Magnetic Resonance In Studying Natural And Synthetic Materials

By Victor V. Rodin

This book describes nuclear magnetic resonance NMR methods which are used to study translational dynamics of molecules in different complex systems including systems made of synthetic and natural polymers, tissues and the porous heterogeneous systems of

• Language: English
• Publisher: Bentham Science Publishers
• Release date: Nov 2, 2018
• ISBN: 9781681086293

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NMR

Basic Principles of NMR and Experimental Techniques

Victor V. Rodin

Abstract

This chapter introduces into NMR methods as the most important techniques for studying materials. The behaviour of spin system is considered in crossing magnetic fields from classical point of view. Basic equations for the vector of the bulk magnetisation M in outer magnetic field (Bloch equations) are discussed in rotating coordinate system. Spin-lattice (longitudinal) relaxation and spin-spin (transverse) relaxation are considered. The chapter describes the NMR experimental techniques for studying relaxation times T1, T2 and cross-relaxation. The role of proton exchange between the water and exchangeable protons of macromolecules is considered. Pulsed field gradient (PFG) NMR techniques are described for application in one- and two-dimensions. Double-quantum-filtered (DQF) NMR spectroscopy is introduced as a technique to study the materials with anisotropic motion of molecules.

Keywords: Apparent diffusion coefficient Dapp, Double-quantum-filter (DQF) NMR, Fourier transform (FT), Free induction decay (FID), Inverse Laplace transformation (ILT), Nuclear Magnetic Resonance, Pulsed Field Gradient (PFG), Radio frequency (RF), Residual dipolar interaction (RDI), Spin-echo (SE), Spin-lattice (longitudinal) relaxation time T1, Spin-spin (transverse) relaxation time T2, Stimulated echo (STE), Two-dimensional diffusion-diffusion correlation NMR spectroscopy (2D DDCOSY).

INTRODUCTION TO NMR

The methods based on the phenomenon of nuclear magnetic resonance (NMR) are effectively used in different fields of physics, chemistry, biology, and applied areas for the investigation of properties and structure of materials [1-3]. At present, NMR is the most important technique to study molecular motion and to characterize materials. Many NMR books describe both basic principles of realization of NMR phenomenon in applied techniques and specific topics which provides in-depth state of the reviews on NMR applications in various fields [1-7].

For understanding NMR methods, the magnetic properties of atomic nuclei should be considered at first. Atoms consist of a dense, positively charged nucleus, which is surrounded at a relatively large distance by negatively charged electrons. The particles in atoms (electrons, protons and neutrons) can be imagined as spinning on their axes. In some atoms, e.g., ¹²C, these spins are paired against each other and the nucleus of the atom has no overall spin. However, in other atoms, such as ¹H, ¹³C, and ³¹P, the nucleus does possess an overall spin. The nuclei with spin experience NMR phenomenon. There are a large number of nuclei, which do have a nonzero spin angular momentum. NMR is a phenomenon, which occurs when the nuclei of atoms with nonzero spin are placed in a static magnetic field and a second oscillating magnetic field is applied [2-5].

The rules for determining the net spin of a nucleus are described as follows. If the number of neutrons and the number of protons are both even, then the nucleus has no spin. If the number of neutrons plus the number of protons is odd, then the nucleus has a half-integer spin, i.e, 1/2, 3/2, 5/2. For instance, the nuclei ¹H, ¹⁵N, ¹³C, ¹⁹F, ³¹P, and ¹²⁹Xe have the spin 1/2. The nuclei ⁷Li, ¹¹B, ²³Na, ³⁹K, and ¹³¹Xe have the spin 3/2.

If the number of neutrons and the number of protons are both odd, then the nucleus has an integer spin, i.e, 1, 2, 3. For example, the nuclei ²H and ¹⁴N have integer spin 1, and the nuclei ¹⁰B and ²²Na have spin 3.

