exam 2: ch.3 and 4 Flashcards
theory of electromagnetic radiation
- James maxwell
- radiation travels through space as waves
-travels at the speed of light
wavelength (y)
distance between one wave crest to another
equation used to find wavelength
y = c/v
frequency (v)
the number of crests that pass through a stationary point in space per second.
cycles per second (s^-1)
Hertz = 1Hz =1 s^-1
equation to find frequency
v = c/y
amplitude
how big the crescent is
doesn’t affect wavelength or frequency
frequency and wavelength have a inverse relationship
short wavelength = highest energy
longest wavelength = lowest energy
equation:
c=yv
where
c- speed of light; constant (2.998 x10^8 m/s)
y- wavelength
v- frequency
blackbody radiation
the electromagnetic radiation emited by a perfect blackbody at a given temperature
Max plank
wiens displacement law
Ymax x T = constant
energy of one photon
E= hc/y
E unit is in jules
E= energy
h= planks constant ; j/s
c= 2.98 x 10^14 m/s
y= wavelength m
photoelectric effect
electrons can be ejected from a metal surface when light having a frequency greater than some threshold frequency is shone on it.
photoelectrons are emitted when the frequency of radiation exceeds some minimum threshold frequency.
greater the frequency, the greater kinetic energy imparted to the escaping electrons.
key observations of photoelectric effect
number of electrons increase as brightness increased.
the kinetic energy does NOT depend on brightness.
kinetic energy increased with increasing frequency of light.
work function
the minimum energy required to release an electron from the surface of a metal.
planks constant x threshold frequency (Eo=cV)
Balmer equation
accurate for hydrogen gas
y= 364.56 nm (m^2/ m^2-4)
Rydberg equation
accurate for other gases besides hydrogen.
directly proportional to wave energy!
1/y = Rh (1/n1^2) - (1/n2^2)
Rh= ryberg constant; 1.0974 x10^7 m-1
energy level
excited state (up) - short term state. not as happy
ground state (down) - most stable state. electron is happy
when electron comes down it emits energy.
change in energy
change in energy = (-2.18 x 10^-18 J ) ( 1/nf^2 - 1/ni^2)
nf = final
ni = inital