an electron | OpenStax | |||

spin quantum number (s) | quantum number associated with the spin angular momentum of an electron | OpenStax | |||

spin-flip transitions | atomic transitions between states of an electron-proton system in which the magnetic moments are aligned and not aligned | OpenStax | |||

spin-orbit coupling | interaction between the electron magnetic moment and the magnetic field produced by the orbital angular momentum of the electron | OpenStax | |||

stimulated emission | when a photon of energy triggers an electron in a metastable state to drop in energy emitting an additional photon | OpenStax | |||

transition metal | element that is located in the gap between the first two columns and the last six columns of the table of elements that contains electrons that fill the d subshell | OpenStax | |||

valence electron | electron in the outer shell of an atom that participates in chemical bonding | OpenStax | |||

Zeeman effect | splitting of energy levels by an external magnetic field | OpenStax | |||

acceptor impurity | atom substituted for another in a semiconductor that results in a free electron | OpenStax | |||

amplifier | electrical device that amplifies an electric signal | OpenStax | |||

base current | current drawn from the base n-type material in a transistor | OpenStax | |||

BCS theory | theory of superconductivity based on electron-lattice-electron interactions | OpenStax | |||

body-centered cubic (BCC) | crystal structure in which an ion is surrounded by eight nearest neighbors located at the corners of a unit cell | OpenStax | |||

breakdown voltage | in a diode, the reverse bias voltage needed to cause an avalanche of current | OpenStax | |||

collector current | current drawn from the collector p-type material | OpenStax | |||

conduction band | above the valence band, the next available band in the energy structure of a crystal | OpenStax | |||

Cooper pair | coupled electron pair in a superconductor | OpenStax | |||

covalent bond | bond formed by the sharing of one or more electrons between atoms | OpenStax | |||

critical magnetic field | maximum field required to produce superconductivity | OpenStax | |||

critical temperature | maximum temperature to produce superconductivity | OpenStax | |||

density of states | number of allowed quantum states per unit energy | OpenStax | |||

depletion layer | region near the p-n junction that produces an electric field | OpenStax | |||

dissociation energy | amount of energy needed to break apart a molecule into atoms; also, total energy per ion pair to separate the crystal into isolated ions | OpenStax | |||

donor impurity | atom substituted for another in a semiconductor that results in a free electron hole | OpenStax | |||

doping | alteration of a semiconductor by the substitution of one type of atom with another | OpenStax | |||

drift velocity | average velocity of a randomly moving particle | OpenStax | |||

electric dipole transition | transition between energy levels brought by the absorption or emission of radiation | OpenStax | |||

electron affinity | energy associated with an accepted (bound) electron | OpenStax | |||

electron number density | number of electrons per unit volume | OpenStax | |||

energy band | nearly continuous band of electronic energy levels in a solid | OpenStax | |||

energy gap | gap between energy bands in a solid | OpenStax | |||

equilibrium separation distance | distance between atoms in a molecule | OpenStax | |||

exchange symmetry | how a total wave function changes under the exchange of two electrons | OpenStax | |||

face-centered cubic (FCC) | crystal structure in which an ion is surrounded by six nearest neighbors located at the faces at the faces of a unit cell | OpenStax | |||

Fermi energy | largest energy filled by electrons in a metal at \(\displaystyle T=0K\) | OpenStax | |||

Fermi factor | number that expresses the probability that a state of given energy will be filled | OpenStax | |||

Fermi temperature | effective temperature of electrons with energies equal to the Fermi energy | OpenStax | |||

forward bias configuration | diode configuration that results in high current | OpenStax | |||

free electron model | model of a metal that views electrons as a gas | OpenStax | |||

hole | unoccupied states in an energy band | OpenStax | |||

hybridization | change in the energy structure of an atom in which energetically favorable mixed states participate in bonding | OpenStax | |||

impurity atom | acceptor or donor impurity atom | OpenStax | |||

impurity band | new energy band create by semiconductor doping | OpenStax | |||

ionic bond | bond formed by the Coulomb attraction of a positive and negative ions | OpenStax | |||

junction transistor | electrical valve based on a p-n-p junction | OpenStax | |||

lattice | regular array or arrangement of atoms into a crystal structure | OpenStax | |||

