関連する実験動画
Updated: May 4, 2026

16:20
Hyperpolarized Xenon for NMR and MRI Applications
Published on: September 6, 2012
19.3K
3Dプリントされた高性能核スピンポラライザー
Panayiotis Nikolaou1, Aaron M Coffey, Laura L Walkup
1Department of Radiology, Vanderbilt University Institute of Imaging Science (VUIIS) , Nashville, Tennessee 37232, United States.
Journal of the American Chemical Society
|January 10, 2014
まとめ
三次元印刷は,クセノン-129ガスを超極化するための簡素化され,費用対効果の高いスピン交換光学ポンプシステム (SEOP) を可能にします. この高度なセットアップは,記録的な二極化レベルを達成し,多様な科学的応用への道を開きます.
科学分野:
- 原子,分子,光学物理学
- マグネティックレゾナンスイメージング (MRI)
- 材料科学 材料科学とは
背景:
- スピン交換光学ポンプ (SEOP) は,クセノン129.9のような高極化貴気体にとって極めて重要です.
- 従来のSEOPのセットアップには,複数の光学および電子部品の複雑な統合が含まれます.
- 高温3Dプリントは,SEOPプローブの構築を簡素化する新しいアプローチを提供します.
研究 の 目的:
- 効率的なクセノン-129のハイパーポラライゼーションのための3DプリントされたSEOPプローブの開発と実証.
- 変動温度操作とインシットモニタリングのための主要なコンポーネントを統合する.
- 高気体密度で高クセノン-129の極化を実現する.
主な方法:
- 高温3Dプリントを使用して,SEOPプローブとコンポーネントを統合しました.
- 84kHzのインシットNMR回路,狭められたレーザー源,および近赤外線スペクトロスコピーを組み込みました.
- 熱電気温度調節と逆反射光学を使用し,性能を最適化しています.
- ハイパーポラライズされたクセノン-129ガスのイメージングのための自動ガスの転送が実証されました.
主要な成果:
- 0.5Lの光学ポンプセルでほぼ統一 (129) Xeの極化値を達成しました.
- 1000 Torr のクセノン部分圧で ~74 ± 7% (129) Xe の偏振を記録し,高い Xe 密度で記録しました.
- 測定された偏振の蓄積率は (3.63 ± 0.15) × 10(-2) min(-1) で,T1のリラクゼーション時間は 2.19 ± 0.06 hでした.
- ハイパーポラライゼーション強化 (129) Xeガスのイメージングが成功裏に実証されました.
結論:
- 3Dプリントは,SEOPプローブの構築を大幅に簡素化し,コストと生産時間を削減します.
- 開発されたSEOPセットアップは,高密度で高効率のクセノン-129ハイパーポラライゼーションを可能にします.
- この技術は,化学,生物学,材料科学,医学における幅広いアプリケーションをサポートしています.
さらに関連する動画
関連する概念動画
Nuclear Overhauser Enhancement (NOE)
1.3K
Irradiation of a spin-active nucleus causes an increase or decrease in the signal intensity of neighboring nuclei that are not necessarily chemically bonded or involved in J-coupling. This phenomenon, called the nuclear Overhauser enhancement (NOE), results from through-space interactions between the nuclear spins. The NOE effect decreases with increasing internuclear distance and is generally not observed beyond 4 angstroms. In NOE, dipole-dipole interactions between neighboring spin-active...
1.3K
Atomic Nuclei: Nuclear Spin
5.1K
All atomic particles possess an intrinsic angular momentum, or 'spin'. Electrons, protons, and neutrons each have a spin value of ½, although protons and neutrons in nuclei may have higher half-integer spins owing to energetic factors.
Atomic nuclei have a net nuclear spin, , which can have an integer or half-integer value. In atomic nuclei, the spins of protons are paired against each other but not with neutrons, and vice versa. Consequently, an even number of protons does not contribute...
Atomic nuclei have a net nuclear spin, , which can have an integer or half-integer value. In atomic nuclei, the spins of protons are paired against each other but not with neutrons, and vice versa. Consequently, an even number of protons does not contribute...
5.1K
Atomic Nuclei: Nuclear Spin State Overview
1.9K
NMR-active nuclei have energy levels called 'spin states' that are associated with the orientations of their nuclear magnetic moments. In the absence of a magnetic field, the nuclear magnetic moments are randomly oriented, and the spin states are degenerate. When an external magnetic field is applied, the spin states have only 2 + 1 orientations available to them. A proton with = ½ has two available orientations. Similarly, for a quadrupolar nucleus with a nuclear spin value of one, the...
1.9K
Atomic Nuclei: Nuclear Magnetic Moment
3.0K
All atomic nuclei are positively charged. When they have a nonzero spin, they behave like rotating charges. As a consequence of their charge and spin, these nuclei generate a magnetic field (B). This, in turn, gives rise to a magnetic moment (μ), which is randomly oriented in the absence of an external magnetic field. When an external magnetic field (B0) is applied, the magnetic moment vectors can align with the field or against it in 2 + 1 orientations. A hydrogen nucleus, which is just a...
3.0K
Atomic Nuclei: Nuclear Spin State Population Distribution
1.7K
Near absolute zero temperatures, in the presence of a magnetic field, the majority of nuclei prefer the lower energy spin-up state to the higher energy spin-down state. As temperatures increase, the energy from thermal collisions distributes the spins more equally between the two states. The Boltzmann distribution equation gives the ratio of the number of spins predicted in the spin −½ (N−) and spin +½ (N+) states.
1.7K
Atomic Nuclei: Nuclear Relaxation Processes
1.1K
In the absence of an external magnetic field, nuclear spin states are degenerate and randomly oriented. When a magnetic field is applied, the spins begin to precess and orient themselves along (lower energy) or against (higher energy) the direction of the field. At equilibrium, a slight excess population of spins exists in the lower energy state. Because the direction of the magnetic field is fixed as the z-axis, the precessing magnetic moments are randomly oriented around the z-axis.
1.1K

