ch 9 - Atomic and Nuclear Phenomena Flashcards
photoelectric effect
when light of high frequency (blue to ultraviolet light) is incident on a metal in a vacuum, the metal atoms emit electrons; an “all or nothing” response
current
created by electrons liberated from the metal by the photoelectric effect that produce a net charge flow per unit time
threshold frequency (f sub T)
minimum frequency of light that causes ejection of electrons and depends on the type of metal being exposed to radiation
f
if frequency of incident photon is less than the threshold frequency then no electron will be ejected because the photons do not have sufficient energy to dislodge the e- from its atom
f>f sub T
If the frequency of incident photon is greater than the threshold frequency then an e- will be ejected and the maximum kinetic energy of the ejected e- will be equal to the difference between hf and hf sub T (also called the work function)
energy of photon equation
E=hf; where E is energy of the photon of light, h is Planck’s constant (6.626 x 10^-34 Jxs); f = frequency of the light
nanometer
1 nm = 10^-9 m
angstroms
1 A = 10^-10 m
max kinetic energy of the ejected e- equation
K sub max = hf - W; where h = Planck’s constant, f = frequency of the light, W = work function of the metal in question
work function related to threshold frequency of a certain metal, equation
work function is the min energy required to eject an electron and is related to the threshold frequency by W = hf sub T; where W = work function of the metal in question; h = Planck’s constant; f sub T = threshold frequency
infrared (IR) spectroscopy
used to determine chemical structure because different bonds will absorb different wavelengths of light
UV-Vis spectroscopy
looks at the absorption of light in the visible and ultraviolet range
note about indicators
most contain large organic compounds that have very different absorption patterns based solely on the protonation state of the compound. often have conjugated double bonds or aromatic ring systems which permit the absorption of light from photons in the visible range
fluorescence
if a fluorescent substance is excited (such as a ruby, emerald or phosphors in fluorescent lights) with uv radiation, it will begin to glow with visible light; it is a stepwise photon emission in which an excited e- returns to the ground state through one or more intermediate excited states in which each step emits a photon
mass defect
difference between the weight of the sum of protons and neutrons inside a nucleus and the actual weight of the nucleus which is slightly smaller
equation embodying mass defect
E = mc^2; E = energy; m = mass and c = the speed of light; this is a result of matter that has been converted to energy
strong nuclear force
force attaching protons and neutrons together to form the nucleus; strong enough to more than compensate for the repulsive electromagnetic force between the protons; acts over very short distances only
binding energy
energy that is radiated away from the nucleus in the form of heat, light or other electromagnetic radiation before the mass defect becomes apparent; allows the nucleons to bind together in the nucleus
weak nuclear force
also contributes to stability of the nucleus, but is one-millionth as strong as the strong nuclear force
Four fundamental forces of nature
strong nuclear force, weak nuclear force, electrostatic forces and gravitation
isotopic notation
notation in which elements are preceded by their atomic number as a subscript and mass number as a superscript
atomic number (Z)
corresponds to number of protons in nucleus
mass number (A)
corresponds to number of protons plus neutrons
fusion
occurs when small nuclei combine to form a larger nucleus
Fission
process by which a large nucleus splits into smaller nuclei; powers most nuclear power plants
radioactive decay
naturally occurring spontaneous decay of certain nuclei accompanied by emission of specific particles
Example of isotope decay arithmetic and nucleon conservation
X represents parent nucleus, Y represents daughter nucleus: (superscript A, subscript Z)X -> superscript A’, subscript Z’)Y + emitted decay particle; when balancing, sum of atomic numbers and mass numbers (separately) must be the same on both sides
Alpha decay
emission of an alpha-particle which is a (superscript 4, subscript 2)He nucleus that consists of two protons, two neutrons, and zero electrons; carries double charge of beta-particle and is much bigger; interact with matter very easily and do not penetrate shielding very extensively
balanced equation example of alpha decay
(superscript A, subscript Z)X -> (superscript A-4, subscript Z - 2)Y + (superscript 4, subscript 2)alpha
Beta decay
emission of the beta-particle which is an electron and is given the symbol e- or beta-; electrons do not reside in nucleus but are emitted by the nucleus when a neutron decays into a proton, a beta-particle, and an antineutrino (v with a line over it); more penetrating and much smaller (electron is 1836 times smaller than proton) than alpha-particle
positron emission
induced decay
positron
has mass of an electron but is positively charged: symbol is e+ or beta+; a neutrino (v) is emitted in positron decay
balanced equation example of beta- decay
(superscript A, subscript Z)X -> (superscript A, subscript Z + 1)Y + beta-; neutron is converted to electron so atomic number will be one more
example equation of beta+ decay
proton is converted into a neutron and beta+ particle is emitted: (superscript A, subscript Z)X -> (superscript A, subscript Z-1)Y + beta+
gamma decay
emission of gamma-rays which are high-energy (high-frequency) photons which carry no charge and simply lower the energy of the parent nucleus without changing the mass number or atomic number
expression equation of gamma decay
(superscript A, subscript Z)X -> (superscript A, subscript Z)X + gamma
electron capture
certain unstable radionuclides are capable of capturing an inner electron that combines with a proton to form a neutron, while releasing a neutrino. Atomic number is one less than the original but mass number remains the same; rare process best thought of as the reverse of beta- decay
expression of electron capture
(superscript A, subscript Z)X + e- -> (superscript A, subscript Z-1)Y
half-life (T sub 1/2)
in a sample of radioactive particles this is the time it takes for half of the sample to decay, in each subsequent half-life, one-half of the remaining sample decays so that the remaining amount asymptotically approaches zero
exponential decay equation
delta n/delta t = -(sign for wavelength)n; sign for wavelength = known as decay constant; solution tells us how the number of radioactive nuclei changes with time
exponential decay equation
n = n sub 0 x e (to the power of -wavelength sign (decay constant) x t); n sub 0 = number of undecayed nuclei at time t = 0
decay constant is related to the half-life by this equation
decay constant (upside down y) = (ln2)/(T sub 1/2) = (0.693)/(T sub 1/2)