Pulsed Nuclear Magnetic Resonance
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UC Berkeley UC Berkeley Electronic Theses and Dissertations
UC Berkeley UC Berkeley Electronic Theses and Dissertations Title Applications of Magnetic Resonance to Current Detection and Microscale Flow Imaging Permalink https://escholarship.org/uc/item/2fw343zm Author Halpern-Manners, Nicholas Wm Publication Date 2011 Peer reviewed|Thesis/dissertation eScholarship.org Powered by the California Digital Library University of California Applications of Magnetic Resonance to Current Detection and Microscale Flow Imaging by Nicholas Wm Halpern-Manners A dissertation submitted in partial satisfaction of the requirements for the degree of Doctor of Philosophy in Chemistry in the Graduate Division of the University of California, Berkeley Committee in charge: Professor Alexander Pines, Chair Professor David Wemmer Professor Steven Conolly Spring 2011 Applications of Magnetic Resonance to Current Detection and Microscale Flow Imaging Copyright 2011 by Nicholas Wm Halpern-Manners 1 Abstract Applications of Magnetic Resonance to Current Detection and Microscale Flow Imaging by Nicholas Wm Halpern-Manners Doctor of Philosophy in Chemistry University of California, Berkeley Professor Alexander Pines, Chair Magnetic resonance has evolved into a remarkably versatile technique, with major appli- cations in chemical analysis, molecular biology, and medical imaging. Despite these successes, there are a large number of areas where magnetic resonance has the potential to provide great insight but has run into significant obstacles in its application. The projects described in this thesis focus on two of these areas. First, I describe the development and implementa- tion of a robust imaging method which can directly detect the effects of oscillating electrical currents. This work is particularly relevant in the context of neuronal current detection, and bypasses many of the limitations of previously developed techniques. -
Thomas Precession and Thomas-Wigner Rotation: Correct Solutions and Their Implications
epl draft Header will be provided by the publisher This is a pre-print of an article published in Europhysics Letters 129 (2020) 3006 The final authenticated version is available online at: https://iopscience.iop.org/article/10.1209/0295-5075/129/30006 Thomas precession and Thomas-Wigner rotation: correct solutions and their implications 1(a) 2 3 4 ALEXANDER KHOLMETSKII , OLEG MISSEVITCH , TOLGA YARMAN , METIN ARIK 1 Department of Physics, Belarusian State University – Nezavisimosti Avenue 4, 220030, Minsk, Belarus 2 Research Institute for Nuclear Problems, Belarusian State University –Bobrujskaya str., 11, 220030, Minsk, Belarus 3 Okan University, Akfirat, Istanbul, Turkey 4 Bogazici University, Istanbul, Turkey received and accepted dates provided by the publisher other relevant dates provided by the publisher PACS 03.30.+p – Special relativity Abstract – We address to the Thomas precession for the hydrogenlike atom and point out that in the derivation of this effect in the semi-classical approach, two different successions of rotation-free Lorentz transformations between the laboratory frame K and the proper electron’s frames, Ke(t) and Ke(t+dt), separated by the time interval dt, were used by different authors. We further show that the succession of Lorentz transformations KKe(t)Ke(t+dt) leads to relativistically non-adequate results in the frame Ke(t) with respect to the rotational frequency of the electron spin, and thus an alternative succession of transformations KKe(t), KKe(t+dt) must be applied. From the physical viewpoint this means the validity of the introduced “tracking rule”, when the rotation-free Lorentz transformation, being realized between the frame of observation K and the frame K(t) co-moving with a tracking object at the time moment t, remains in force at any future time moments, too. -
Magnetic Moment of a Spin, Its Equation of Motion, and Precession B1.1.6