NMR is a quantum phenomenon [4-9]. Quantum mechanics tells us that this nuclear spin is characterised by a nuclear spin quantum number, I. According to quantum mechanics, a nucleus of spin I will have 2I + 1 possible orientations in magnetic field. An interaction of the spin-half nucleus (I = 1/2) with a magnetic field results in two energy levels. In the absence of an external magnetic field, these orientations are of equal energy. If a magnetic field is applied, then the energy levels split. Each level is given by a magnetic quantum number, m. According to quantum mechanics, m value is restricted to the values from −I to I in integer steps. Thus, for a spin-half nucleus, there are only two values of magnetic quantum number m, +1/2 and −1/2.

There is a tradition in NMR to denote the energy state with m =+1/2 as α, which is often described as spin up notation. The state with m = −1/2 is denoted β and is then described as spin down notation. The m values (+1/2, −1/2) express the parallel and antiparallel orientations of the nuclear spin with respect to the applied magnetic field. Thus, these orientations are described by spin basic functions (α, β). The state with basic function α is the one with the lowest energy [4, 7]. According to quantum mechanics, m value is the eigenvalue of the spin operator I. Thus, these two eigenfunctions have the properties as shown in eq. (1):

Here, eigenvalues are expressed in units of ħ=h/2π [4]. The details of energy levels for two or more spins in molecule can be found elsewhere in literature [1, 3-9].

When the nucleus is in a magnetic field, the initial populations of the energy levels are determined by thermodynamics in accordance with the Boltzmann distribution. It does mean that in the state of equilibrium the lower energy level will contain slightly more nuclei than the higher level. It is possible to excite the nuclei from the low level into the higher level with an electromagnetic radiation. The frequency of radiation needed is determined by the difference in energy between the energy levels ΔE = Eβ–Eα.

When positive charged nucleus is spinning, this generates a small magnetic field. Therefore, the nucleus possesses a magnetic moment µ. This magnetic moment is proportional to its spin I, Planck’s constant h, and the constant γ, which is called the gyromagnetic ratio [4, 5, 9]. γ for nucleus is a ratio of magnetic dipole moment to its angular momentum. γ is a fundamental nuclear constant, which has a different value for every nucleus [2-4]. The energy Em of each energy level m is proportional to the strength of the magnetic field at the nucleus B0, magnetic quantum number m and γh. So, the transition energy ΔE, considered as the difference in energy between levels, will be also proportional to B0. If the magnetic field B0 is increased, then ΔE value is also increased. When a nucleus has a relatively large gyromagnetic ratio, ΔE is large too. In order to understand how a radiation is absorbed by nucleus in a magnetic field, the behaviour of a charged particle in a magnetic field would be better considered from a classical point of view. Let us imagine a nucleus (I = 1/2) in a magnetic field. This nucleus is in a base state, i.e., at the lower energy level and its magnetic moment does not oppose the applied field. The nucleus is spinning on its axis. In the presence of a magnetic field, this axis of rotation will precess around the magnetic field. The frequency of precession is called the Larmor frequency. The Larmor frequency is identical to the transition frequency. The potential energy of the precessing nucleus is given by E = –µ.B0.cosφ, where φ is the angle between the direction of the applied field and the axis of nuclear rotation. The angle of precession, φ, will change when energy is absorbed by the nucleus. For a nucleus with spin of 1/2, the magnetic moment is flipped by absorption of radiation so that it opposes the applied field. An adsorption of energy results in the higher energy state. Due to the difference in population of levels in the state of equilibrium, there is a macroscopic magnetization M, oriented along the direction of magnetic field B0 (Z-axis).