Madelung constant | constant that depends on the geometry of a crystal used to determine the total potential energy of an ion in a crystal | OpenStax | |||

majority carrier | free electrons (or holes) contributed by impurity atoms | OpenStax | |||

minority carrier | free electrons (or holes) produced by thermal excitations across the energy gap | OpenStax | |||

n-type semiconductor | doped semiconductor that conducts electrons | OpenStax | |||

p-n junction | junction formed by joining p- and n-type semiconductors | OpenStax | |||

p-type semiconductor | doped semiconductor that conducts holes | OpenStax | |||

polyatomic molecule | molecule formed of more than one atom | OpenStax | |||

repulsion constant | experimental parameter associated with a repulsive force between ions brought so close together that the exclusion principle is important | OpenStax | |||

reverse bias configuration | diode configuration that results in low current | OpenStax | |||

rotational energy level | energy level associated with the rotational energy of a molecule | OpenStax | |||

selection rule | rule that limits the possible transitions from one quantum state to another | OpenStax | |||

semiconductor | solid with a relatively small energy gap between the lowest completely filled band and the next available unfilled band | OpenStax | |||

simple cubic | basic crystal structure in which each ion is located at the nodes of a three-dimensional grid | OpenStax | |||

type I superconductor | superconducting element, such as aluminum or mercury | OpenStax | |||

type II superconductor | superconducting compound or alloy, such as a transition metal or an actinide series element | OpenStax | |||

valence band | highest energy band that is filled in the energy structure of a crystal | OpenStax | |||

van der Waals bond | bond formed by the attraction of two electrically polarized molecules | OpenStax | |||

vibrational energy level | energy level associated with the vibrational energy of a molecule | OpenStax | |||

acceptor impurity | atom substituted for another in a semiconductor that results in a free electron | OpenStax | |||

activity | magnitude of the decay rate for radioactive nuclides | OpenStax | |||

alpha (α) rays | one of the types of rays emitted from the nucleus of an atom as alpha particles | OpenStax | |||

alpha decay | radioactive nuclear decay associated with the emission of an alpha particle | OpenStax | |||

antielectrons | another term for positrons | OpenStax | |||

antineutrino | antiparticle of an electron’s neutrino in β^{−} decay |
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atomic mass | total mass of the protons, neutrons, and electrons in a single atom | OpenStax | |||

atomic mass unit | unit used to express the mass of an individual nucleus, where 1u=1.66054×10^{−27 }kg |
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atomic nucleus | tightly packed group of nucleons at the center of an atom | OpenStax | |||

atomic number | number of protons in a nucleus | OpenStax | |||

becquerel (Bq) | SI unit for the decay rate of a radioactive material, equal to 1 decay/second | OpenStax | |||

beta (ββ) rays | one of the types of rays emitted from the nucleus of an atom as beta particles | OpenStax | |||

beta decay | radioactive nuclear decay associated with the emission of a beta particle | OpenStax | |||

binding energy (BE) | energy needed to break a nucleus into its constituent protons and neutrons | OpenStax | |||

binding energy per nucleon (BEN) | energy need to remove a nucleon from a nucleus | OpenStax | |||

breeder reactor | reactor that is designed to make plutonium | OpenStax | |||

carbon-14 dating | method to determine the age of formerly living tissue using the ratio \(\displaystyle ^{14}C/^{12}C\) | OpenStax | |||

chart of the nuclides | graph comprising stable and unstable nuclei | OpenStax | |||

critical mass | minimum mass required of a given nuclide in order for self-sustained fission to occur | OpenStax | |||

criticality | condition in which a chain reaction easily becomes self-sustaining | OpenStax | |||

curie (Ci) | unit of decay rate, or the activity of 1 g of \(\displaystyle ^{226}Ra\), equal to \(\displaystyle 3.70×10^{10}Bq\) | OpenStax | |||

daughter nucleus | nucleus produced by the decay of a parent nucleus | OpenStax | |||