Magnetic Moment of a Spin, Its Equation of UNIT B1.1 Motion, and Precession OVERVIEW The ability to “see” protons using magnetic resonance imaging is predicated on the proton having a mass, a charge, and a nonzero spin. The spin of a particle is analogous to its intrinsic angular momentum. A simple way to explain angular momentum is that when an object rotates (e.g., an ice skater), that action generates an intrinsic angular momentum. If there were no friction in air or of the skates on the ice, the skater would spin forever. This intrinsic angular momentum is, in fact, a vector, not a scalar, and thus spin is also a vector. This intrinsic spin is always present. The direction of a spin vector is usually chosen by the right-hand rule. For example, if the ice skater is spinning from her right to left, then the spin vector is pointing up; the skater is rotating counterclockwise when viewed from the top. A key property determining the motion of a spin in a magnetic field is its magnetic moment. Once this is known, the motion of the magnetic moment and energy of the moment can be calculated. Actually, the spin of a particle with a charge and a mass leads to a magnetic moment. An intuitive way to understand the magnetic moment is to imagine a current loop lying in a plane (see Figure B1.1.1). If the loop has current I and an enclosed area A, then the magnetic moment is simply the product of the current and area (see Equation B1.1.8 in the Technical Discussion), with the direction n^ parallel to the normal direction of the plane. -
Electron Spins in Nonmagnetic Semiconductors
Electron spins in nonmagnetic semiconductors Yuichiro K. Kato Institute of Engineering Innovation, The University of Tokyo Physics of non-interacting spins Optical spin injection and detection Spin manipulation in nonmagnetic semiconductors Physics of non-interacting spins 2 In non-magnetic semiconductors such as GaAs and Si, spin interactions are weak; To first order approximation, they behave as non-interacting, independent spins. • Zeeman Hamiltonian • Bloch sphere • Larmor precession ∗ • , , and • Bloch equation The Zeeman Hamiltonian 3 Hamiltonian for an electron spin in a magnetic field magnetic moment of an electron spin : magnetic moment : magnetic field : Landé g-factor (=2 for free electrons) : Bohr magneton 58 eV/T , ) : electronic charge : Planck constant : free electron mass : spin operator : Pauli operator The Zeeman Hamiltonian 4 Hamiltonian for an electron spin in a magnetic field magnetic moment of an electron spin : magnetic moment : magnetic field : Landé g-factor (=2 for free electrons) : Bohr magneton 2 58 eV/T : electronic charge : Planck constant : free electron mass : spin operator 2 : Pauli operator The energy eigenstates 5 Without loss of generality, we can set the -axis to be the direction of , i.e., 0,0, 1 Spin “up” |↑ |↑ 2 1 2 2 1 Spin “down” |↓ |↓ 2 1 2 2 Spinor notation and the Pauli operators 6 Quantum states are represented by a normalized vector in a Hilbert space Spin states are represented by 2D vectors Spin operators are represented by 2x2 matrices. -
4 Nuclear Magnetic Resonance
Chapter 4, page 1 4 Nuclear Magnetic Resonance Pieter Zeeman observed in 1896 the splitting of optical spectral lines in the field of an electromagnet. Since then, the splitting of energy levels proportional to an external magnetic field has been called the "Zeeman effect". The "Zeeman resonance effect" causes magnetic resonances which are classified under radio frequency spectroscopy (rf spectroscopy). In these resonances, the transitions between two branches of a single energy level split in an external magnetic field are measured in the megahertz and gigahertz range. In 1944, Jevgeni Konstantinovitch Savoiski discovered electron paramagnetic resonance. Shortly thereafter in 1945, nuclear magnetic resonance was demonstrated almost simultaneously in Boston by Edward Mills Purcell and in Stanford by Felix Bloch. Nuclear magnetic resonance was sometimes called nuclear induction or paramagnetic nuclear resonance. It is generally abbreviated to NMR. So as not to scare prospective patients in medicine, reference to the "nuclear" character of NMR is dropped and the magnetic resonance based imaging systems (scanner) found in hospitals are simply referred to as "magnetic resonance imaging" (MRI). 4.1 The Nuclear Resonance Effect Many atomic nuclei have spin, characterized by the nuclear spin quantum number I. The absolute value of the spin angular momentum is L =+h II(1). (4.01) The component in the direction of an applied field is Lz = Iz h ≡ m h. (4.02) The external field is usually defined along the z-direction. The magnetic quantum number is symbolized by Iz or m and can have 2I +1 values: Iz ≡ m = −I, −I+1, ..., I−1, I. -