NMR experiments are performed on the nuclei of atoms. The information obtained about the nuclei is used to clarify the chemical environment of many particular nuclei [1-5]. NMR researcher normally uses quite often one-dimensional NMR techniques to study chemical structures in frequency domain. In order to determine the structure of complex molecules, in particular, protein structures, two-dimensional techniques are used [4, 7, 9]. Using the time-domain NMR measurements, researchers can study molecular dynamics in solutions, viscous liquids, gels, pastes as well as liquids in porous media [3, 6, 8, 10-12]. Liquids filled in porous materials can follow different dynamics at sub-zero temperatures. Different fractions of porous liquids can be discovered [5, 6, 8]. On the base of time-domain NMR experiments, a method for the estimation of the pore sizes and characterization of the materials can be developed.

NMR spectroscopy applies Fourier transformation to transfer data between time-domain and frequency-domain. The Fourier transform (FT) is a mathematical technique for converting data from time-domain to data in frequency-domain, and an inverse Fourier transform (IFT) converts data from frequency-domain to time-domain. So, FT is defined as shown in eq. (2), in which f(t) corresponds to the time-domain function; F(ω) corresponds to the spectrum in the frequency-domain.

F(ω) in eq. (2) is a complex function consisting of a real and an imaginary parts. It is equally valid to display the spectrum by using either the real part or the imaginary part as the frequency-domain function. In 1D NMR, the spectrum is usually represented by the real part to display the absorption signal [5, 9]. The Fourier transform is relatively simple procedure, i.e., it is possible to implement this on a computer and to generate the frequency-domain signal (spectrum) from the time-domain signal.

According to a classical point of view, a behaviour of spin system in crossing magnetic fields (alternative magnetic field B1(t) = B1m.cos(ωt) is perpendicular to constant magnetic field B0) is considered on the base of movement of magnetization vector M. Basic equations for the vector of the bulk magnetization M in outer magnetic field are the differential Bloch equations with taking into account the spin-lattice and spin-spin relaxations [3, 5, 6, 8]. These equations are much easier in a rotating coordinate system X´Y´Z´, which rotates with frequency ω around B0 (Z, Z´-axes) in the direction of nuclear precession [3, 5]. In rotation frame, vector M rotates around magnetic field B1 (X´-axis). In the absence of magnetic field B1, magnetization M is along the direction of outer magnetic field B0. The angle frequency of rotation of vector M around X´-axis is ω = γB1. The angle θ for rotation of magnetization M during time tp is presented as θ = γB1tp [3, 5]. If vector M turns by θ = 90° during time tp, then this rotation is called as a 90° or π/2 pulse (duration time tp is called the pulse length). When θ=180°, then this rotation is called as a π pulse.

An application of π/2 pulse to the magnetization M (when originally field B1 was absent and only field B0 did work) results in vector M being along the Y´-axis and the intensity of measurable signal (along Y´-axis) has maximal value. During the time (because of relaxation processes) a projection of magnetization vector M to the Y´-axis will decrease. This detected signal is called as a free induction decay (FID). Fig. (1) shows typical FID (top) and NMR spectrum (bottom) produced in frequency-domain.

SPIN-LATTICE AND SPIN-SPIN NMR RELAXATION

In NMR spectroscopy on protons, the signal intensity depends on the population difference between the two energy levels. The system is irradiated with a frequency, whose energy is equal to the difference in energy between these two energy levels. The transitions will be induced from the lower energy level to the higher and also in the reverse direction. Upward transitions absorb energy and downward transitions release energy. The probability for transitions in either direction is the same. The number of transitions in either direction is determined by multiplying the initial level population by a probability. A population of the initial level is determined by thermodynamics in accordance with the Boltzmann distribution.

The nuclei, which are in a lower energy state, can absorb radiation. This is a small proportion of nuclei. At absorption of radiation, a nucleus jumps to the higher energy state. When the populations of the energy levels are the same, the number of transitions in either direction will also be the same. Therefore, the absorption and release of energy will balance each other to zero. Then, there will be no further absorption of radiation in this case. Thus, the spin system will be saturated. However, a possibility of saturation means that the relaxation processes would occur to return nuclei to the lower energy state.

