# Muon spin spectroscopy

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Muon spin spectroscopy

Muon spin spectroscopy is an experimental technique based on the implantation of spin-polarized muons in matter and on the detection of the influence of the atomic, molecular or crystalline surroundings on their spin motion. The motion of the muon spin is due to the magnetic field experienced by the particle and may provide information on its local environment in a very similar way to other magnetic resonance techniques, such as electron spin resonance (ESR or EPR) and, more closely, nuclear magnetic resonance (NMR).

## Acronym

In analogy with the acronyms for these previously established spectroscopies, the muon spin spectroscopy is also known as µSR, which stands for muon spin rotation, or relaxation, or resonance, depending respectively on whether the muon spin motion is predominantly a rotation (more precisely a precession around a still magnetic field), or a relaxation towards an equilibrium direction, or, again, a more complex dynamics dictated by the addition of short radio frequency pulses. The intention of the mnemonic acronym was to draw attention to the analogy with NMR and ESR. More generally speaking, the abbreviation covers any study of the interactions of the muon's magnetic moment with its surrounding when implanted into any kind of matter.

## How it works

### Introduction

µSR is a relatively new nuclear method. Roughly speaking it can be classified in between NMR and diffraction techniques. The NMR technique which is closest parallel to µSR is "pulsed NMR", in which one observes time-dependent transverse nuclear polarization or so-called "free induction decay" of the nuclear polarization. However, a key difference is the fact that in µSR one uses a specifically implanted spin (the muon's) and does not rely on internal nuclear spins.

In addition, and due to the specificity of the muon, the µSR technique does not require any radio-frequency technique to align the probing spin. On the other hand, a clear distinction between the µSR technique and those involving neutrons or x-rays is that scattering is not involved. Neutron diffraction techniques, for example, use the change in energy and/or momentum of a scattered neutron to deduce the sample properties. In contrast, the implanted muons are not diffracted but remain in a sample until they decay. Only a careful analysis of the decay product (i.e. a positron) provides information about the interaction between the implanted muon and its environment in the sample.

As many of the other nuclear methods, µSR relies on discoveries and developments made in the field of particle physics. Following the discovery of the muon by Seth Neddermeyer and Carl D. Anderson in 1936, pioneer experiments on its properties were performed with cosmic rays. Indeed, with one muon hitting each square centimeter of the earth's surface every minute, the muons constitute the foremost constituent of cosmic rays arriving at ground level. However, µSR experiments require muon fluxes of the order of 104 − 107 muons per second and square centimeter. Such fluxes can only be obtained in high-energy particle accelerators which have been developed during the last 50 years.

### Muon Production

The collision of an accelerated proton beam (typical energy 600 MeV) with the nuclei of a production target produces positive pions (π + ) via the possible reactions:

$\begin{array}{lll} p + p & \rightarrow & p + n + \pi^+\\ p + n & \rightarrow & n + n + \pi^+\\ \end{array}$

From the subsequent decay of the pions (mean lifetime $\tau_{\pi^+}$ = 26.03 ns) positive muons (μ + ) are formed via the two body decay:

$\pi^+ \rightarrow \mu^+ + \nu_{\mu} .$

Since the neutrino has an helicity h = -1, both the neutrino and the μ + have their spin antiparallel to their momentum in the pion rest frame. According to the value of the pion momentum at the decay-time, different types of μ + -beams are available for µSR measurements.

#### High-energy beam

The first type of muon beam is formed by the pions escaping the production target at high energies. They are collected over a certain solid angle by quadrupole magnets and directed on to a decay section consisting of a long superconducting solenoid with a field of several Tesla. If the pion momentum is not too high, a large fraction of the pions will have decayed before they reach the end of the solenoid.

In the laboratory frame the polarization of a high-energy muon beam is limited to about 80% and its energy is of the order of ~40-50MeV. Although such a high energy beam requires the use of suitable moderators and samples with sufficient thickness, it guarantees an homogeneous implantation of the muons in the sample volume. Such beams are also used to study specimens inside of recipients, e.g. samples inside pressure cells.

Such muon beams are available at PSI, TRIUMF, J-PARC and RIKEN-RAL.

