Chem Module 2 Flashcards

1
Q

Quantization

A

When an electron is ‘confined’ to a finite region of space by the forces exerted on it
- total energy is restricted t certain values

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2
Q

Light and its three fields

A

electromagnetic radiation that transmits energy through space/medium, travels in waves
- electric field, magnetic field, direction that oscillate perpendicular to eachother

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3
Q

wavelength

A

distance between adjacent maxima

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4
Q

period

A

time for electric field to return to its max strength

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5
Q

frequency

A

related to period , 1/T

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6
Q

The electromagnetic spectrum in increaing wavelength (decreasing frequency )

A

gama rays, x rays, ultraviolet, visible, infrared, microwave, radiowaves

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7
Q

Range of visible region in nm

A

from 400 to 750 nm

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8
Q

visible spectrum and their colours

A
  • violet (400)
  • indigo
  • blue
  • green (570)
  • yellow
  • orange
  • red (750)
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9
Q

3 experiments that support the concept of energy being quantized at the molecular level

A
  1. Blackbody Radiation
  2. The Photoelectric Effect
  3. Line Spectra of Atoms
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10
Q

Blackbody Radiation

A
  • atoms in a heated solid osciallte with certain energies only
  • Energy of oscillation = nhv
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11
Q

Max Planck

A

First suggestion of quantization of energy , quanta of energy are absorbed by and emitted from matter
- Frequency : v=c/landa
- Energy: E = nhv (h is an constant , v is frequency)
- plancks constant

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12
Q

The photoelectric effect

A
  • Energy of light is highly localized and is proportional to its frequency
  • light can produce and electric current
  • discovered by having electrons dislodge from the surface of a metal
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13
Q

Observations of the photoelectric effect

A
  • electrons were ejected only if the frequency of light was greater than some “threshold” frequency
  • ejected electron increased proportionally with frequency
  • energy of the light must be highly localized in space and not spread out over the entire wave
  • proportionality constant between frequency and energy is equal to Planck’s constant

Ephoton =hv

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14
Q

Line Spectra of atoms

A

Energy of an electron in an atom is not arbitrary , restricted to certain special values.
- absorbed or emitted colours show that atoms absorb or emit photons with certain specific energies - emission lines

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15
Q

Problems with the Bohr Model

A
  • doesn’t explain why the angular momentum and energy of the electron is quantized
  • model not extended to other atoms
  • why doesn’t the H atom emit radiation continuously?
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16
Q

2 solutions to the limitations of the Bohr Model (behaviour of electrons)

A
  1. de Brogile’s hypothesis
  2. the Heisenberg uncertainty principle
17
Q

de Brogile’s hypothesis

A

particles exhibit wave-particle duality by understanding
- diffraction (light behaving as a wave)
- The photoelectric effect (light behaves as particles)

experiment: diffraction pattern produced by constructive and destructive interference of light waves

18
Q

Heisenberg uncertainty principle

A

we can never know the true behaviour of a system
- if we tried to measure the position of an electron, we will change its momentum

19
Q

n quantum number

A

principal quantum number - determines size of orbital (any integer)

20
Q

l quantum number

A

orbital angular momentum quantum number - determines the shape of an orbital (n-1)

21
Q

ml quantum number

A

magnetic quantum number - the number of distinct orientations allowed for a particular orbital (-l to +l)

22
Q

Radial factors, what does it describe and its axis

A

R(r) and r, how the wave function changes w distance from nucleus

23
Q

Radial electron density, what does it describe and its axis

A

R(r)^2 and r, probability of finding electron changes as we move away from the nucleus

24
Q

Radial Distribution plot, what does it describe and its axis

A

r^2(R)r^2 and r, average distance between nucleus and electron

25
Q

Significance of Schrodinger equation

A

describes the behaviour of a single electron moving about the nucleus in the H atom