In order to avoid saturation, the populations of the levels should go back to the states at equilibrium. It does mean that nuclei from the higher energy state return to the state with lower energy. Emission of radiation is insignificant because the probability of re-emission of photons varies with the cube of the frequency. At radio frequencies, re-emission is negligible. Commonly, the NMR researcher would like relaxation rates to be fast but not too fast. If the relaxation rate is fast, then saturation is reduced. If the relaxation rate is too fast, line-broadening in the resultant NMR spectrum is observed. There are two major relaxation processes: (1) spin-lattice (longitudinal) relaxation and (2) spin-spin (transverse) relaxation.

Fig. (1))

FID signal (top) and ¹H NMR spectrum in frequency domain (bottom) for water protons of cement paste (water to cement ratio of 0.4). Age =3 days. T=298 K. Frequency for protons is 400 MHz. The Fourier transform between time domain (top) and frequency domain (bottom) has been performed using software MestreC. Frequency scale (bottom) is presented in points (pt): 50 pts correspond to 12 kHz.

Spin-Lattice (Longitudinal) Relaxation

All nuclei in the sample that are not observable are considered as lattice. Nuclei in the lattice are in vibrational and rotational motion which creates a complex magnetic field. The magnetic field caused by motion of nuclei within the lattice is called the lattice field. The components of the lattice field, which are equal in frequency and phase to the Larmor frequency of the considered nuclei, can interact with nuclei in the higher energy state, and cause them to lose energy and to return to the lower state. The effect of a resonant radio frequency (RF) pulse is to disturb the system of spins from its equilibrium state. The equilibrium is considered as a state of polarization with magnetization M0 directed along the longitudinal magnetic field B0. The restoration of the equilibrium is named longitudinal relaxation. This process can be described by eq. (3):

The relaxation time constant, T1, describes the average lifetime of nuclei in the higher energy state. T1 is typically in the range of 0.1 - 20 sec for protons in non-viscous liquids and other dielectric materials at room temperatures. A larger T1 indicates a slower or more inefficient spin relaxation [1-3]. T1 is dependent on the gyromagnetic ratio of nucleus and the mobility of lattice. As mobility increases, the vibrational and rotational frequencies increase, making it more likely for a component of the lattice field to be able to interact with the excited nuclei. However, at extremely high mobility, the probability of a component of the lattice field being able to interact with the excited nuclei decreases. The efficiency of spin-lattice relaxation depends on factors that influence molecular movement in the lattice, such as viscosity and temperature. The relaxation process is kinetically first order. The applications of relaxation times are very important as they are used in the determination of the mobility of macromolecules and studying intra- and intermolecular interactions. Understanding the relaxation processes and relaxation times is essential in MRI studies. In order to monitor the different MR signals in various soft tissues, the pulse sequences, which include T1-weighted sequences, are applied. T1-weighted sequences are designed for obtaining the images and evaluation of anatomic structures.

The longitudinal relaxation times are often measured using the inversion-recovery pulse sequence (180°–τ‒90°) [5, 8, 10-12]. Here τ is the time gap between 180° and 90° pulses. With the aid of the 1st RF pulse, the equilibrium magnetization M0 rotates by 180° and becomes oriented along the –Z´-axis. During spin-lattice relaxation process, the magnetization changes from –M0 via 0 towards the equilibrium magnetization M0. After time τ, if a 90°x pulse (with B1 oriented along the X´-axis) is applied to the system, a magnetization will be oriented along the –Y´(Y´)-axes and can be measured. When τ is varied, then experimental dependence Mτ = f(τ) can be obtained and fitted by the law of Mτ = M0×[1‒2×exp(‒τ/T1)] for single exponential spin-lattice relaxation. In the case of several components, Mτ = ∑ M0i×[1‒2×exp(‒τ/T1i)] (where summation is doing for all relaxation components whereas i is the number of relaxation component). T1 values are then calculated by performing nonlinear least squares fit to the data [3, 5, 8, 12]. Fig. (2) shows the result of one particular inversion recovery NMR experiment with fitting magnetization curve by two exponential components.

