Purpose:
To determine experimentally the value of Plank's constant.
Method:
Use a diffraction grating, 2 meter sticks, and a voltmeter to record the wavelength and potential drop across a collection of differently colored LEDs.
The data from our experiment can be found here.
Four LEDs were chosen;
blue
red
yellow
and green
their differences in wavelength should allow for the construction of a graph of photon energy vs. wavelength.
Quantum physics predicts that photons which are emitted from an atom are created when an electron travels from an excited state to a relaxed state. The energy levels of each of those states are of definite energy, and thus every photon emitted should have an identical wavelength. If the atom which emits the electron is bound in a crystal lattice, the energy levels of each state cannot overlap with nearby atoms because of the Pauli Principle. Thus the energy levels of each atom exist in a band approximately centered around the original energy level. This allows for photons of various wavelengths to be emitted from a sample of uniform atomic nature.
The observation associated with this effect is a smearing of the observed emission line when viewed through a diffraction grating.
A light emitting diode, or LED, is an electronic device which takes advantage of this property to generate photons in the visible spectrum. It is usually fabricated using p-type and n-type silicon in such a way that the energy an electron gains by traveling across the LED is equal to the energy of the desired photon.
Upon analysis of of data, a graph of photon energy vs. frequency was obtained from Microsoft Excel.
Unfortunately, the units on the vertical axis are too small to be properly displayed, but they can be viewed in the associated spreadsheet. The slope of this graph is found to be 8.8269 E-34 J/m, which is in error of 33% when compared to the accepted value of plank's constant, 6.626 E-34.
This value of error is unsatisfactory, so a separate method was used to estimate Plank's constant.
If the data points for energy are divided by their corresponding frequency, a set of ratios is obtained.
E/f
Red: 6.38E-34 J/m
Yellow: 5.97E-34 J/m
Green: 7.08E-34 J/m
Blue: 6.81E-34 J/m
These numbers are much closer to the accepted value of Plank's constant, and when averaged, yields a ratio of 6.56E-34 J/m, which is in error by only a single percent.
Modern Physics Blog BPW
Modern Physics Electronic Laboratory Journal.
Sunday, December 11, 2011
Saturday, November 26, 2011
Wavelength of a gas lamp
It is clear that there are three spectral images formed to the right of the actual lamp. These three spectral images have colors corresponding to the wavelengths of photons emitted from mercury when one of its electrons is excited and then relaxes to a lower energy state.
Our experimental apparatus, as visible in the picture, consists of a 2 meter stick, and a meter stick arranged orthogonally on a table. The horizontal displacement of the spectral images can thus be converted into an angular relationship, or it can be left in units of length to solve for the wavelength of the light directly.
Similar to the CD diffraction experiment, the position of the spectral images and the spacing of the diffraction grating can be used to determine wavelength. The governing equation is:
λ = (D*d)/sqrt(L^2+D^2)
Where:
D = the horizontal distance of the image
d = the diffraction spacing
L = the distance between the diffraction grating and the gas lamp
This experimental setup yielded the following data for a hydrogen lamp placed in the same location:
position of image in cm:
1=48
2=54
3=74.5
uncertainty: .5cm
L = 2 meters
d = .000002 meters
This setup yields the following prediction for the wavelengths
1 = 466nm
λ = (D*d)/sqrt(L^2+D^2)
Where:
D = the horizontal distance of the image
d = the diffraction spacing
L = the distance between the diffraction grating and the gas lamp
This experimental setup yielded the following data for a hydrogen lamp placed in the same location:
position of image in cm:
1=48
2=54
3=74.5
uncertainty: .5cm
L = 2 meters
d = .000002 meters
This setup yields the following prediction for the wavelengths
1 = 466nm
2 = 523nm
3 = 698nm
Calibration of our apparatus against a white light, yielded a correction factor for our setup which included a systematic error of +37.7nm
When factored into the previous data, our final results are
1 = 428.3nm
2 = 485.3nm
3 = 660.3nm
when compared to the actual spectra for hydrogen:
1 = 434 nm
2 = 486 nm
3 = 656 nm
It appears our predictions are correct to within a single percent. This falls approximately in the same range as our uncertainty in horizontal position.
3 = 698nm
Calibration of our apparatus against a white light, yielded a correction factor for our setup which included a systematic error of +37.7nm
When factored into the previous data, our final results are
1 = 428.3nm
2 = 485.3nm
3 = 660.3nm
when compared to the actual spectra for hydrogen:
1 = 434 nm
2 = 486 nm
3 = 656 nm
It appears our predictions are correct to within a single percent. This falls approximately in the same range as our uncertainty in horizontal position.