Optical Detection of Electron Spin Dynamics Driven by Fast Variations of a Magnetic Field
www.nature.com/scientificreports OPEN Optical detection of electron spin dynamics driven by fast variations of a magnetic feld: a simple ∗ method to measure T1 , T2 , and T2 in semiconductors V. V. Belykh1*, D. R. Yakovlev2,3 & M. Bayer2,3 ∗ We develop a simple method for measuring the electron spin relaxation times T1 , T2 and T2 in semiconductors and demonstrate its exemplary application to n-type GaAs. Using an abrupt variation of the magnetic feld acting on electron spins, we detect the spin evolution by measuring the Faraday rotation of a short laser pulse. Depending on the magnetic feld orientation, this allows us to measure either the longitudinal spin relaxation time T1 or the inhomogeneous transverse spin dephasing time ∗ T2 . In order to determine the homogeneous spin coherence time T2 , we apply a pulse of an oscillating radiofrequency (rf) feld resonant with the Larmor frequency and detect the subsequent decay of the spin precession. The amplitude of the rf-driven spin precession is signifcantly enhanced upon additional optical pumping along the magnetic feld. Te electron spin dynamics in semiconductors can be addressed by a number of versatile methods involving electromagnetic radiation either in the optical range, resonant with interband transitions, or in the microwave as well as radiofrequency (rf) range, resonant with the Zeeman splitting1,2. For a long time, the optical methods were mostly represented by Hanle efect measurements giving access to the spin relaxation time at zero magnetic feld3. New techniques giving access both to the spin g factor and relaxation times at arbitrary magnetic felds have been very actively developed. -
Griffith's Example 4.3: Larmor Precession We Will Be Considering the Spin of an Electron
Griffith's Example 4.3: Larmor Precession We will be considering the spin of an electron. The operator for the component of spin in the rˆ = (sin cosijˆˆ sin sin cosˆ ) k cos sin ei cos(½ ) leading to Sˆ which has an eigen-spinor rˆ rˆ i i sin e cos sin(½ )e i rˆ sin(½ )e with eigenvalue ½ and with eigenvalue -½ . We can imagine a cos(½ ) state in which the spin is initially in the x-z plane and makes an angle relative to the cos(½ ) z axis so (0) . sin(½ ) First we consider an applied magnetic field in the z direction providing interaction ˆ ˆ energy: H Bkozo SB Bmos. Using the standard eigenstates of Sz, ½0 B ˆ o H 0½ Bo Note that the difference between the energies of the spin up and spin down states is Bo. We expect things to oscillate at frequencies corresponding to the energy differences so the frequency for this problem is Bo, the Larmor frequency. The frequencies associated with the two states have a magnitude of one-half of the Larmor frequency; the difference between the frequencies is the relevant frequency for oscillation of probability density or, in this case, precessing. The hamiltonian is diagonal so the spin z up and down states are the eigenfunctions. a ½it ½0 Bo a cos(½ )e Hiˆ it () t t b ½it 0½ Bo b t sin(½ )e where = Bo . The expectation values can be computed with the results: Sz(t) = cos() ( /2); Sx(t) = sin() ( /2) sin(t);Sy(t) = -sin() ( /2) cos(t) Exercise: Compute Sz(t) and Sx(t) for(t) given above. -
II Spins and Their Dynamics
