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The objective of this experiment is to measure and analyze the Verdet constant for Corning 7980, a fused silica glass with no previously published Verdet constant data. The Verdet constant is measured by the Faraday effect - a magneto-optical phenomenon that describes the rotation of the plane of polarization of light in a medium in the presence of an external magnetic field. This experiment quantifies the rotation of the polarization plane with respect to wavelength and magnetic field.

Data collected through this experiment shows a linear relationship between the rotation angle and the magnetic field.

INTRODUCTION

MICHAEL FARADAY

THE FARADAY EFFECT

Faraday discovered that when 'heavy glass' is subjected to an external magnetic field, it becomes optically active. When plane-polarized light passes through this glass, parallel to the external magnetic field, there is a rotation in the polarization angle (Figure 1). This rotation depends on the strength of the magnetic field and the distance the light travels within that medium.

Where  is the angle by which the plane of polarization of light is rotated (in radians), 𝐵 is the uniform external magnetic field (in Tesla), 𝑙 is the length of the glass (in meters), and 𝑉 is the Verdet constant. The Verdet constant is characteristic of the medium and is defined as the rotation of the plane of polarization per unit length per unit magnetic field (Jenkins and White 1976).

MOTIVATION: THE BELLE II EXPERIMENT

THE BELLE II DETECTOR

To identify new particles or study new physics, reconstructing the entire event is extremely crucial. To do this, we need to be able to identify all the long-lived daughter particles produced in the interaction. The usual method for identifying a particle is its mass, which is possible if the velocity and momentum of the particle are known.

THE IMAGING TIME OF PROPAGATION DETECTOR

The kaons and pions have different masses and therefore different speeds as they travel through the quartz glass. The Cherenkov radiation emitted by these particles has different Cherenkov opening angles depending on the velocity of the particle. As the radiation travels through the quartz glass, it is captured and channeled by total internal reflection.

The counter detects the propagation time of the radiation with remarkable accuracy and thus distinguishes between the two types of particles (Figure 5). The red arrow in Figure 5 shows the path of the particle as it passes through the TOP counter. A 1.5 Tesla magnetic field exists inside the iTOP that causes a change in the polarization angle of these Cherenkov photons.

The collection efficiency of MC-PMTs in iTOP has a strong dependence on the polarization state of the photons. To achieve a better understanding of photon collection efficiency, the polarization state of these photons must be taken into account. This research project determines the rotation of the polarization angle of Cherenkov photons, inside the iTOP, due to the external magnetic field.

Figure 3 Cherenkov Angle  𝜃 𝑐  (Courtesy of the Belle II collaboration)
Figure 3 Cherenkov Angle 𝜃 𝑐 (Courtesy of the Belle II collaboration)

THE EFFECT OF THE FARADAY EFFECT

The vector sum of the two modes is still linearly polarized, but they undergo a net rotation due to their different velocities (Jenkins and White 1976) (Kroeger, et al. 2015). Where 𝑉𝐵 is the Verdet constant, 𝜔 is the frequency of light, 𝑛0 is the refractive index of the medium, 𝐵 is the magnetic field, 𝑛+ is the refractive index of the right-handed polarization mode and 𝑛− is the refractive index of the left-handed polarization mode (Jenkins and White 1976). As the graph suggests (Figure 6), the change in the incidence angle has a drastic effect on the collection efficiency of the MC-PMTs.

There also exists a strong asymmetry for the transverse electric and transverse magnetic component of the photon polarization for the collection efficiency of the MC-PMTs. This critical angle is unfortunately 43o, the angle at which the collection efficiency (%QE) drops to 7% for the transverse magnetic wave (Kroeger, et al. 2015). Knowing the polarization states of the photons and integrating them into the Mote Carlo analysis will give us a better understanding of photon collection efficiency, and therefore aid in highly accurate particle identification.

Figure 6 The polarization dependence of the collection efficiency of the Micro Channel PMTs as a function  of incidence angle (Courtesy Belle II Collaboration)
Figure 6 The polarization dependence of the collection efficiency of the Micro Channel PMTs as a function of incidence angle (Courtesy Belle II Collaboration)

METHODOLOGY

EXPERIMENTAL SETUP

The experimental setup (Figure 7) used to accurately measure the Verdet constant was partially built by the machine shop at the physics department. Two of the diode lasers (650 nm and 532 nm) were provided as part of the apparatus. The study of the Faraday effect in the shorter wavelengths is crucial since most of the photons detected in the iTOP are near the ultraviolet region of the spectrum.

The polarizer was used to plane polarize the light before it entered the quartz rod. Because the diode lasers were slightly polarized, the angle of the polarizer was chosen so that the maximum amount of light could pass through the glass. Two solenoids (Figure 9) with a length of approximately 21 cm were built in the machine shop of the Physics Department.