#### Surface beam

The second type of muon beam is often called the surface or Arizona beam (recalling the pioneer works of Pifer et al.[1] from the University of Arizona). Here muons are used that arise from pions decaying at rest still inside, but near the surface, of the production target. Such muons, which are 100 % polarized, ideally monochromatic and have a very low momentum of 29.8 MeV/c, which corresponds to a kinetic energy of 4.1 MeV, have a range width in matter of the order of 180 mg/cm2. Hence the paramount advantage of this type of beam is the possibility to use relatively thin samples.

Such muon beams are available at PSI (Swiss Muon Source SµS), TRIUMF, J-PARC, ISIS and RIKEN-RAL.

#### Low-energy muon beam

Finally, muon beams of even lower energy (ultra slow muons with energy down to the eV-keV range) can be obtained by further reducing the energy of an Arizona beam using moderators, as a thin layer of a van der Waals gas frozen on a substrate. The tunable energy range of such muon beams corresponds to implantation depths in solids of less than a nanometer up to several hundred nanometers. Therefore the study of magnetic properties as a function of the distance from the surface of the sample is possible.

Up to now, PSI is the only Facility where such low-energy muon beam is available on a regular basis. Technical developments have been also conducted at RIKEN-RAL, but with a strongly reduced low-energy muons rate. J-PARC is projecting the development of a high-intensity low-energy muon beam.

### Different types of muon sources: continuous vs. pulsed

In addition to the above mentioned classification based on energy, muon beams are also divided according to the time structure of the particle accelerator, i.e. continuous or pulsed.

For continuous (or cw= continuous wave) muon sources no dominating time structure is present. By selecting an appropriate muon incoming rate, muons are implanted into the sample one by one. The main advantage is that the time resolution is solely determined by the detector construction and the read-out electronics. There are two main limitations for this type of sources: (i) a non-negligible random background signal; (ii) a rather limited muon incoming rate. Only the background problem can be overcome by using electrostatic deflectors to ensure that no muons enter the sample until the decay of the precedent muon has been observed. PSI and TRIUMF host the two cw muon sources available for µSR experiments.

For pulsed muon sources protons hitting the production target are bunched into pulses which is also reflected on the secondary muon beam. The advantages of a pulsed muon sources are that in principle, one can use the entire incoming muon intensity and there is almost no background due to accidental coincidences between the incoming muons and decay positrons. The absence of background allows the extension of the time window for measurements up to about ten times the muon mean lifetime. The reverse of the medal is that the width of the muon pulse limits the time resolution. ISIS and J-PARC are the two pulsed muon sources available for µSR experiments.

### The Technique

#### Muon Implantation

The muons are implanted into the sample of interest where they lose energy very quickly. Fortunately, this deceleration process occurs in such a way that it does not jeopardize a μSR measurement. On one side it is very fast (much faster than 100 ps), which is much shorter than a typical μSR time window (up to 20 μs), and on the other side, all the processes involved during the deceleration are Coulombic (ionization of atoms, electron scattering, electron capture) in origin and do not interact with the muon spin, so that the muon is thermalized without any significant loss of polarization.

The positive muons usually adopt interstitial sites of the crystallographic lattice. In most metallic samples the muon's positive charge is collectively screened by a cloud of conduction electrons. Thus, in metals, the muon is in a so-called diamagnetic state and behave like a free muon. In insulators or semiconductors a collective screening cannot take place and the muon will usually pick-up one electron and form a so-called muonium (Mu=μ++e-), which has similar size (Bohr radius), reduced-mass and ionization energy to the hydrogen atom.

#### Detecting the Muon Polarization

The decay of the muon into an electron and two neutrinos occurs via the weak interaction process after an average lifetime of τμ = 2.197034(21) μs:

$\mu^+ \rightarrow e^+ + \nu_e + \bar{\nu}_{\mu}~.$

The parity violation in the weak interaction leads to an anisotropic distribution of the positron emission with respect to the spin direction of the μ+ at the decay time. The positron emission probability is given by

$W(\theta)d\theta \propto (1 + A\cos\theta)d\theta~,$

where θ is the angle between the positron trajectory and the μ+-spin, and A is an asymmetry parameter which depends on the polarization of the muon beam and positron energy. This anisotropic emission constitutes in fact the basics for the μSR technique.