decay | process by which an individual atomic nucleus of an unstable atom loses mass and energy by emitting ionizing particles | OpenStax | |||

decay constant | quantity that is inversely proportional to the half-life and that is used in equation for number of nuclei as a function of time | OpenStax | |||

decay series | series of nuclear decays ending in a stable nucleus | OpenStax | |||

fission | splitting of a nucleus | OpenStax | |||

gamma (γγ) rays | one of the types of rays emitted from the nucleus of an atom as gamma particles | OpenStax | |||

gamma decay | radioactive nuclear decay associated with the emission of gamma radiation | OpenStax | |||

half-life | time for half of the original nuclei to decay (or half of the original nuclei remain) | OpenStax | |||

high dose | dose of radiation greater than 1 Sv (100 rem) | OpenStax | |||

isotopes | nuclei having the same number of protons but different numbers of neutrons | OpenStax | |||

lifetime | average time that a nucleus exists before decaying | OpenStax | |||

liquid drop model | model of nucleus (only to understand some of its features) in which nucleons in a nucleus act like atoms in a drop | OpenStax | |||

low dose | dose of radiation less than 100 mSv (10 rem) | OpenStax | |||

mass defect | difference between the mass of a nucleus and the total mass of its constituent nucleons | OpenStax | |||

mass number | number of nucleons in a nucleus | OpenStax | |||

moderate dose | dose of radiation from 0.1 Sv to 1 Sv (10 to 100 rem) | OpenStax | |||

neutrino | subatomic elementary particle which has no net electric charge | OpenStax | |||

neutron number | number of neutrons in a nucleus | OpenStax | |||

nuclear fusion | process of combining lighter nuclei to make heavier nuclei | OpenStax | |||

nuclear fusion reactor | nuclear reactor that uses the fusion chain to produce energy | OpenStax | |||

nucleons | protons and neutrons found inside the nucleus of an atom | OpenStax | |||

nucleosynthesis | process of fusion by which all elements on Earth are believed to have been created | OpenStax | |||

nuclide | nucleus | OpenStax | |||

parent nucleus | original nucleus before decay | OpenStax | |||

positron | electron with positive charge | OpenStax | |||

positron emission tomography (PET) | tomography technique that uses \(\displaystyle β^+\) emitters and detects the two annihilation \(\displaystyle γ\) rays, aiding in source localization | OpenStax | |||

proton-proton chain | combined reactions that fuse hydrogen nuclei to produce He nuclei | OpenStax | |||

radiation dose unit (rad) | ionizing energy deposited per kilogram of tissue | OpenStax | |||

radioactive dating | application of radioactive decay in which the age of a material is determined by the amount of radioactivity of a particular type that occurs | OpenStax | |||

radioactive decay law | describes the exponential decrease of parent nuclei in a radioactive sample | OpenStax | |||

radioactive tags | special drugs (radiopharmaceuticals) that allow doctors to track movement of other drugs in the body | OpenStax | |||

radioactivity | spontaneous emission of radiation from nuclei | OpenStax | |||

radiopharmaceutical | compound used for medical imaging | OpenStax | |||

radius of a nucleus | radius of a nucleus is defined as \(\displaystyle r=r_0A^{1/3}\) | OpenStax | |||

relative biological effectiveness (RBE) | number that expresses the relative amount of damage that a fixed amount of ionizing radiation of a given type can inflict on biological tissues | OpenStax | |||

roentgen equivalent man (rem) | dose unit more closely related to effects in biological tissue | OpenStax | |||

sievert (Sv) | SI equivalent of the rem | OpenStax | |||

single-photon-emission computed tomography (SPECT) | tomography performed with \(\displaystyle γ\)-emitting radiopharmaceuticals | OpenStax | |||

strong nuclear force | force that binds nucleons together in the nucleus | OpenStax | |||

transuranic element | element that lies beyond uranium in the periodic table | OpenStax | |||

antiparticle | subatomic particle with the same mass and lifetime as its associated particle, but opposite electric charge | OpenStax | |||