The solenoid created a relatively uniform magnetic field and the quartz glass was placed inside it. The quartz sample is a very specific fused silica - Corning 7980, the same material the iTOP is built with. This material was chosen by Belle because of its properties such as uniformity in refractive index, low stress birefringence values, large size capabilities, exceptional transmission from deep ultraviolet through the infrared region, and a ultra low coefficient of thermal expansion.

The quartz glass sample was wrapped in black paper for thermal insulation and to prevent light leakage. The analyzer is another fine angle disc polarizer with a minimum count of 0.1 degrees per division and was used to measure the polarization angle of light after passing the light through quartz glass. A Pin-Hole Photodiode is used to measure the intensity of light after passing through the analyzer.

This instrument was a significant upgrade compared to the one supplied in the instrument set by. As the current passing through the solenoid was changed, the magnetic field changed proportionally, causing a rotation in the polarization angle of the light in the quartz glass.

Figure 8 (Left) Diode Laser. (Right) Polarizer
Figure 8 (Left) Diode Laser. (Right) Polarizer

EXPERIMENTAL PROCEDURE

A precision constant current power supply is connected to the solenoid to produce a constant uniform magnetic field. The exact constant current mode on the power supply played a crucial role in data collection; without this mode it would have been difficult to obtain a constant magnetic field. Now, when the current is turned on, there is a magnetic field inside the solenoid that rotates the polarization plane of the light.

The difference between  and 0 gives the rotation of the polarization angle in the presence of a magnetic field. This process is repeated several times for a given magnetic field and an average is obtained.

RESULTS

ROTATION OF PLANE OF POLARIZATION VS. CURRENT

Here, B is the magnetic field, 𝜇 is the permeability of the medium, n is the number of coil turns per unit length, and I is the current flowing through the coil. The graph shows a very uniform magnetic field along the z-axis except at the ends of the solenoids (Figure 14). The magnetic field in the solenoid was determined using the results observed in the paper by Muniz, Bhattacharya and Bagnato.

This is also repeated for the larger solenoid where the flux is summed for the 14 layers.

Figure 14 The magnetic field within the solenoid for the smaller solenoid along the z-axis
Figure 14 The magnetic field within the solenoid for the smaller solenoid along the z-axis

BECQUEREL FORMULA

The equations presented by Muniz et al. are adapted for this experiment, and the magnetic flux is calculated for each of the fifteen layers of the small solenoid and added to give ∫ 𝐵 ⋅ ⅆ𝑙. 25. was also observed by other authors such as Tan and Arndt when measuring the Verdet constant for a silicate glass called Supracil W2).

Figure 15 Verdet Constant vs. Wavelength
Figure 15 Verdet Constant vs. Wavelength

FINAL EQUATION

ERROR ANALYSIS

  • THE ANALYZER AND BACKLASH ERROR
  • TEMPERATURE DEPENDENCE OF THE VERDET CONSTANT
  • ERROR PROPAGATION IN ∫ 𝐵 ⋅ ⅆ𝑙
  • POWER SUPPLY
  • LIGHT FROM REFLECTION
  • TAN AND ARNDT MODEL
  • FINAL ERROR CALCULATION

The larger solenoid was constructed with 10-gauge wire, and each row was separated with heat-resistant Kapton tape to prevent heat dissipation. When the current was increased to 25A or more and allowed to pass continuously, there was a significant increase in the temperature of the solenoid. Leaving the setup on for longer periods at higher currents can lead to a significant difference in the angle of rotation.

The installation was allowed to cool for 10-15 minutes before the next measurement was taken, and measurements requiring higher currents were taken several times over several days to check for consistency. Part of the uncertainty in the measurement of the Verdet constant is due to. The point at which light enters and exists in the glass rod is given by (s, z);.

However, a shift from this central position would contribute to the error in the magnetic field experienced by the light. The high-precision power supply in constant current mode has an error of less than ±10 mA in the current output. Light reflecting from the faces of the glass sample passes through the sample twice more before hitting the photodiode and therefore has a different polarization angle.

The maximum rotation observed is about 7 degrees for 7.2 amperes, this means that the light after reflecting twice has rotated 21 degrees. Statistical errors in the calculation of the Verdet constant for individual wavelengths propagate into the Tan and Arndt model. The most important sources of systematic errors include the inaccuracy of the current supply and light from reflections.

When added in quadrature, this adds up to a total of 0.199 % systematic error in the measurement.

Figure 18 The sample is placed off center Solenoid
Figure 18 The sample is placed off center Solenoid

CONCLUSION AND FUTURE WORK

Considering the final polarization angle of the photons when they reach the photomultiplier tubes would certainly increase the understanding of the efficiency with which the photons and thus the particles can be detected. Most of the photons in the glass rod in the iTOP are located in this region of the.

Gambar

Figure 1  Rotation of the plane of polarization of light within a medium due to an external magnetic field
Figure 2 iTOP Quartz bar
Figure 4 Cherenkov radiation as it travels through the quartz bar
Figure 3 Cherenkov Angle  𝜃 𝑐  (Courtesy of the Belle II collaboration)
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