Principios Básicos de RMN en sólidos destinado a usuarios. Gustavo Monti. Fa.M.A.F. Universidad Nacional de Córdoba Argentina

Similar documents
Principios Básicos de RMN en sólidos destinado a usuarios. Gustavo Monti. Fa.M.A.F. Universidad Nacional de Córdoba Argentina

Center for Sustainable Environmental Technologies, Iowa State University

4 Spin-echo, Spin-echo Double Resonance (SEDOR) and Rotational-echo Double Resonance (REDOR) applied on polymer blends

Solid-state NMR and proteins : basic concepts (a pictorial introduction) Barth van Rossum,

Direct dipolar interaction - utilization

NMR, the vector model and the relaxation

Cross Polarization 53 53

NMR course at the FMP: NMR of organic compounds and small biomolecules - II -

Carbon 13 NMR NUCLEAR MAGNETIC RESONANCE SPECTROSCOPY

T 1, T 2, NOE (reminder)

General NMR basics. Solid State NMR workshop 2011: An introduction to Solid State NMR spectroscopy. # nuclei

An introduction to Solid State NMR and its Interactions

Slow symmetric exchange

TECNICHE DI ALTA E BASSA RISOLUZIONE IN NMR STATO SOLIDO

Spin Relaxation and NOEs BCMB/CHEM 8190

Chemistry 431. Lecture 23

Principles of Nuclear Magnetic Resonance in One and Two Dimensions

Double-Resonance Experiments

The NMR Spectrum - 13 C. NMR Spectroscopy. Spin-Spin Coupling 13 C NMR. A comparison of two 13 C NMR Spectra. H Coupled (undecoupled) H Decoupled

Relaxation, Multi pulse Experiments and 2D NMR

Magnetic Resonance Spectroscopy

Spin Dynamics Basics of Nuclear Magnetic Resonance. Malcolm H. Levitt

NMR-spectroscopy of proteins in solution. Peter Schmieder

8.2 The Nuclear Overhauser Effect

Spin Interactions. Giuseppe Pileio 24/10/2006

Introduction to 1D and 2D NMR Spectroscopy (4) Vector Model and Relaxations

CONTENTS. 2 CLASSICAL DESCRIPTION 2.1 The resonance phenomenon 2.2 The vector picture for pulse EPR experiments 2.3 Relaxation and the Bloch equations

Physical fundamentals of magnetic resonance imaging

It is possible to choose the temperature for each experiment by setting a temperature under the Temp pane (under the Standard panel).

NMR NEWS June To find tutorials, links and more, visit our website

Magnetic Resonance Imaging. Pål Erik Goa Associate Professor in Medical Imaging Dept. of Physics

Chem8028(1314) - Spin Dynamics: Spin Interactions

PRACTICAL ASPECTS OF NMR RELAXATION STUDIES OF BIOMOLECULAR DYNAMICS

Problem Set #6 BioE 326B/Rad 226B

4 DQF-COSY, Relayed-COSY, TOCSY Gerd Gemmecker, 1999

Chem 325 NMR Intro. The Electromagnetic Spectrum. Physical properties, chemical properties, formulas Shedding real light on molecular structure:

NMR IMAGING OF SOLIDS WITH A SURFACE COIL. J.B. Miller and A.N. Garroway

NMR Dynamics and Relaxation

Biophysical Chemistry: NMR Spectroscopy

Classical behavior of magnetic dipole vector. P. J. Grandinetti

Polarised Nucleon Targets for Europe, 2nd meeting, Bochum 2005

High-Resolutio n NMR Techniques i n Organic Chemistry TIMOTHY D W CLARIDGE

NMR STUDY OF EXCHANGE AND HYDRATION SITE IDENTIFICATION IN MCM-41

Introduction to Relaxation Theory James Keeler

The NMR Inverse Imaging Problem

MRI Physics I: Spins, Excitation, Relaxation

Physikalische Chemie IV (Magnetische Resonanz) HS Solution Set 2. Hand out: Hand in:

Spectral Broadening Mechanisms

NMR in Structural Biology

τ 1 > 1/J - if this lifetime is significantly shortened, the coupling (splitting of the signal) will not be observed

PAPER No. 12: ORGANIC SPECTROSCOPY. Module 19: NMR Spectroscopy of N, P and F-atoms

0.5. Dip. Freq. HkHzL D HppmL

C NMR Spectroscopy

Second Order Effects, Overtone NMR, and their Application to Overtone Rotary Recoupling of 14 N- 13 C Spin Pairs under Magic-Angle-Spinning

