Midterm 1 Flashcards
(33 cards)
Gamma Rays (y)
wavelength: 10^-11 - 10^-15
Blackbody Radiation
Emits light when heated
Absorbs radiation
X-rays
wavelength: 10^-9 - 10^-13
Ultra-violet
wavelength: 10^-7 - 10^-9
Visible Light Wavelengths
Violet 390nm Blue 450nm Green 525nm Yellow 600nm Orange 650nm Red 750nm
Infrared
wavelength: 10^-3 - 10^-6
Microwave
wavelength: 10^-1 - 10^-3
Radiowaves
wavelength: 10^4 - 10^2
micro (u)
10^-6
nano (n)
10^-9
Angstrom (Å)
10^-10
pico (p)
10^-12
Radius of cations
smaller
Radius of anions
larger
Emission Spectra
v = c(RH) (1/n^2 - 1/n^2)
Emission Spectroscopy
Excited sample - slit - prism - lines
change in E: negative
Absorption Spectroscopy
light thru sample - slit - prism - spectrum missing lines
change in E: positive
Pauli Exclusion Principle
no two electrons can have the same quantum numbers
Hund’s Rule
electrons occupy degenerate orbitals singularly but in the same spin state
Aufau Process
fill to minimize energy
1s 2s 2p 3s 3p 4s 3d 4p 5s 4d 5p 6s
Exceptions filling orbitals
Cr [Ar] 3d^5 4s^1
Cu [Ar] 3d^10 4s^1
Radial Distribution Function (RDF)
Probability of finding an electron at distance r
RDF = 4(pi)r^2(workfunction)^2
Standing Wave Equation
L = n(wavelength/2) n = nodes + 1
Energy in a wave is
proportional to the amplitude