Fig. (2))

The behaviour of longitudinal magnetization (normalized to M0) vs. time registered in the inversion-recovery experiment (180°–τ‒90°) on the Bombyx mori silk with water content of 0.18 g H2O per g dry mass.T=298 K. Frequency is 400 MHz. Solid line is the fit of the experimental data set by the sum of two components (a and b): Mτ = M0a×[1‒2×exp(‒τ/T1a)] + M0b×[1‒2×exp(‒τ/T1b)]. Spin-lattice relaxation time T1a for slow relaxing component was 0.53 s, whereas fast relaxing component T1b = 9 ms. Silk fibers from the Bombyx mori silkworm have two protein-monofilaments (brins) embedded in a glue-like sericin coating [13, 14]. The brins are fibroin filaments made up of bundles of nanofibrils, circa 5 nm in diameter, with a bundle diameter of around 100 nm. The nanofibrils are oriented parallel to the axis of the fiber, and are interacting strongly with each other [14].

Spin-Spin (Transverse) Relaxation

Spin-spin relaxation describes the interaction between neighbouring nuclei with identical precessional frequencies but differing magnetic quantum states. In this situation, the nuclei can exchange quantum states. A nucleus in the lower energy level will be excited, while the excited nucleus relaxes to the lower energy state. There is no net change in the populations of the energy states, but the average lifetime of a nucleus in the excited state will decrease. This can result in line-broadening. More details can be found in literature [1-5].

Transverse (spin-spin) relaxation is characterized by time constant T2. Transverse relaxation is a process whereby nuclear spins come to thermal equilibrium between themselves. At room temperatures, the T2 values for different materials are usually in the range of 10 µs - 10 sec. It is always true for T2 ≤ T1.

In solutions T2 ≈ T1, and in solids T2<<T1.

The values of T2 are much less dependent on field strength, than T1 values. Transverse magnetization corresponds to a state of phase coherence between the nuclear spin states. Transverse relaxation is unlike the longitudinal relaxation. It is sensitive to the interaction which results in dephasing nuclear spins. A description of spin-spin relaxation is presented in eq. (4):

For measurement of T2, it is possible to use Han pulse sequence (90°–τ‒180°). This is a sequence which creates a signal of spin-echo at the momentt = 2τ [3, 5]. When interval 2τ is varied, an experimental dependence M2τ = f(2τ) can be obtained and modelled to calculate the T2 [3]. The modification of Han method is Carr-Purcell (CP) pulse sequence (90°–τcp‒180°–2τcp‒180°–2τcp‒ 180°–...) which contains π pulses train. The Carr-Purcell-Meiboom-Gill (CPMG) sequence is the next modification of CP-method that uses phase shift of π pulses (by 90°) with respect to initial 90° pulse [5, 8, 11, 12]. Fig. (3) shows an example of spin-echo intensities obtained in one particular CPMG experiment on wood sample.

Normally, in these CPMG NMR studies, it is necessary to model the decays of spin-echo intensities by a sum of several relaxation components [15]. Alternatively, a distribution of T2 relaxation times, which could reconstruct spin-echo decay very closed to that from CPMG experiment, should be found. Conversion of the relaxation signal into a continuous distribution of T2 relaxation components is based on inverse Laplace transform (ILT) [8, 15-18], i.e., the inverse Laplace transform is used for extraction of f(T2) [19]. Thus, the data can be fitted applying ILT in one direction. The probability density f(T2) is calculated as follows from the eq. (5) for the spin-echo signal Mt presented according to [8, 16, 19]:

The eq. (5) has the form of a Laplace transform. Fig. (4) presents an example of ILT application on data set obtained in CPMG experiment on