baryon number | baryon number has the value \(B=+1\) for baryons, \(–1\) for antibaryons, and 0 for all other particles and is conserved in particle interactions | OpenStax | |||

baryons | group of three quarks | OpenStax | |||

Big Bang | rapid expansion of space that marked the beginning of the universe | OpenStax | |||

boson | particle with integral spin that are symmetric on exchange | OpenStax | |||

color | property of particles and that plays the same role in strong nuclear interactions as electric charge does in electromagnetic interactions | OpenStax | |||

cosmic microwave background radiation (CMBR) | thermal radiation produced by the Big Bang event | OpenStax | |||

cosmology | study of the origin, evolution, and ultimate fate of the universe | OpenStax | |||

dark energy | form of energy believed to be responsible for the observed acceleration of the universe | OpenStax | |||

dark matter | matter in the universe that does not interact with other particles but that can be inferred by deflection of distance star light | OpenStax | |||

electroweak force | unification of electromagnetic force and weak-nuclear force interactions | OpenStax | |||

exchange symmetry | property of a system of indistinguishable particles that requires the exchange of any two particles to be unobservable | OpenStax | |||

fermion | particle with half-integral spin that is antisymmetric on exchange | OpenStax | |||

Feynman diagram | space-time diagram that describes how particles move and interact | OpenStax | |||

fundamental force | one of four forces that act between bodies of matter: the strong nuclear, electromagnetic, weak nuclear, and gravitational forces | OpenStax | |||

gluon | particle that that carry the strong nuclear force between quarks within an atomic nucleus | OpenStax | |||

grand unified theory | theory of particle interactions that unifies the strong nuclear, electromagnetic, and weak nuclear forces | OpenStax | |||

hadron | a meson or baryon | OpenStax | |||

Hubble’s constant | constant that relates speed and distance in Hubble’s law | OpenStax | |||

Hubble’s law | relationship between the speed and distance of stars and galaxies | OpenStax | |||

lepton | a fermion that participates in the electroweak force | OpenStax | |||

lepton number | electron-lepton number \(L_e\), the muon-lepton number \(L_μ\), and the tau-lepton number \(L_τ\) are conserved separately in every particle interaction | OpenStax | |||

mesons | a group of two quarks | OpenStax | |||

nucleosynthesis | creation of heavy elements, occurring during the Big Bang | OpenStax | |||

particle accelerator | machine designed to accelerate charged particles; this acceleration is usually achieved with strong electric fields, magnetic fields, or both | OpenStax | |||

particle detector | detector designed to accurately measure the outcome of collisions created by a particle accelerator; particle detectors are hermetic and multipurpose | OpenStax | |||

positron | antielectron | OpenStax | |||

quantum chromodynamics (QCD) | theory that describes strong interactions between quarks | OpenStax | |||

quantum electrodynamics (QED) | theory that describes the interaction of electrons with photons | OpenStax | |||

quark | a fermion that participates in the electroweak and strong nuclear force | OpenStax | |||

redshift | lengthening of the wavelength of light (or reddening) due to cosmological expansion | OpenStax | |||

Standard Model | model of particle interactions that contains the electroweak theory and quantum chromodynamics (QCD) | OpenStax | |||

strangeness | particle property associated with the presence of a strange quark | OpenStax | |||

strong nuclear force | relatively strong attractive force that acts over short distances (about \(10^{−15}) m) responsible for binding protons and neutrons together in atomic nuclei | OpenStax | |||

synchrotron | circular accelerator that uses alternating voltage and increasing magnetic field strengths to accelerate particles to higher and higher energies | OpenStax | |||

synchrotron radiation | high-energy radiation produced in a synchrotron accelerator by the circular motion of a charged beam | OpenStax | |||

theory of everything | a theory of particle interactions that unifies all four fundamental forces | OpenStax | |||

virtual particle | particle that exists for too short of time to be observable | OpenStax | |||

W and Z boson | particle with a relatively large mass that carries the weak nuclear force between leptons and quarks | OpenStax | |||

weak nuclear force | relative weak force (about \(10^{−6}\) the strength of the strong nuclear force) responsible for decays of elementary particles and neutrino interactions | OpenStax |