Nature Of Light Flashcards

(39 cards)

0
Q

Define a line spectrum

A

Discrete lines each typical of the element concerned

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1
Q

Does line spectra consist of a continuous band of different colours? What does it if not?

A

No

Discrete separate lines

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2
Q

How do you observe line spectra in the laboratory?

A

By viewing a discharge tube with a diffraction grating

Gas discharge lamp through a diffraction grating

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3
Q

How does the diffraction grating allow the spectrum to be viewed?

A

A voltage is applied across sodium for example which would vaporise; the hot vapors emit light and the diffraction grating allows it to be viewed

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4
Q

How are line spectra observed

A

By viewing a discharge tube with a diffraction grating

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5
Q

Change in E =

A

Hf

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6
Q

How do you convert from eV to J

A

X1.6x10^-19

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7
Q

How is an emission line spectra produced

A

By a hot gaseous element

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8
Q

What happens to electrons at higher temperatures

A

They’re excited into higher energy levels

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9
Q

Is energy emitted or absorbed when going from a high to a low energy level

A

Emitted

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10
Q

What is the difference between an emission and absorption spectrum

A

An absorption spectrum has black lines on a coloured background where as an emission spectrum his coloured lines on a black background

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11
Q

What do you see in an absorption spectrum (in terms of vapor and light)

A

When white light passes through a cooler water vapor

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12
Q

What has the absorption spectrum been used for in our universe

A

Looking at the composition of distant stars (their elements)

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13
Q

How are elements determined on different stars?

A

Using the absorption spectrum where
the white light passes through the cooler vapours of the outer layers of the star and the positions of the dark lines are compared to the absorption spectra of elements we know on earth

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14
Q

How can we check what an element is on a distant star?

How can we be sure?

A

Use the absorption spectra of the star from white light going through the cooler vapours on the outer layer of the star then comparing the spectrum to that of known elements on earth; the absorption spectra of an element is the same universally

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15
Q

What is redshift and what does it suggest/show?

A

Redshift is the spectral lines of light shifting to lower frequencies (red light) which suggests the source is moving away from us in support of the Big Bang theory as the origin of the universe.

16
Q

What happens to the energy when an electron moves up or down in energy levels
How could we calculate this energy value

A

It is emitted as a photon

Using E=hf

17
Q

What direction do the electrons move in an emission spectrum

A

Down energy levels towards the ground state

18
Q

What is the Bohr radius

A

The shortest radius of the closest possible orbit of an electron around a nucleus

19
Q

What is the de Broglie wavelength equation

A

Wavelength=h/p

20
Q

What does the de Broglie wavelength suggest

A

That electrons behave as waves as well as particles

21
Q

What does a stationary wave have to have, to occupy Bohr orbits
Why?

A

Waves with whole numbers of wavelengths because they’re stable and odd ones are not

22
Q

Why must the waves be standing for the Bohr orbits to exist

A

Because otherwise the waves wouldn’t be stable and would give out there energy and consequently cease to exist

23
Q

E=hc/?

A

Hc/wavelength

24
What happens to an unstable electron or wave at higher energy levels
It returns to it's lowest possible energy level and the energy difference is radiated away as a photon
25
How is a photon emitted from an atom
When an electron moves from a higher to a lower energy level
26
How is a photon absorbed
When an electron moves from a lower to a higher energy level
27
How can you calculate the wavelength of a photon when knowing it's energy difference only
Wavelength=hc/E
28
What is the photoelectric effect proving
That light can behave as a stream of particles as well as a wave I.e. Wave particle duality
29
How do you find the photon energy
E=hf
30
What is the work function
The minimum amount of energy required for an electron to escape the surface
31
Energy delivered by a photon goes where
To electrons to get then to the surface and to get then too escape
32
Where does the kinetic energy of an escaped photoelectron come from
It is left over from the energy transferred from a photon to the electron to get it to the surface and escape
33
The speed of an escaping electron depends on how much of their energy is used to get to the surface, what will be the fastest electrons then and what equation can we obtain from this?
The surface electrons because the energy needed to get them to the surface is zero hf=W + Ekmax
34
What is the threshold frequency
Where the energy of the photon is not great enough to cause an emission of an electron from the surface of a metal
35
What happens above and below the threshold frequency
Above=electrons are emitted | Below=electrons aren't emitted
36
What is the x intercept of a max KE/frequency graph equal to
The threshold frequency
37
Qvstop=
KE max
38
Can the ground state lose energy
No