Particle in a box
Welcome to another edition of SOLVE THAT ACTIVPHYSICS PROBLEM. Our contestant today must answer 10 questions related to the particle in a box simulation at:
http://wps.aw.com/aw_young_physics_11/13/3510/898597.cw/index.html
Lets get this contest started.
Questions in order:
Question 1: Standing Waves
From your study of mechanical waves, what is the longest wavelength standing wave on a string of length L?
The longest wavelength for a standing wave is twice the length of the string, or twice the distance between the two hard boundaries.
Question 2: The de Broglie Relation
What is the momentum of the longest wavelength standing wave in a box of length L?
de Broglie hypothesized that the momentum of a particle must be equal to plank's constant divided by the wavelength, which in this case is 2L.
Question 3: Ground State Energy
Assuming the particle is not traveling at relativistic speeds, determine an expression for the ground state energy.
Ground state energy here refers to the kinetic energy stored in the particle, if we are operating at non-relativistic speeds then:
p=mv
K=.5mv^2
p^2 = (mv)^2
p^2/(2m) = K
then, applying p = h/2L
K = (h/2L)^2/(2m)
K = h^2/(8mL)
Question 4: Increasing L
If the size of the box is increased, will the ground state energy increase or decrease?
It will decrease, as the relationship places L as the divisor of the energy equation.
Question 5: The Correspondence Principle: Large Size
In the limit of a very large box, what will happen to the ground state energy and the spacing between allowed energy levels? Can this result explain why quantum effects are not noticable in everyday, macroscopic situations?
As L approaches the scale of human objects, the ground state energy takes on a magnitude of 10^-37 Joules, which is negligible on macroscopic scale.
Question 6: The Correspondence Principle: Large Mass
In the limit of a very massive particle, what will happen to the ground state energy and the spacing between allowed energy levels?
Massive particles also act as divisors in the energy equation, thus large particles have low levels of ground stage energy.
Question 7: Ground State Probability
If a measurement is made of the particle's position while in the ground state, at what position is it most likely to be detected?
The particle is most likely to be found in the middle of the trap.
Question 8: Probability: Dependence on Mass and Size
The most likely position to detect the particle, when it is in the ground state, is in the center of the box. Does this observation depend on either the mass of the particle or the size of the box?
No, the wave function of the particle is independent of mass, and always has a maximum at L/2.
Question 9: Probability: Dependence on Energy Level
The most likely position to detect the particle, when it is in the ground state, is in the center of the box. Does this observation hold true at higher energy levels?
No, for instance the first excited state is more likely to be found at L/4 and 3L/4.
Question 10: The Correspondence Principle: Large n
In the limit of large n, what will happen to the spacing between regions of high and low probability of detection? Does this agree with what is observed in everyday, macroscopic situations?
As n approaches large values, the probability density function becomes almost continuously flat, or equally likely in every location. This is consistent with a free particle, which has no definite location.
http://wps.aw.com/aw_young_physics_11/13/3510/898597.cw/index.html
Lets get this contest started.
Questions in order:
Question 1: Standing Waves
From your study of mechanical waves, what is the longest wavelength standing wave on a string of length L?
The longest wavelength for a standing wave is twice the length of the string, or twice the distance between the two hard boundaries.
Question 2: The de Broglie Relation
What is the momentum of the longest wavelength standing wave in a box of length L?
de Broglie hypothesized that the momentum of a particle must be equal to plank's constant divided by the wavelength, which in this case is 2L.
Question 3: Ground State Energy
Assuming the particle is not traveling at relativistic speeds, determine an expression for the ground state energy.
Ground state energy here refers to the kinetic energy stored in the particle, if we are operating at non-relativistic speeds then:
p=mv
K=.5mv^2
p^2 = (mv)^2
p^2/(2m) = K
then, applying p = h/2L
K = (h/2L)^2/(2m)
K = h^2/(8mL)
Question 4: Increasing L
If the size of the box is increased, will the ground state energy increase or decrease?
It will decrease, as the relationship places L as the divisor of the energy equation.
Question 5: The Correspondence Principle: Large Size
In the limit of a very large box, what will happen to the ground state energy and the spacing between allowed energy levels? Can this result explain why quantum effects are not noticable in everyday, macroscopic situations?
As L approaches the scale of human objects, the ground state energy takes on a magnitude of 10^-37 Joules, which is negligible on macroscopic scale.
Question 6: The Correspondence Principle: Large Mass
In the limit of a very massive particle, what will happen to the ground state energy and the spacing between allowed energy levels?
Massive particles also act as divisors in the energy equation, thus large particles have low levels of ground stage energy.
Question 7: Ground State Probability
If a measurement is made of the particle's position while in the ground state, at what position is it most likely to be detected?
The particle is most likely to be found in the middle of the trap.