SSSC Discovery Series NMR2 Multidimensional NMR Spectroscopy

NMR Spectroscopy: A Quantum Phenomena

The Theory of Nuclear Magnetic Resonance Behind Magnetic Resonance Imaging. Catherine Wasko Physics 304 Physics of the Human Body May 3, 2005

Ferdowsi University of Mashhad

ANALYTICAL AND NUMERICAL INVESTIGATIONS *

Overhauser Magnetometers For Measurement of the Earth s Magnetic Field

Topics. The concept of spin Precession of magnetic spin Relaxation Bloch Equation. Bioengineering 280A Principles of Biomedical Imaging

Spectroscopy of Polymers

PROTEIN NMR SPECTROSCOPY

Physical Background Of Nuclear Magnetic Resonance Spectroscopy

Principles of Nuclear Magnetic Resonance Microscopy

NMR-spectroscopy. I: basics. Peter Schmieder

Advanced Quadrupolar NMR. Sharon Ashbrook School of Chemistry, University of St Andrews

More NMR Relaxation. Longitudinal Relaxation. Transverse Relaxation

Relaxation. Ravinder Reddy

e 2m p c I, (22.1) = g N β p I(I +1), (22.2) = erg/gauss. (22.3)

MR Fundamentals. 26 October Mitglied der Helmholtz-Gemeinschaft

6 NMR Interactions: Zeeman and CSA

Nuclear magnetic resonance in condensed matter

Solid state 13 Cand 1 H MAS NMR investigations of C 60 (ferrocene-d 10 ) 2 complex

8 NMR Interactions: Dipolar Coupling

Chapter 7. Nuclear Magnetic Resonance Spectroscopy

Spectral Broadening Mechanisms. Broadening mechanisms. Lineshape functions. Spectral lifetime broadening

Nuclear Magnetic Resonance Imaging

The Basics of Magnetic Resonance Imaging

Lecture #7 In Vivo Water

PRACTICAL ASPECTS OF NMR RELAXATION STUDIES OF BIOMOLECULAR DYNAMICS

Introduction to MRI. Spin & Magnetic Moments. Relaxation (T1, T2) Spin Echoes. 2DFT Imaging. K-space & Spatial Resolution.

1 General Introduction

Classical Description of NMR Parameters: The Bloch Equations

NMR of large protein systems: Solid state and dynamic nuclear polarization. Sascha Lange, Leibniz-Institut für Molekulare Pharmakologie (FMP)

16.1 Introduction to NMR Spectroscopy. Spectroscopy. Spectroscopy. Spectroscopy. Spectroscopy. Spectroscopy 4/11/2013

NMR = Nuclear Magnetic Resonance

Chapter 13 Nuclear Magnetic Resonance Spectroscopy

Uses of Nuclear Magnetic Resonance (NMR) in Metal Hydrides and Deuterides. Mark S. Conradi

NMR journey. Introduction to solution NMR. Alexandre Bonvin. Topics. Why use NMR...? Bijvoet Center for Biomolecular Research

NMR and MRI : an introduction

Nuclear Magnetic Resonance Spectroscopy Chem 4010/5326: Organic Spectroscopic Analysis Andrew Harned

Biophysical Chemistry: NMR Spectroscopy

1 Magnetism, Curie s Law and the Bloch Equations

Classical Description of NMR Parameters: The Bloch Equations

Solid state and advanced NMR

Structure Determination: Nuclear Magnetic Resonance Spectroscopy

Supplementary Figure 1: Spin noise spectra of 55 Mn in bulk sample at BL =10.5 mt, before subtraction of the zero-frequency line. a, Contour plot of

NMR of CeCoIn5. AJ LaPanta 8/15/2016

Chapter 15 Lecture Outline

Transcription:

Principios Básicos de RMN en sólidos destinado a usuarios Gustavo Monti Fa.M.A.F. Universidad Nacional de Córdoba Argentina

CONTENIDOS MODULO 2: Alta resolución en sólidos para espines 1/2 Introducción Rotación al ángulo mágico Desacople con alta potencia Secuencias de desacoples de pulsos múltiples Polarización cruzada

High resolution in solids for ½ spins In solid state NMR, usually we deal with powder samples, ie samples that consist of many crystallites oriented at random. The interactions we have seen all depend on the crystallite orientation, ie they are anisotropic. As a result, the NMR spectrum of a powdered sample consists of broad lines or patterns of powders, since all other molecular orientation gives rise to different spectral frequencies.

