1/46
Looks like no tags are added yet.
Name | Mastery | Learn | Test | Matching | Spaced |
---|
No study sessions yet.
quantum theory
idea that atoms/molecules emit energy in discrete quantities called quanta rather than continuously
by Planck
wave
a vibrating disturbance by which energy is transmitted
speed depends on type and nature of medium its travelling through (ex: air, water, vacuum)
wavelength (lambda)
the distance between identical points on successive waves
frequency (v: nu)
the number of waves that pass through a particular point in one second
unit: hertz (Hz) = 1 cycle/s
amplitude
the vertical distance from the midline of a wave to the peak or trough
speed (u)
equals wavelength times frequency
= (lambda) (nu)
electromagnetic wave
has an electric field component and a magnetic field component (both components have same wavelength, frequency, and speed, but travel in mutually perpendicular planes)
Maxwell's theory
provides a mathematical description of the general behavior of light
electromagnetic radiation
the emission and transmission of energy in the form of electromagnetic waves
speed of light (c)
speed of electromagnetic wave in a vacuum
3 x 10^8 m/s, 186,000 miles per sec
v = c / lambda
types of radiation
gamma rays, X rays, UV, visible light (violet to red), infrared, microwave, radio waves (FM to AM)
quantum
the smallest quantity of energy that can be emitted (or absorbed) in the form of electromagnetic radiation
E = hv = h (c / lambda)
h is Planck's constant, v is frequency of radiation
Planck's constant
6.63 x 10^-34 J s
photoelectric effect
a phenomenon in which electrons are ejected from the surface of certain metals exposed to light of at least a certain minimum frequency (threshold frequency: all or none)
number of ejected electrons is proportional to intensity
photons
by Einstein
particles of light
each must possess energy E
KE = hv -W
emission spectra
either continuous or line spectra of radiation emitted by substances
unique for each element, like a fingerprint
line spectra
the light emission only at specific wavelengths
bright lines in different parts of the visible spectrum instead of a continuous spread of wavelengths from red to violet
Rhydberg constant
for hydrogen: 2.18 x 10^-18 J
En = -Rh ( 1 / n^2)
ground state (level)
the lowest energy state of a system
excited state (level)
higher in energy than the ground state
node
points on the string where amplitude of the wave is 0
located at each end and sometimes between ends
greater frequency means more
De Broglie
2pir = n lambda
r is radius of orbit, lambda is wavelength, n = 1, 2, 3
lambda = h / mu
Heisenberg uncertainty principle
it's impossible to know simultaneously both the momentum (mass times velocity) and the position of a particle with certainty
can't know location and momentum at the same time
quantum (wave) mechanics
Schrodinger
electron density
gives the probability that an electron will be found in a particular region of an atom
atomic orbital
the wave function of an electron in an atom
many-electron atoms
atoms containing 2+ electrons
quantum numbers
required to describe the distribution of electrons in hydrogen and other atoms
principle (n), angular (l), magnetic (ml), electron spin (ms)
principle quantum number (n)
integral values: 1, 2, 3, etc.
larger means farther from nucleus
angular momentum quantum number (l)
tells shape of the orbital
dependent on n (can be from 0 to n-1)
designated by s(0), p(1), d(2), f(3), g(4), h (5)
magnetic quantum number (ml)
describes orientation of orbital in space
depends on l: -l, (-l + 1), ... 0 ... (+l - 1), +l
electron spin quantum number (ms)
can be +1/2 or -1/2 depending on spinning motion of electron
boundary surface diagram
encloses about 90% of total electron density in an orbital
s orbital
spherical
size is proportional to n^2
electron configuration
how the electrons are distributed among the various atomic orbitals
electron configuration
ex: 1s^1 (read 1 s 1)
1: principle quantum number n
s: angular momentum number l
^1: number of electrons in the orbital/subshell
orbital diagram
shows the spin of the electron
upward vs. downward arrow
pauli exclusion principle
no 2 electrons in an atom can have the same 4 quantum numbers (change ms if n, l, and ml are the same)
only 2 electrons can occupy the same orbital: they must have opposite spins
paramagnetic substances
contain net unpaired spins and are attracted by a magnet (up up or down down): parallel spins
diamagnetic substances
don't contain net unpaired spins, are slightly repelled by a magnet (up down or down up): antiparallel spins
hund's rule
the most stable arrangement of electrons in subshells is the one with the greatest number of parallel spins
general rules
1. each shell or principle level of quantum number n has n subshells
2. each subshell of quantum number l has (2l + 1) orbitals
3. no more than 2 electrons in each orbital: max number of electrons is 2x number of orbitals used: must have opposite spins
4. determine mx number of electrons in a principle level using 2n^2
1. no 2 electrons can have same 4 quantum numbers (pauli exclusion)
2. most stable arrangement of electrons is one with greatest number of parallel spins (hund's rule)
3. unpaired electrons: paramagnetic, atoms with paired electrons are diamagnetic
4. in hydrogen, energy of electron only depends on n, in many-electron atoms, the energy depends on n and l
5. in many-electron atoms, subshells are filled in order (figure 7.21)
6. s > p > d > f (more energy needed to separate 3s electron than a 3p electron)
aufbau principle
as protons are added one by one to the nucleus o build up the elements, electrons are similarly added to the atomic orbitals
noble gas core
shows in brackets the noble gas element that most nearly precedes the element being considered
transition metals
either have incompletely filled d subshells or readilygive rise to cations that have incompletely filled d subshells
ground-state configurations of elements
see pg. 242 + 243
lanthanides (rare earth series)
have incompletely filled 4f subshells or readily give rise to cations with incompletely filled 4f subshells
actinide series
last row of elements
most aren't found in nature (synthesized)