Question 8: Probability: Dependence on Mass and Size
The most likely position to detect the particle, when it is in the ground state, is in the center of the box. Does this observation depend on either the mass of the particle or the size of the box?
No, the wave function of the particle is independent of mass, and always has a maximum at L/2.
Question 9: Probability: Dependence on Energy Level
The most likely position to detect the particle, when it is in the ground state, is in the center of the box. Does this observation hold true at higher energy levels?
No, for instance the first excited state is more likely to be found at L/4 and 3L/4.
Question 10: The Correspondence Principle: Large n
In the limit of large n, what will happen to the spacing between regions of high and low probability of detection? Does this agree with what is observed in everyday, macroscopic situations?
As n approaches large values, the probability density function becomes almost continuously flat, or equally likely in every location. This is consistent with a free particle, which has no definite location.
Experiment 12: CD diffraction
Using the properties of diffraction, it is possible to measure the space between adjacent grooves on a CD. If you shine a laser on a CD and observe the spacing between the central maxima and the resulting accessory maxima it is possible to calculate the groove spacing by using the following geometric relationship.
Photo credits to sciwebhop
the distance between points A and B is notated as d. Θ is measured in degrees from the normal to the diffraction grating, and λ is the wavelength of the light incident on the diffraction grating. The following equation relates these variables.
d*sin(Θ)= m * λ
d*sin(Θ)= m * λ
Where m is the number of the maxima counting away from the central maxima.
When a laser is shone upon a CD the reflected pattern may appear something like this.
It is clear from this image that some form of diffraction is taking place. By measuring the spacing between these maxima, and measuring the distance from the wall to our CD we can determine the angular separation of these maxima, additionally we know the wavelength of the laser to be 630-680 nanometers.
This table holds all of the relevant data.
It is clear from the calculations that there is some sort of systematic error in our data collection, and it most likely stems from the fact that we were not measuring the appropriate phenomena.
The predicted groove spacing based on our data is 2.6 * 10^-5 meters which is 16 times larger than the specifications listed for a CD(1.6 micrometers).
Unfortunately, we were unable to collect data after determining the flaw in our experiment and are unable to verify the CD groove spacing with the current data.
Additionally, here is an interesting video on another method for determining the groove spacing.
http://www.youtube.com/watch?v=IKKFPtcaZpQ
Wednesday, November 2, 2011
Time dialation
Einstein based the special theory of relativity on two postulates.
The first being that the laws of physics are the same in any inertial frame.
The second being that the speed of light is measured to be the same in any inertial frame. Take these two light clocks for example...
The first being that the laws of physics are the same in any inertial frame.
The second being that the speed of light is measured to be the same in any inertial frame. Take these two light clocks for example...
The guy standing next to the stationary clock measures the speed of light to be c.
A guy riding on the moving clock measures the speed of light to be c.
On the surface, these simple postulates seem both logical and convenient, but they lead to a plethora of paradoxes. Take for example a person in a spaceship travelling at half the speed of light, if they turn on the headlights for their spaceship, the light travels away from them at the speed of light.
But how does this appear to a stationary observer watching the same ship?
Classical Newtonian physics predicts that if light has a velocity of c compared to the spaceship, and the spaceship has velocity .5c compared to the observer, then the light must be travelling at 1.5c compared to the stationary observer.This however violates the second postulate, that the speed of light is measured to be the same by the people in the spaceship AND the stationary observer. How is this possible?
In a deft side step, Albert invents this half baked theory of time dilation.
What is time dilation you say?
In the simple form it means that time is travelling slower for the people on the spaceship than it is for the stationary observer. (A more through approach reveals that this too produces a paradox, but lets just wave our hands and say 'OKAY Albert, what ever you say must be true.')
Well, if time is travelling at different rates for different people, how do we compare them to one another?
BAM! We have this convenient formula.
The t' represents the magnitude of a unit of time, lets call it a second, compared to the stationary observer's time, t. The denominator has terms v, for the velocity of the travelling thing, and c for the speed of light. The denominator can also be represented by multiplying t by a term we refer to as gamma. Interesting to note is that in the limit where v approaches c, t' approaches infinity. As such, it appears all things happen simultaneously to things travelling at the speed of light.
One might ask, how do we use this? Well, the nice people over at activphysics
provided us with an example using the light clocks from above. If told that the round trip time for the moving clock is 7.45 us, measured from the stationary frame, and that the stationary clock takes 6.67 us, we can determine the value that the coefficient of t must take in the above equation. The value that expression takes is also known as the Lorentz Factor.
A simple division results that the Lorentz factor for the moving clock is 1.117, meaning that a single second in the stationary frame lasts 1.117 seconds in the moving frame. Solving this expression for velocity results in a v of, .445c.
