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Abstract

In this experiment, we shall:

Observe and demonstrate the interaction between the magnetic moment of the electron spin with an external magnetic field.

Determine the characteristic parameter of this interaction, namely the Landé g-factor for spin (denoted gs)

Introduction

When we applied an external magnetic field and then by supplying electromagnetic energy on a paramagnetic solid material (which have unpaired electron spins), transitions can be induced between spin states. The resulting absorption spectra are described as electron spin resonance (ESR) or electron paramagnetic resonance (EPR).

ESR is a purely quantum mechanical effect. It relates to the interaction of an external magnetic field to an electron’s magnetic moment, which is a result of intrinsic spin. The spin of an electron may be up or down. This implies that in the presence of an external magnetic field, one spin state will be higher in energy than other. More specially, the spin with a moment pointing in the direction of the external field is lowest in energy. These states have an energy E, as either:

U = -µ.Bs = -µsz B =±(1/2) gs µB B     (1)

Where g is the Lande’ factor, µB is the Bohr magneton (a constant), and B is the value of the external magnetic field. Thus, the change in energy from the negative to the positive spin state can be written:

DE = g µBB             (2)

Therefore, because g and µB are constants, there are pairs of values of the energy E and of the external field B that satisfy Eq. (2) and result in a transition of spin states. At commonly attainable magnetic field strengths the corresponding energy lies in the radio-frequency (RF) regime. Where the general expression for the energy of a photon applies:

E = hv        (3)

Where E is the energy of an RF photon, h is Plank’s constant, and ν is the frequency of the photon. When a photon of energy E is incident on an electron in a field of strength B electron resonance will be observed.



Spin of the electron, The Landé g-factor.

The idea of electron spin and its associated magnetic moment was first introduced by George Uhlenbeck and Samuel Goudsmit to explain the fine structure in atomic optical spectra. A proper relativistic quantum mechanical treatment of the hydrogen atom leads naturally to the electron possessing, in addition to its mass m and charge e, an intrinsic spin angular momentum with quantum number s = 1/2. The new quantum property, the spin, obeys the same quantization rules as those governing orbital angular momentum of atomic electrons. The spin vector S has magnitude :

S = (S(S + 1))^1/2ћ      (4)

In the presence of a magnetic field, the component of spin parallel to the field (z direction) is quantized. It has two possible values,

Sz = msħ = ± (1/2)ħ  (5)



Since an electron has a charge and an angular momentum, it also has a magnetic moment, µL,  proportional to the orbital angular momentum, given by

μl = gl (e/2m) l     (6)

Where gl is the electron orbital momentum g-factor.

The electron also has a magnetic moment, µs, proportional to its spin, and it is given by:

μs= -gs (e/2m)S = ±(1/2) gs (eħ /2m)   (7)

where gs is the electron spin g-factor. According to Dirac’s theory, gs is precisely 2.

Transitions between the states can therefore be excited by photons of frequency nr, given by

hvr = gs μB B  (8)


Free Radicals

The electrons that we will manipulate are located in the paramagnetic molecule Diphenyl-Picryl-Hydrazyl (DPPH). DPPH is pictured below; notice the unpaired electron. This electron is also very weakly bound to the nitrogen atom. The combination of these two properties makes this molecule ideal for studying the magnetic properties of the electron.




Figure 3 shows a block diagram depicting the experimental setup. There are essentially two circuits: The first controls and monitors the RF signal driving of the electrons (at left), and the second controls the external magnetic field (right). You should observe the output of the absorption of the DPPH on one channel of the oscilloscope (DC couple the o-scope channel) and the voltage across the resistor on the other channel.




Helmholtz Coils

The magnetic field is provided by a pair of Helmholtz coils in a series connection with an AC and a DC power supply. The average magnetic field can be determined from the current in the coil which is measured by the DC ammeter.

The characteristic which distinguishes Helmholtz coils from other sources of magnetic field is that the distance between the coils is equal to their radius (R). 

The magnetic field midway between the coils and on their axis is given by:

B= 8μ0NI / √125 R

where I is the current and N is the number of turns in each coil.



    The RF unit

For the typical magnetic fields used in this experiment, photons of frequencies in the range ~25-50MHz are required for the transitions referred to above. These are provided by a short coil connected to a high frequency oscillator. The magnetic field of this coil is perpendicular to that provided by the Helmholtz coils, an arrangement that results in a perturbing torque acting on the electron’s spin dipole moment. When the oscillator frequency matches the resonance condition, the impedance of the oscillator circuit decreases and the current increases. A DC voltage proportional to this current is fed to the Y-input of the oscilloscope.


Methodology


We will use:

- DPPH sample,

- ESR unit: ESR resonator with field coils and ESR power supply

- Oscilloscope

- Teslameter, digital

Procedure

* The setup was ready as the figure above.

* We inserted the sample into large RF coil, then we put the sample at the middle between Helmholtz coils.

* We turned the oscilloscope on, power supply, RF unit and the multimeter at DC amperes.

