Source: {"pile_set_name": "USPTO Backgrounds"}

Recent developments in magnetic resonance tomography (MRT) and [nuclear] magnetic resonance (NMR) spectroscopy using polarized noble gases have many applications in medicine, physics, and in the physical sciences. Noble gas nuclei may be polarized by optical pumping using alkali metal atoms, as described by Happer et al in Phys. Rev. A, 29, 3092 (1984).
The concept of optical pumping encompasses the method developed by Kastler, in which the occupation numbers of specific energy states are significantly increased with respect to the equilibrium state by irradiation of light into matter. By use of optical pumping, the relative occupation numbers of energy levels in atoms, ions, molecules, and solids may be changed, and ordered states may be produced. The occupation density of the optically pumped state differs markedly from the thermal occupation probability of the state according to the Boltzmann distribution. By optical pumping of Zeeman levels it is possible, for example, to achieve a parallel configuration of the magnetic moments of the electrons or atomic nuclei.
In practice, the alkali metal atom rubidium is typically used in the presence of the noble gases helium and nitrogen. In this manner it is known to achieve a nuclear spin polarization of approximately 20% for 129Xe, for example. Such a nuclear spin polarization is approximately 100,000 times larger than the equilibrium polarization in clinical magnetic resonance tomography at 1 T and 300 K. The associated drastic increase in the signal-to-noise ratio is the reason that new application options are in demand in medicine, science, and technology.
The term “polarization” is understood to mean the degree of alignment (ordering) of the spins of atomic nuclei, electrons, or photons. For example, 100% polarization means that all nuclei or electrons are identically oriented. A magnetic moment is associated with the polarization of nuclei or electrons.
Hyperpolarization refers to a polarization level of nuclear or electron spins that is greater than the degree of thermal polarization of the spins in a given magnetic field at room temperature.
Hyperpolarized noble gases are used as contrasting agents or for NMR spectroscopy. For example, hyperpolarized 129Xe is inhaled by or injected into a person. The polarized xenon accumulates in the brain 10 to 15 seconds later. The distribution of the noble gas in the brain is determined by use of magnetic resonance tomography, and the results are used for further analyses.
The selection of the noble gas depends on the particular application. 129Xe has a large chemical shift. When xenon is adsorbed onto a surface, for example, the resonance frequency of the xenon is significantly altered. In addition, xenon is soluble in lipophilic liquids. Xenon is used when such characteristics are desired.
The noble gas helium has very low solubility in liquids. Therefore, the isotope 3He is routinely used when cavities are involved. The human lung represents an example of such a cavity.
Some noble gases have valuable properties other than those stated above. For example, the isotopes 83Kr, 21Ne, and 131Xe have a quadrupole moment that is of interest, for example, for experiments in basic research or surface physics. However, these noble gases are very costly, which makes them unsuitable for applications that use large quantities.
It is known from Driehuys et al (Appl. Phys. Lett. (1996), 69, 1668) to polarize noble gases in a polarizer in the following manner.
Starting with a gas supply, a gas stream composed of a mixture of 129Xe, 4He, and N2 in an Rb container is enriched with Rb vapor and passed through a pump cell. Circularly polarized light, i.e., light in which the angular momentum or the photon spin is aligned in the same direction, is provided by a laser. In the pump cell the Rb atoms as a pumpable species are optically pumped longitudinally with respect to a magnetic field by means of the laser beam (λ˜795 nm, Rb D1 line), thereby polarizing the electron spins of the Rb atoms. The angular momentum of the photons is transferred to free electrons of alkali metal atoms. The spins of the electrons of the alkali metal atoms thus have a large deviation from thermal equilibrium. The alkali metal atoms are consequently polarized. Collision of an alkali metal atom with a noble gas atom causes the polarization of the electron spin to be transferred from the alkali metal atom to the noble gas atom, resulting in a nuclear spin-polarized noble gas. The polarization of the electron spin of the alkali metal atoms produced by the optical pumping of alkali atoms is thus transferred from alkali electrons to the nuclear spin of the noble gases by spin exchange, as first demonstrated by Bouchiat on the Rb/3He system.
