Physical lecture 2 Flashcards

1
Q

State the fundamental equation for the speed of an EM wave

A

c = fλ
c is the speed of the wave
f is the frequency
λ is the wavelength

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2
Q

State the multiplier for the prefix ‘nano’

A

10^-9

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3
Q

Define one Å

A

Å represents ‘angstrom’. One angstrom = 1x10^-10m

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4
Q

Define wavenumber (v~) and relate it to photon energy

A

1/λ, measured in (length)-1. We can get E = hcv~, so photon energy is proportional to wavenumber. It is an energy equivalent unit

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5
Q

State how to convert from m^-1 to cm^-1

A

Divide by 100

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6
Q

Describe the emission spectra of the hydrogen atom

A

There are many lines which are clearly in groups (ie series), with each series of lines converging with decreasing wavelengths/ an increasing photon energy. All lines in a series have the same value of n1. The names correspond to the scientists who observed them.

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7
Q

Give Bohr’s equation for wavenumber and explain the terms

A

v~ = -RH(1/n2^2 - 1/n1^2), usually measured in cm-1
RH is the Rydberg constant for the hydrogen atom.
n2 is the quantum number of the upper level of the transition, and n1 the number of the lower level
n2 > n1

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8
Q

State the names of the first four series and their values of n1

A

Lyman (n1 = 1), Balmer (n1 = 2) , Paschen (n1 = 3) and Brackett (n1 = 4)

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9
Q

Describe Bohr’s explanation of his equation for wavenumber

A

He said the electron orbiting the nucleus must be confined to specific orbits of fixed energies, with each orbit having a different value of n

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10
Q

Give the energy level expression for the hydrogen atom in joules and wavenumbers

A

-hcR/n^2 in joules
-R/n^2 in wavenumbers
n is the principle quantum number

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11
Q

Define the zero of energy

A

Also known as the ionisation limit, where n = ∞, this is defined as a separated proton and electron. From this we can see why orbital energies are negative.

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12
Q

Describe how to determine the value of R in the energy level expression for an atom

A

Start by looking at values of wavenumber of lines in one series; all values of n1 will be the same so 1/n1^2 can be labelled as a constant c. Now the Bohr equation resembles that of a straight line, and -R can be found by calculating the gradient of this line

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13
Q

Describe the Rydberg constant

A

Rx is calculated using values of wavenumber for a particular atom. It differs slightly for different atoms.

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14
Q

Describe Bohr’s three postulates that quantitatively explain the energy level equation for the hydrogen atom

A
  • Electrons move in circular orbits around the nucleus
  • Only certain orbits are allowed, ie those with integer values of n. While in these orbits, electrons do not emit energy.
  • A single photon is emitted or absorbed when an electron moves into a different orbital
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15
Q

Give the equation that gives the force required to keep a particle in its circular orbit and explain the terms

A
F = - mv^2/r
F = force
m = mass of the particle
v = velocity of the particle
r = radius of the orbit
Note the negative sign: force is in the opposite direction to the radius, ie it points towards the centre of the orbit
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16
Q

Give the equation for linear momentum

A
p = mv 
p = momentum 
m = mass 
v = velocity
17
Q

Describe angular momentum

A

It is a vector quantity and its direction is perpendicular to the plane of rotation. It is important as electrons and photons have angular momentum which is usually conserved in chemical processes.

18
Q

Give the equation for angular momentum and explain the terms

A

L = Iω
I is the moment of inertia; the angular equivalent of mass
ω (omega) is the angular velocity in rads-1

19
Q

Describe I, the moment of inertia

A

I is the sum over all the masses that make up the body multiplied by the square of their distance from the axis of rotation. Ie heavy objects with a lot of mass far from the axis of rotation have a large moment of inertia