The asymmetry of W is given by A = aPμ(0), where

$P_{\mu}(0) = |\mathbf{P}_{\mu}(0)|$

is the beam polarization (of the order of ~1) and a is an intrinsic asymmetry parameter determined by the weak decay mechanism. Theoretically, an average of 1/3 is obtained if all emitted positrons are detected with the same efficiency irrespective of their energy. Practically, values of A ≈ 0.25 are routinely obtained.

The time scale on which the spin motion may be exploited is that of the muon decay, i.e. a few mean lifetimes, each roughly 2.2 µs (2.2 millionths of a second). Both the production of muon beams with nearly perfect alignment of the spin to the beam direction (what was referred to above as spin polarization and caused by the spontaneous symmetry breaking), and the ability to detect the muon spin direction at the instant of the muon decay rely on the violation of parity, which takes place whenever weak forces are at play.

In short this means that certain elementary events happen only when including clockwise (or only when including counter-clockwise) rotations. For instance, the positive muon decays into a positron plus two neutrinos and the positron is preferentially emitted in the direction of the muon spin. Therefore it would most often see the spin as a counter-clockwise rotation while flying away from the decay point.

Spin alignment allows the production of a muon beam with an aligned magnetic moment. Muons are injected into the material under investigation as short-lived probes sending information from the interior back out to the experimental apparatus. These muons are able to send a message from inside the crystal about the local magnetic field in their surroundings. After some time (mean lifetime 2.2 µs) these spies decay and emit positrons. A beam of aligned muons produces asymmetric positron radiation. The asymmetry of positron radiation contains information about the direction of local magnetic field in the moment of muon decay. Taking into consideration the initial direction of muon magnetic moment and the time interval between the moment of injection and moment of muon decay we can calculate the precession frequency (how rapidly the muon's magnetic moment rotates). The frequency of magnetic moment precession depends on the local magnetic field. Larmor precession is appeared with z-direction magnetic field and only decay in 2.2 µs. But when x-direction magnetic field is applied in muon, the rate of decay is enhanced by gaussian with depolarization rate.

Since 1987 this method was used to measure internal magnetic fields inside high-temperature superconductors. High-temperature superconductors are Type II superconductors, in which the local magnetic fields inside the superconductor depend on the superconducting carrier density—one of the significant parameters of any superconductor (see for example the Bardeen–Cooper–Shrieffer theory of superconductors).

## Applications

Muon Spin Rotation and Relaxation are mostly performed with positive muons. They are well suited to the study of magnetic fields at the atomic scale inside matter, such as those produced by various kinds of magnetism and/or superconductivity encountered in compounds occurring in nature or artificially produced by modern material science.

The London penetration depth is one of the most important parameters characterizing a superconductor because its inverse square provides a measure of the density ns of Cooper pairs. The dependence of ns on temperature and magnetic field directly indicates the symmetry of the superconducting gap. Muon spin spectroscopy provides a way to measure the penetration depth, and so has been used to study high-temperature cuprate superconductors since their discovery in 1986.

Other important fields of application of µSR exploit the fact that positive muons capture electrons to form muonium atoms which behave chemically as light isotopes of the hydrogen atom. This allows investigation of the largest known isotope effect in some of the simplest types of chemical reactions, as well as the early stages of formation of radicals in organic chemicals. Muonium is also studied as an analogue of hydrogen in semiconductors, where hydrogen is one of the most ubiquitous impurities.

## Facilities

µSR requires a particle accelerator for the production of a muon beam. This is presently achieved at few large scale facilities in the world: the CMMS continuous source at TRIUMF in Vancouver, Canada; the SµS continuous source at the Paul Scherrer Institut (PSI) in Villigen, Switzerland; the ISIS and RIKEN-RAL pulsed sources at the Rutherford Appleton Laboratory in Chilton, United Kingdom; and the J-PARC facility in Tokai, Japan, where a new pulsed source is being built to replace that at KEK in Tsukuba, Japan. Muon beams are also available at the Laboratory of Nuclear Problems, Joint Institute for Nuclear Research (JINR) in Dubna, Russia. The International Society for µSR Spectroscopy (ISMS) exists to promote the worldwide advancement of µSR. Membership in the society is open free of charge to all individuals in academia, government laboratories and industry who have an interest in the society's goals.

## References

1. ^ A.E. Pifer, T. Bowen and K.R. Kendall, Nuclear Instruments and Methods 135, 39 (1976), http://dx.doi.org/10.1016/0029-554X(76)90823-5

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