From WO 1999/008766 it is known to use, in addition to a first optically pumpable alkali metal, an auxiliary alkali metal as a second polarizable species. The optically pumped alkali metal species transfers the electron spin polarization to the auxiliary alkali metal, thereby more effectively and rapidly transferring the alkali polarization to the noble gas nuclei, for example 3He.
Alkali metal atoms are used because they have a large optical dipole moment that interacts with the light. The alkali metal atom also has one free electron, thus preventing disadvantageous interactions from occurring between two or more electrons per atom.
Cesium, which is superior to rubidium for achieving the above-referenced effects, might be considered as a well-suited alkali metal atom. However, lasers matched to the optical wavelength of Cs and having sufficient power necessary for polarization of xenon by cesium are not prevalent on the market, compared to the corresponding lasers for Rb.
In order to utilize as many photons as possible in the use of broadband high-power semiconductor lasers, pressures of several atmospheres are used in the optical pumping of noble gases. Thus, the optical pumping of alkali metal atoms differs, depending on the type of the noble gas to be polarized.
For polarization of 129Xe, a gas mixture under a pressure of approximately 7 to 10 bar is continuously or semicontinuously passed through a cylindrical glass cell. The gas mixture is composed of 94% 4He, 5% nitrogen, and 1% xenon. The flow rate of the gas mixture is typically 1 cm per second.
Hyperpolarized nuclear and electron spins relax more or less rapidly as a function of their environment. A distinction is made between the longitudinal T1 relaxation time (T1 time for short), referred to as spin lattice relaxation of adjacent spins, and the transverse T2 relaxation time, referred to as spin-spin relaxation.
In the case of polarization of 3He, the pressure required in the polarizer is produced by the 3He itself since the electron spin relaxation rate of Rb—3He collisions is small. This is not is the case for spin exchange pumping of Rb—129Xe, for which reason the pressure is produced by an additional buffer gas such as 4He. Various requirements are imposed on the polarizer as the result of the differing relaxation and spin exchange rates.
Thus, for 3He the nuclear spin polarization build-up times are in the range of hours. However, since the rubidium spin decomposition rate for rubidium-3He collisions is also relatively small, in this case high 3He pressures (>5 bar) may be used.
For 129Xe, on the other hand, the nuclear spin polarization build-up times are between 20 and 40 seconds on account of the larger effective spin exchange cross-sectional area. Due to the very large rubidium electron spin relaxation rate for rubidium-xenon collisions, during the optical spin exchange pumping the xenon partial pressure can only slightly exceed 100 mbar in order to maintain a sufficiently high rubidium polarization. For this reason, in such polarizers 4He is used as a buffer gas for line broadening.
The polarizer may be designed as a flow polarizer for polarizing 129Xe, for example, or may be provided with a sealed sample cell for 3He, for example.
In a flow polarizer, the gas mixture initially flows through a vessel, referred to hereinafter as a “supply vessel,” in which a certain quantity of Rb is present. The supply vessel containing the rubidium together with the connected glass cell is heated to approximately 100 to 170 degrees Celsius. At these temperatures the rubidium is vaporized. The concentration of the vaporized rubidium atoms in the gaseous phase is determined by the temperature in the supply vessel. The gas stream transports the vaporized rubidium atoms from the supply vessel into a cylindrical sample cell, for example. A laser that provides a high-power, circularly polarized light and having a power rating of approximately 50-100 watts continuously irradiates the sample cell in an axial direction, i.e., in the direction of flow, and optically pumps the rubidium atoms in a highly polarized state. The wavelength of the laser must be matched to the optical absorption line of the rubidium atoms (D1 line).
In other words, in order to optimally transfer the polarization of light to an alkali metal atom, the frequency of the light must match the resonance frequency of the optical transition.
The sample cell is located in a static magnetic field Bo of approximately 10 gauss, which is generated by coils, in particular by a Helmholtz coil pair. The direction of the magnetic field extends parallel to the cylindrical axis of the sample cell, i.e., parallel to the beam direction of the laser. The magnetic field is used to guide the polarized atoms. The rubidium atoms that are optically highly polarized by the laser light collide in the glass cell with the xenon atoms, among other species, and transfer their polarization to the xenon atoms.
At the outlet of the sample cell, the rubidium deposits on the wall due to its high melting point compared to the melting points of the other gases. The polarized xenon or the residual gas mixture is conveyed from the sample cell into a freezer unit, which is composed