Different parts of an experiment and interactions are affected: Choosing a diluted nucleus: for example 13C, 1.1% abundant which effectively removes homonuclear interactions (13C, 13C). Homonuclear decoupling: remove homonuclear interactions in the case of abundant spins, for example (1H, 1H) Rotation the magic angle: (Magic angle spinning, MAS) which averages the anisotropy of chemical shielding to the isotropic value as in solution and also helps reduce heteronuclear dipolar coupling. Proton dipolar decoupling: This removes the interactions (1H, 13C). Cross polarization (CP): Additionally, the signal to noise ratio (s/ n) of a spectrum can be greatly increased by using a pulse technique which transfers magnetization from protons to carbons and other diluted nuclei.

Magic angle rotation (MAS: magic angle spinning) The largest interaction for dilute nuclei (besides heteronuclear coupling with abundant nuclei such as protons) is the chemical shift anisotropy. In solution, the anisotropy is averaged to its isotropic value by rapid random motion of molecules. This same averaging net can be obtained in a polycrystalline sample by rotating it rapidly (up to 60 khz, usually 10-15 khz) about an axis tilted at an angle of 54 o 44 with respect to the external magnetic field direction, this is called "magic angle". The reason for the success of this technique is the term 3cos 2 θ-1, where θ is the angle between a specific fixed molecular axis and the direction of static magnetic field Chemical Shift Interaction

Homonuclear Dipolar Hamiltonian Heteronuclear Dipolar Hamiltonian Quadrupolar Hamiltonian

The sample is rotated in a cylindric rotor; r s direction of the z axis of the chemical shift anisotropy pas. direction of the rotor rotation, β χ θ β+χ. Average over all of microcrystalites of the sample: <1-3cos 2 θ> = (1/2)(1-3cos 2 β)<3cos 2 χ-1>, para β=54 o 44, <1-3cos 2 θ> = 0. Thus, if the frequency of rotation is fast enough compared to the anisotropy of the interaction, the anisotropic interaction is averaged to zero.

If the rotation frequency is not fast enough compared to the frequency range that covers the interaction, 3 or 4 times greater, appear what we called rotational bands. These are narrow lines that appear in addition to the isotropic chemical shift line. Their positions on frequency, respect to the isotropic line, are ± nν R (n = 1, 2,...), so that their positions change with the speed of rotation of the sample, but not the isotropic line. Static 0.7 khz MAS 5.0 khz MAS 8.0 khz MAS

High power decoupling For high resolution in solids is necessary to eliminate nuclear couplings, in particular those of dipole type. Homonuclear decoupling, for example (1H, 1H), requires special techniques of pulse sequences or very fast rotations at the magic angle (> 20 khz). Heteronuclear decoupling is easier to achieve. In most systems containing carbon there are many hydrogen atoms and dipolar interactions (13C, 1H) are very large. To remove these interactions we use double resonance. That is, while detecting the signal of 13C, the protons are irradiated simultaneously in resonance with radio frequency for which they require very high power (100 to 1000 watts, in frequency units of magnetic field strengths of irradiation γb 1 / 2π to 100 khz may be required).

High power decoupling. This eliminates the effects of 1H dipolar coupling in the spectrum of the nucleus to observe, X in this case. Of course, this technique can beapplied to any heavy nucleus rather than protons. Irradiation with high power is applied to the spins of the protons while the signal is acquired simultaneously for X spins Here we use a single pulse to create transverse magnetization of spin X. More complicated pulse sequences can also be used to prepare the spin system X.

Multiple pulse decoupling sequences The magic angle rotation can remove homonuclear dipolar coupling effects if the rotation speed is greater than the dipolar interaction. For protons this is not always possible since these usually have homonucleardipolar interactions of tens of kilohertz. In these cases then are used pulse sequences to achieve homonuclear dipolar decoupling. Most of these sequences are arranged so that, in certain windows within the pulse sequence, the effect of the dipolar Hamiltonian on the magnetization is zero. If the magnetization is detected in these windows the homonuclear dipolar coupling effect in the NMR spectrum is removed Unlike MAS, which averages to zero the geometric terms of the interaction, these sequences averaged to zero the spin terms of the interaction.

WAHUHA sequence. All pulses are 90 to the phases are shown in the figure. The points of signal detection are indicated by an arrow. The four pulses are repeated periodically until the signal has decayed completely in the xy plane.

The effect of WAHUHA sequence (and any other) on the spin system can be treated by the average Hamiltonian theory. Briefly we give some indication of how it works in this description. One can show that at the end of one cycle of the sequence the spin system has evolved under the action of "average Hamiltonian" Hˆ = ( Hˆ + Hˆ + 2 Hˆ + Hˆ + Hˆ ) / 6 z y x y z As during the free evolution of spin system is under the action of the interactions of chemical shift and homonuclear dipolar coupling the average Hamiltonian is ˆ 1 ˆ j ˆ j ˆ j 1 ( ) ( ˆ I I ˆ I I ˆ I I H = ω j I z I y I x H z H y H x ) 3 + + + + + 3 j One can show that dipolar term ˆ I I ˆ I I ˆ I I ( H z + H y + H x ) = 0 vanishes, so that the sequence eliminates the effect of this interaction.