For the spins to precess, and for us to detect them, II we need to somehow force them away from Spins and their equilibrium – for example, make them perpendicular to the main field: Dynamics Lecture notes by Assaf Tal B0 1. Excitation 1.1 WhyU Excite? If we do this and let them be, two things will Let us recant the facts from the previous lecture: happen: 1 1. We’re interested in the bulk 1. They will precess about B0 at a rate gB0. (macroscopic) magnetization. 2. Eventually they will return to equilibrium 2. When put in a constant magnetic field, because of thermal relaxation. This this bulk magnetization tends to align usually takes ~ 1sec, but can vary. itself along the field: Until they return to thermal equilibrium their signal is “up for grabs”, which is precisely the idea of a basic NMR/MRI experiment: B0 1. Excite the spins. 2. Measure until they return to sum equilibrium. What to exactly do with the measured signal and how to recover an image from it is something we’ll discuss in subsequent lectures. Meanwhile, let’s Microscopic Macroscopic just ask ourselves how can one excite a spin? That is, how can one tilt it from its equilibrium position along the main field and create an angle between 3. The macroscopic magnetization precesses them (usually 90 degrees, but not always)? about the external magnetic field. 1.2 TheU RF Coils In MRI, we can only detect a signal from the spins if they precess and therefore induce a current in Fortunately (or perhaps unfortunately), our our MRI receiver coils by Faraday’s law. -
Cond-Mat.Supr-Con] 1 Sep 2004 Hnn B Lcutoso H W Ee Ytm Nteoxi the in Systems Level Two 1 the of Fluctuations (B) De Phonon
Decoherence of a Josephson qubit due to coupling to two level systems Li-Chung Ku and C. C. Yu Department of Physics, University of California, Irvine, California 92697, U.S.A. (Dated: October 30, 2018) Abstract Noise and decoherence are major obstacles to the implementation of Josephson junction qubits in quantum computing. Recent experiments suggest that two level systems (TLS) in the oxide tunnel barrier are a source of decoherence. We explore two decoherence mechanisms in which these two level systems lead to the decay of Rabi oscillations that result when Josephson junction qubits are subjected to strong microwave driving. (A) We consider a Josephson qubit coupled resonantly to a two level system, i.e., the qubit and TLS have equal energy splittings. As a result of this resonant interaction, the occupation probability of the excited state of the qubit exhibits beating. Decoherence of the qubit results when the two level system decays from its excited state by emitting a phonon. (B) Fluctuations of the two level systems in the oxide barrier produce fluctuations and 1/f noise in the Josephson junction critical current Io. This in turn leads to fluctuations in the qubit energy splitting that degrades the qubit coherence. We compare our results with experiments on Josephson junction phase qubits. PACS numbers: 03.65.Yz, 03.67.Lx, 85.25.Cp arXiv:cond-mat/0409006v1 [cond-mat.supr-con] 1 Sep 2004 1 I. INTRODUCTION The Josephson junction qubit is a leading candidate as a basic component of a quantum computer. A significant advantage of this approach is scalability, as these qubits may be readily fabricated in large numbers using integrated-circuit technology. -
Semiclassical Approach to Atomic Decoherence by Gravitational Waves
Semiclassical approach to atomic decoherence by gravitational waves Diego A. Qui˜nones, Benjamin Varcoe August 2, 2018 Abstract A new heuristic model of interaction of an atomic system with a gravitational wave is proposed. In it, the gravitational wave alters the local electromagnetic field of the atomic nucleus, as perceived by the electron, changing the state of the system. The spectral decomposition of the wave function is calculated, from which the energy is obtained. The results suggest a shift in the difference of the atomic energy lev- els, which will induce a small detuning to a resonant transition. The detuning increases with the quantum numbers of the levels, making the effect more prominent for Rydberg states. We performed calcu- lations on the Rabi oscillations of atomic transitions, estimating how they would vary as a result of the proposed effect. 1 Introduction In general relativity, gravity is the curvature of the space-time continuum produced by the mass of objects [41]. Similar to how accelerating electrical charges produce electromagnetic waves, accelerating masses will produce rip- ples in the fabric of space-time [16, 17], which are called gravitational waves (GWs). They are predicted to exist in a very wide range of frequencies, de- pending on the source that generate them [2, 11, 14, 27, 29, 30, 37, 39, 40, 44], but even the most energetic ones (like the ones produced by rotating neutron stars [3]) will only produce a very small distortion of space, making them arXiv:1706.01287v3 [quant-ph] 1 Dec 2017 very hard to detect. Although GWs have been previously observed indirectly [43], it was only re- cently that a direct detection was performed by analyzing the signal of very big interferometers [18–20]. -
