Docsity
Docsity

Prepare for your exams
Prepare for your exams

Study with the several resources on Docsity


Earn points to download
Earn points to download

Earn points by helping other students or get them with a premium plan


Guidelines and tips
Guidelines and tips

heisenberg data sheet labratory, Lecture notes of Quantum Physics

quantum labratory data sheet heisenberg experiment

Typology: Lecture notes

2022/2023

Uploaded on 06/03/2025

deren-2
deren-2 ๐Ÿ‡น๐Ÿ‡ท

2 documents

1 / 2

Toggle sidebar

This page cannot be seen from the preview

Don't miss anything!

bg1
HEISENBERG UNCERTAINTY PRINCIPLE EXPERIMENT
ANALYSIS OF DATA:
๐‘‘ ๐‘ ๐‘–๐‘›๐œƒ = ๐‘›๐œ† ๐‘› = 1, 2,3, โ€ฆ ๐ท๐‘Ž๐‘Ÿ๐‘˜ ๐น๐‘Ÿ๐‘–๐‘›๐‘”๐‘’ (1)
๐‘‘ ๐‘ ๐‘–๐‘›๐œƒ = (๐‘› + 1
2) ๐œ† ๐‘› = 1,2, 3, โ€ฆ๐ต๐‘Ÿ๐‘–๐‘”โ„Ž๐‘ก ๐น๐‘Ÿ๐‘–๐‘›๐‘”๐‘’ (2)
Part I) Single Slit Diffraction:
1. If you are going to use dark points, use Equation 1; if you are going to use bright points, use
Equation 2.
2. In these equations, find sinฮธ by using the distance between the sensor and the laser source,
"L", and the distance of the bright or dark fringe from the centripetal illumination, "y".
3. Record the positions of the bright and dark fringes, 3 on the right side and 3 on the left side
of the centripetal illumination, and the sinฮธ values for these positions in Table 1.
4. Take the average of the wavelength ฮป values you found using Equation 1 or 2.
5. Compare the theoretical wavelength with what you found and calculate the error.
6. Draw the n-sinฮธ graph and calculate the slit width from the slope of this graph, compare it
with the value written on the slit.
Part II) Double Slit Diffraction:
Repeat the same steps as in the Single Slit Diffraction part and fill in Table 2 for this part.
Part I) Single Slit Diffraction: ๐‘ณ =
๐’…๐‘ป๐’‰๐’†๐’๐’“๐’Š๐’„ =
๐€๐‘ป๐’‰๐’†๐’๐’“๐’Š๐’„ =๐Ÿ“๐Ÿ‘๐Ÿ ๐’๐’Ž
TABLE 1
n
Dark Fringes
Bright Fringes
y
(mm)
๐’”๐’Š๐’๐œฝ = ๐’šโˆš(๐‘ณ๐Ÿ+๐’š๐Ÿ)
โ„
ฮป
(nm)
๐’”๐’Š๐’๐œฝ = ๐’šโˆš(๐‘ณ๐Ÿ+๐’š๐Ÿ)
โ„
ฮป
(nm)
-3
-2
-1
0
1
2
3
๐›Œ๐’‚๐’—๐’ˆ
(nm)
๐›Œ๐’‚๐’—๐’ˆ
(nm)
% Error:
Slope = d =
% Error:
pf2

Partial preview of the text

Download heisenberg data sheet labratory and more Lecture notes Quantum Physics in PDF only on Docsity!

HEISENBERG UNCERTAINTY PRINCIPLE EXPERIMENT

ANALYSIS OF DATA:

Part I) Single Slit Diffraction:

  1. If you are going to use dark points, use Equation 1; if you are going to use bright points, use Equation 2.

  2. In these equations, find sinฮธ by using the distance between the sensor and the laser source, "L", and the distance of the bright or dark fringe from the centripetal illumination, "y".

  3. Record the positions of the bright and dark fringes, 3 on the right side and 3 on the left side of the centripetal illumination, and the sinฮธ values for these positions in Table 1.

  4. Take the average of the wavelength ฮป values you found using Equation 1 or 2.

  5. Compare the theoretical wavelength with what you found and calculate the error.

  6. Draw the n-sinฮธ graph and calculate the slit width from the slope of this graph, compare it with the value written on the slit. Part II) Double Slit Diffraction: Repeat the same steps as in the Single Slit Diffraction part and fill in Table 2 for this part. Part I) Single Slit Diffraction: ๐‘ณ = ๐’…๐‘ป๐’‰๐’†๐’๐’“๐’Š๐’„ = ๐€๐‘ป๐’‰๐’†๐’๐’“๐’Š๐’„ = ๐Ÿ“๐Ÿ‘๐Ÿ ๐’๐’Ž TABLE 1 n Dark Fringes Bright Fringes y (mm) ๐’”๐’Š๐’๐œฝ = ๐’š โˆš(๐‘ณ๐Ÿ^ + ๐’š๐Ÿ) โ„ ฮป (nm) y (mm) ๐’”๐’Š๐’๐œฝ = ๐’š โˆš(๐‘ณ๐Ÿ^ + ๐’š๐Ÿ) โ„ **ฮป (nm)

  • 3
  • 2
  • 1 0 1 2 3** ๐›Œ๐’‚๐’—๐’ˆ (nm) ๐›Œ๐’‚๐’—๐’ˆ (nm) % Error: Slope = d = % Error:

Part II) Double Slit Diffraction: TABLE 2 n Dark Fringes Bright Fringes y (mm) ๐’”๐’Š๐’๐œฝ = ๐’š โˆš(๐‘ณ๐Ÿ^ + ๐’š๐Ÿ) โ„ ฮป (nm) y (mm) ๐’”๐’Š๐’๐œฝ = ๐’š โˆš(๐‘ณ๐Ÿ^ + ๐’š๐Ÿ) โ„ ฮป (nm)

**- 3

  • 2
  • 1** 0 1 2 3 ๐›Œ๐’‚๐’—๐’ˆ๐’• (nm) ๐›Œ๐’‚๐’—๐’ˆ (nm) % Error: Slope = d = % Error: III) Verification of Heisenberg's Principle d: ๐›Œ (measured ) : y: L:

sin(arctan )๏€ฝ

L

d y

% Error: