Title: Sin t
1Plancks constant in the light of an
incandescent lamp
2Introduction
3The idea of light quanta
- Planck (1900) emission of radiant energy by
matter does not take place continuously, but in
finite quanta of energy h?
(h Plancks constant 6.63x10-34 J.s,
? frequency) - Einstein (1905) light quanta (photons) as
inherent in the nature of radiation itself
4Distribution of intensity of heat radiation as a
function of the wavelength
? Emissivity (1 for perfect black-body
radiation)
C1, C2 Constant parameters
5Plancks radiation law
Radiation energy per time unit for the
wavelength ?
Where c2hc/k h Plancks constant c
velocity of light k Boltzmanns constant
Main objective of this experiment
6Report on the experiment
7Emission of a 12 V tungsten lamp
8The light spectrum emitted by the filament is
continuous.
9A narrow band of the visible spectrum is
selected with a combination of Orange II and
Copper Sulphate solution (it absorbs infrared
strongly).
?0
Liquid filter
10 We will assume that the selected band is
nearly monochromatic.
?0
Liquid filter
11The wavelength of the selected band is in the
spectral response range of a Light Dependent
Resistor (LDR)
?0
Liquid filter
12Block diagram
From the formula
For small ?
lllumination E on the LDR is proportional to the
transmitted energy
Plotting
Resistance R of LDR is related to illumination
as
Taking logarithms
Combining (2), (3) and (4)
b constant ? parameter
13Experimental setup
14GENERAL DIAGRAM
15COMPONENTS
16INSTALLING THE EQUIPMENT
171
Turn the potentiometer knob anticlockwise up
to the limit
18 Turn slowly the tube holder aligning the
lateral holes between the lamp and the LDR.
2
19Move the LDR towards its lateral hole,
positioning its surface as the figure shows.
3
204
Insert the solution filter tube in its holder.
21Put the cover onto the platform to protect from
the outside light. In order to ensure the
correct initial conditions, LDR should keep in
total darkness for at least 10 minutes before the
measurements.
5
22Procedure
Some previous measurements are needed before
using Equation (6)
23T? Temperature of the emmitting filament
Relation between the resistance of the filament
(RB) and its temperature (T)
RB
Experimental data fit
RB0
a can be derived from the filament resistance
(RB0) at room temperature (T0)
Using the multimeter as a thermometer.
RB0 can be extrapolated to I 0 from
measurements of V and I,
24?? transmission of the filter
- Solution of
- Orange II.
- CuSO4 (it absorbs the infrared light).
?/nm
25?? Parameter of the LDR
26COLLECTING DATA
27From the slope
We obtain
And finally the Plancks constant
h Plancks constant. k Boltzmanns constant. c
speed of light.
28End of presentation