Charge Qubit Coupled to Quantum Telegraph Noise
Charge Qubit Coupled to Quantum Telegraph Noise Florian Schröder München 2012 Charge Qubit Coupled to Quantum Telegraph Noise Florian Schröder Bachelorarbeit an der Fakultät für Physik der Ludwig–Maximilians–Universität München vorgelegt von Florian Schröder aus München München, den 20. Juli 2012 Gutachter: Prof. Dr. Jan von Delft Contents Abstract vii 1 Introduction 1 1.1 Time Evolution of Closed Quantum Systems . .... 2 1.1.1 SchrödingerPicture........................... 2 1.1.2 HeisenbergPicture ........................... 3 1.1.3 InteractionPicture ........................... 3 1.2 Description of the System of Qubit and Bath . ..... 4 2 Quantum Telegraph Noise Model 7 2.1 Hamiltonian................................... 7 2.2 TheMasterEquation.............................. 7 2.3 DMRGandModelParameters. 11 2.3.1 D, ∆, γ and ǫd ............................. 11 2.3.2 DiscretizationandBathLength . 11 3 The Periodically Driven Qubit 15 3.1 TheFullModel ................................. 15 3.2 RabiOscillations ................................ 15 3.2.1 Pulses .................................. 17 3.3 Bloch-SiegertShift .............................. 18 3.3.1 Finding the Bloch-Siegert Shift . .. 18 3.4 DrivenQubitCoupledtoQTN ........................ 21 3.5 Simulations of Spin Echo and Bang-Bang with Ideal π-Pulses. 23 4 Conclusion and Outlook 27 A Derivations 29 A.1 MasterEquation ................................ 29 A.1.1 ProjectionOperatorMethod. 29 A.1.2 Interaction Picture Hamiltonian . ... 31 A.1.3 BathCorrelationFunctions . 33 A.2 DiscreteFourierTransformation . ..... 36 vi Contents A.3 SolutionoftheRabiProblem . 39 A.3.1 Rotating-Wave-Approximation . .. 39 A.3.2 Bloch-SiegertShift ........................... 40 A.4 Jaynes-Cummings-Hamiltonian . ... 41 Bibliography 47 Acknowledgements 48 Abstract I simulate the time evolution of a qubit which is exposed to quantum telegraph noise (QTN) with the time-dependent density matrix renormalization group (t-DMRG). -
Vortices in a Trapped Dilute Bose–Einstein Condensate
INSTITUTE OF PHYSICS PUBLISHING JOURNAL OF PHYSICS: CONDENSED MATTER J. Phys.: Condens. Matter 13 (2001) R135–R194 www.iop.org/Journals/cm PII: S0953-8984(01)08644-1 TOPICAL REVIEW Vortices in a trapped dilute Bose–Einstein condensate Alexander L Fetter and Anatoly A Svidzinsky Department of Physics, Stanford University, Stanford, CA 94305-4060, USA Received 29 November 2000, in final form 2 February 2001 Abstract We review the theory of vortices in trapped dilute Bose–Einstein condensates and compare theoretical predictions with existing experiments. Mean-field theory based on the time-dependent Gross–Pitaevskii equation describes the main features of the vortex states, and its predictions agree well with available experimental results. We discuss various properties of a single vortex, including its structure, energy, dynamics, normal modes, and stability, as well as vortex arrays. When the nonuniform condensate contains a vortex, the excitation spectrum includes unstable (‘anomalous’) mode(s) with negative frequency. Trap rotation shifts the normal-mode frequencies and can stabilize the vortex. We consider the effect of thermal quasiparticles on vortex normal modes as well as possible mechanisms for vortex dissipation. Vortex states in mixtures and spinor condensates are also discussed. Contents 1. Introduction 2. The time-dependent Gross–Pitaevskii equation 2.1. Unbounded condensate 2.2. Quantum-hydrodynamic description of the condensate 2.3. Vortex dynamics in two dimensions 2.4. Trapped condensate 3. Static vortex states 3.1. Structure of a single trapped vortex 3.2. Thermodynamic critical angular velocity for vortex stability 3.3. Experimental creation of a single vortex 3.4. Vortex arrays 4.