Tyrosine Homonuclear dipolar coupling DUMBO 67 khz 35 khz 24 khz 15 khz and 7 khz DUMBO is a homonuclear decoupling multipulse sequence, here combined with MAS (CRAMPS) at high speed

Cross Polarization There is an additional problem not connected to the line broadening. To explain itis necessary to understand the phenomenon of relaxation. For relaxation we understand the processes that the magnetization back to equilibrium when it hasbeen disturbed by an rf pulse. We consider three types of processes. First type: spin-lattice relaxation or longitudinal relaxation, is the recovery of the magnetization component along the external field. The characteristic time of this process is called T 1 and governs the speed at which the rf pulses can be repeated in a simple experiment of a single pulse and acquisition. [M 0 - M z (t)] = [M 0 - M z (0)] exp(-t/t 1 ) Second type: transverse relaxation or spin-spin. Is the decay of the transverse component of magnetization related to the dephasing of spins in the xy plane."the characteristic time is called T 2 and related to the line width of the NMR signal. M xy (t) = M xy (0) exp(-t/t 2 ) Third type: spin-lattice relaxation in the rotating system, governs the equilibrium of the magnetization perpendicular to z axis in the presence of rf. The time that characterizes this process is called T 1ρ. M(t) = M 0 exp(-t/t 1ρ )

13 C 13C T 1ρ measurement M 0is along the rf magnetic field B, 1 we say taht it is spin-locked. Since B 0 >> B 1 the magnitude of 0 is far away bigger than expected at room temperature. In this way will be relaxation while the spins get hoter. SL: spin-lock. DD: dipolar decoupling. M

For solids the following relation between these three relaxation times holds T 2 << T 1ρ << T 1 T 2 being the order of tens of microseconds, T 1ρ the order of tens of milliseconds, T 1 from several seconds to hours. The spin relaxation times for diluted nuclei as 13C in solids are often substantially longer than for 1H (they can be around one hour). Due to get a reasonable s/n ratio, the experiment must be repeated thousands of times, and the repetition rate must be greater than 5T 1, the experiment of a single pulse with proton decoupling is totally inefficient. This situation can be remedied with a pulse sequence called cross-polarization

energy level matching: Hartmann-Hahn matching laboratory rotating laboratory frame, I spin frame frame, S spin ω0,i ω = 1,I ω1,s ω 0, S ω ω 0,I 1,I = γ B I I = γ B 0 1,I Hartmann-Hahn match: γ B = γ B I 1,I S 1, S

90 x 1 H contact decoupling 13 C contact aquire Diagram of the cross-polarization 1 H 13 C pulse sequence.

The sequence consists of a spin-locking of the protons and the beginning of a period of double resonance known as contact time, where the B rf fields are set according to the Hartmann- 1 Hahn condition: γ C B 1C = γ H B 1H During the contact time the proton transverse magnetization along is transferred to the carbon nuclei (along B B 1 H ) mainly via flip-flop transitions via the dipole interaction term. The contact times are of 1 C the order of milliseconds, the 13C magnetization value increases over the Boltzman value by a factor γ H / γ C ~ 4. Additionally, the repetition rate depends on T 1H rather than T 1C (T 1H <<T 1C ) so you can use shorter repetition rates than in an experiment of a single pulse.

90 contact proton magnetization decays with T 1ρ 90 1 H ~ T 1ρ cross polarization builds up with T IS ~ T IS 13 C signal follows combined effect of buildup and decay

CP is not quantitaive short T IS (~500 ms): directly attached protons (-CH 3, -CH 2 -, >CH-) long T IS (>1-2 ms): quaternary carbons (>C<, -COO-, substituted aromatic systems,...), high mobility short T 1ρ : paramagnetic systems/impurities (e.g. in coal), high mobility

An old example about we can say up to here is a carboxilate[r. K. Harris, Nuclear Magnetic Resonance Spectroscopy: A Physicochemical View, ISBN 0-582-44653-8, Ch. 6, Longman Scientific and Technical, Harlow (1994)]. Clearly the asymmetric unit cell has four acetates groups. Calcium acetate 13 C spectrum. 2Ca(CH 3 CO 2 ) 2.2H 2 O. a) static without proton decoupling, b) static wiht high power proton decoupling, c) with decoupling and MAS d) detail of c)