MODULE 8 IQ 3 Flashcards
limitations of rutherford’s atomic model
- could not explain electron/atomic stability
- no restriction on orbit of electrons –> produce continuous spectra –> contradicts existing discrete emission lines of hydrogen atoms
bohr’s 1st postulate
electrons orbit in stationary states and do not radiate energy –> stays in quantised energy levels
bohr’s 2nd postulate
transition between stationary states would be accompanied by absorption or emission of energy in the form of EMR
bohr’s 3rd postulate
angular momentum is quantised
- electrons undergo uniform circular motion due to electrostatic attraction between itself and nucleus
limitations of bohr’s atomic model
- did not clearly explain discrete emission of photons beyond hydrogen
- didn’t explain why hydrogen spectral lines were not of equal intensity
- zeeman effect –> when gas is excited in magnetic field, emission spectrum shows a splitting of spectral line
balmer equation
calculate wavelengths of these lines
1/wavelength = R(1/m^2 - 1/n^2)
rydberg’s equation
predict wavelength of proton absorbed or emitted when an electron transitions between orbits of different states
louis de broglie equation
wavelength = h/mv
louis de broglie model
linked waves and particles together
- any moving particle has an associated wavelength
- should be possible to detect wave nature of electrons if they were diffracted from surface of crystal
using de broglie to explain stationary states
applying particle-wave duality –> electron orbits were standing waves (radius of each energy level was an integer multiple of electron’s wavelength)
n x h/2(pi) = 2(pi)r
- now orbit in standing waves, they do not lose energy
davisson and gemer
tried to observe the scattering of electrons onto the surface of a piece of nickel
- accidentally annealed the metal, producing a smooth region of large crystals
- formed interference pattern –> calculate wavelength of electron by using diffraction methods: wavelength = 2dsin(theta)
erwin schrodinger model of the atom
- defined a wave function through solving a differential equation derived from the forces acting upon an electron
- square of this wave gave probability that an electron would be at that distance from the nucleus