* We started with 35 MHz up to 75 for the first coil and recorded the current value (the current value was 2I not I).

* We put the second coil and repeat the previous steps starting from 80MHz up to 125MHz.


Data Analysis

Table1: The current of Helmholtz coils  (A), resonance frequency (MHz)


2I(A)

f(MHz)

0.33

20

0.43

25

0.5

30

0.58

35

0.66

40

0.74

45

0.83

50

0.92

55

1.02

60

1.08

65

1.18

70

1.24

75

1.36

80

1.43

85

1.52

90

1.59

95

1.67

100

1.76

105

1.93

110

2

 

2.09

 

2.13

 

Δf=±0.01MHz

ΔI=±0.01 A

N=320 ( Number of turns)

R=6.8 cm ( raduis of one coil)






























2I(A)

I (A)

f(MHz)

B  T

0.33

0.165

20

0.00047685

0.43

0.215

25

0.00062135

0.5

0.25

30

0.0007225

0.58

0.29

35

0.0008381

0.66

0.33

40

0.0009537

0.74

0.37

45

0.0010693

0.83

0.415

50

0.00119935

0.92

0.46

55

0.0013294

1.02

0.51

60

0.0014739

1.08

0.54

65

0.0015606

1.18

0.59

70

0.0017051

1.24

0.62

75

0.0017918

1.36

0.68

80

0.0019652

1.43

0.715

85

0.00206635

1.52

0.76

90

0.0021964

1.59

0.795

95

0.00229755

1.67

0.835

100

0.00241315

1.76

0.88

105

0.0025432

1.93

0.965

110

0.00278885

2

1

115

0.00289

2.09

1.045

120

0.00302005

2.13

1.065

125

0.00307785



To estimate the true value of our slope and y-intercept we use the least square method:


Where a is the intercept and b is the slope, we can find the error in a (δa) and error in b (δb) using the following equations:



where s is the standard deviation  

B  T

f(MHz)

B^2

x*y

(y-a-bx)^2

0.00047685

20

2.27386E-07

0.009537

44.14918224

0.00062135

25

3.86076E-07

0.01553375

32.18162422

0.0007225

30

5.22006E-07

0.021675

27.84430797

0.0008381

35

7.02412E-07

0.0293335

23.82080494

0.0009537

40

9.09544E-07

0.038148

20.11111516

0.0010693

45

1.1434E-06

0.0481185

21.7520854

0.00119935

50

1.43844E-06

0.0599675

23.45740378

0.0013294

55

1.7673E-06

0.073117

31.33918713

0.0014739

60

2.17238E-06

0.088434

16.41105147

0.0015606

65

2.43547E-06

0.101439

23.09679592

0.0017051

70

2.90737E-06

0.119357

10.61995211

0.0017918

75

3.21055E-06

0.134385

26.67366333

0.0019652

80

3.86201E-06

0.157216

17.58171107

0.00206635

85

4.2698E-06

0.17563975

19.11811262

0.0021964

90

4.82417E-06

0.197676

11.56561952

0.00229755

95

5.27874E-06

0.21826725

9.028293602

0.00241315

100

5.82329E-06

0.241315

10.13838582

0.0025432

105

6.46787E-06

0.267036

63.47850827

0.00278885

110

7.77768E-06

0.3067735

48.94037815

0.00289

115

8.3521E-06

0.33235

51.48222217

0.00302005

120

9.1207E-06

0.362406

20.04401341

0.00307785

125

9.47316E-06

0.38473125

15153.95468

0.03900055

1595

8.30719E-05

3.382456

15706.7891


Slope= 27.127(+-)0.251

gs= h*slope/M =1.93818

The theoretical value of gs=2.0023, we will find the percentage error:

𝐏.𝐄 = |𝐠𝐬(𝐞𝐱𝐩𝐞𝐫𝐞𝐦𝐞𝐧𝐭𝐚𝐥𝐥𝐲)−𝐠𝐬(𝐭𝐡𝐞𝐨𝐫𝐢𝐭𝐢𝐜𝐚𝐥𝐥𝐲)| /𝐠𝐬𝐭𝐡𝐞𝐨𝐫𝐭𝐢𝐜𝐚𝐥𝐥𝐲 *100%

= 3.2023%

Error in ∆gs = gs(exp)*∆slope/slope

Error propagation in gs = (+-)0.01793

∆f=+-0.01 MHz

∆I=+-0.01 A


Conclusion

1- The relation between the frequency and the applied magnetic field is linear according to equation 8.

2- The interaction of an external magnetic field with an electron spin depends upon the magnetic moment associated with the spin.

3- Resonance is the absorption of energy from the weak alternating magnetic field of the microwave when its frequency corresponds to the difference between two spin states.

4- Free radical, such as DPPH that we used in our experiment exhibit g-factors very close to the value for free electrons = 2.0023.


 References

1- Practical physics (0342411) manual.

2- https://homepage.physics.uiowa.edu/~fskiff/Physics_132/New%20Lab%20Manual/int_lab_man/pdfs/A4_ESR_v6.pdf 

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