Sunday, October 9, 2011
Measuring a Human Hair
Interference is a property of wave interaction. The presence of interference in the propagation of light is a strong argument for it being a wave.
Using a laser, it is possible to observe interference when it is projected past a human hair. A picture of the experimental set up follows.
The note card in the picture has had a hole punched in it, and a human hair is suspended across the hole and held in place by tape. A laser is aimed past the hair so that the beam is bisected by it. On the recieving surface, it is possible to observe interference effects, though this photo did not capture them. This is due to the low intensity of the constructive interference bands.
By measuring the distance from the notecard to the flat surface, the distance from the center of the laser beam to the center of one of the intensity peaks, and using the wavelength of the laser, it is possible to measure the diameter of the hair suspended in the notecard.
Our experiment generated the following results
Length from notecard to board : 2 meters
distance from laser center to 3rd anti-node (Ym): 6.5 cm
wavelength of light emitted: 630 - 680 nanometers
using the constructive interference approximation equation
Ym = Length * wavelength * anti-node number / diameter of hair
Solving this equation for diameter results in a range of diameters from 5.85*10^-5 meters to 6.27*10^-5 meters. Upon further investigation, a microscope determined that the diameter of the hair was approximately 6*10^-5 meters which supported the laser measurement.
Using a laser, it is possible to observe interference when it is projected past a human hair. A picture of the experimental set up follows.
The note card in the picture has had a hole punched in it, and a human hair is suspended across the hole and held in place by tape. A laser is aimed past the hair so that the beam is bisected by it. On the recieving surface, it is possible to observe interference effects, though this photo did not capture them. This is due to the low intensity of the constructive interference bands.
By measuring the distance from the notecard to the flat surface, the distance from the center of the laser beam to the center of one of the intensity peaks, and using the wavelength of the laser, it is possible to measure the diameter of the hair suspended in the notecard.
Our experiment generated the following results
Length from notecard to board : 2 meters
distance from laser center to 3rd anti-node (Ym): 6.5 cm
wavelength of light emitted: 630 - 680 nanometers
using the constructive interference approximation equation
Ym = Length * wavelength * anti-node number / diameter of hair
Solving this equation for diameter results in a range of diameters from 5.85*10^-5 meters to 6.27*10^-5 meters. Upon further investigation, a microscope determined that the diameter of the hair was approximately 6*10^-5 meters which supported the laser measurement.
Thin Lens experiment
As always, the data for this experiment can be found on google documents by following this link.
A magnifying lens can be modelled as a thin lens in the physics of optics because its total thickness is negligible in comparison to the radius of curvature for each surface.
For this experiment we used a light box, a paper with a non symmetric cross printed on it, a magnifying lens, and a flat surface to project the image on.
The above image shows the light box and lens combination.
When the ambient lighting is suppressed and the light box is projected through the lens, an inverted image can be seen on the opposite side of the lens.
Though barely visible in the glass, it is possible to see that the reflection of the cross is both vertically and horizontally inverted from the image that appears on the flat box.
The sharpness and size of the projected image was found to be variant with light box distance (object distance) and projected surface distance (image distance). Both measurements are in reference to the center of the lens.
In order to collect data, the light box was placed at a known distance, and the flat surface was moved until a sharp image was formed. The two relative distances were recorded and put into a table. The plot of Image distance vs. object distance follows.
It appears to have a relationship which approximates a reciprocal, however, a plot of their inverses, when summed provides a more thorough explanation.
It is apparent from this graph that the summation of the reciprocal of the two values is nearly constant. Further investigation reveals that the average value for this summation is approximately 1/focal length.
A magnifying lens can be modelled as a thin lens in the physics of optics because its total thickness is negligible in comparison to the radius of curvature for each surface.
For this experiment we used a light box, a paper with a non symmetric cross printed on it, a magnifying lens, and a flat surface to project the image on.
The above image shows the light box and lens combination.
When the ambient lighting is suppressed and the light box is projected through the lens, an inverted image can be seen on the opposite side of the lens.
Though barely visible in the glass, it is possible to see that the reflection of the cross is both vertically and horizontally inverted from the image that appears on the flat box.
The sharpness and size of the projected image was found to be variant with light box distance (object distance) and projected surface distance (image distance). Both measurements are in reference to the center of the lens.
In order to collect data, the light box was placed at a known distance, and the flat surface was moved until a sharp image was formed. The two relative distances were recorded and put into a table. The plot of Image distance vs. object distance follows.
It appears to have a relationship which approximates a reciprocal, however, a plot of their inverses, when summed provides a more thorough explanation.
It is apparent from this graph that the summation of the reciprocal of the two values is nearly constant. Further investigation reveals that the average value for this summation is approximately 1/focal length.
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