ArticleslgStudy

physics

Gyromagnetic ratio

Gyromagnetic ratio is a physics topic covered in the lgStudy science library. This page brings together a partial reference excerpt, illustrations, worked examples, real-world applications and a short study plan, so you can understand Gyromagnetic ratio rather than just read about it. In short: In physics, the gyromagnetic ratio (also sometimes known as the magnetogyric ratio in other disciplines) of a particle or system is the ratio of its magnetic moment to its angular momentum, and it is often denoted by the symbol γ, gamma. Its SI unit is the reciprocal second per tesla (s−1⋅T−1) or, equivalently, the coulomb per kilogram (C⋅kg−1).

Gyromagnetic ratio — main illustration
Gyromagnetic ratio — illustration

Key takeaways

  • Gyromagnetic ratio belongs to physics; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect Gyromagnetic ratio to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of Gyromagnetic ratio from memory before moving on to harder problems.

Reference excerpt

In physics, the gyromagnetic ratio (also sometimes known as the magnetogyric ratio in other disciplines) of a particle or system is the ratio of its magnetic moment to its angular momentum, and it is often denoted by the symbol γ, gamma. Its SI unit is the reciprocal second per tesla (s−1⋅T−1) or, equivalently, the coulomb per kilogram (C⋅kg−1). The g-factor of a particle is a related dimensionless value of the system, derived as the ratio of its gyromagnetic ratio to that which would be classically expected from a rigid body of which the mass and charge are distributed identically, and for which total mass and charge are the same as that of the system.

For a classical rotating body Consider a nonconductive charged body rotating about an axis of symmetry. According to the laws of classical physics, it has both a magnetic dipole moment due to the movement of charge and an angular momentum due to the movement of mass arising from its rotation. It can be shown that as long as its charge and mass densities and currents are distributed identically and rotationally symmetric, its gyromagnetic ratio is

γ = q 2 m , {\displaystyle \gamma ={\frac {q}{2m}},}

where q is its charge, and m is its mass. The derivation of this relation is as follows. It suffices to demonstrate this for an infinitesimally narrow circular ring within the body, as the general result then follows from an integration. Suppose the ring has radius r, area A = πr2, mass m, charge q, and angular momentum L = mvr. Then the magnitude of the magnetic dipole moment is

μ = I A = q v 2 π r π r 2 = q 2 m m v r = q 2 m L . {\displaystyle \mu =IA={\frac {qv}{2\pi r}}\,\pi r^{2}={\frac {q}{2m}}\,mvr={\frac {q}{2m}}L.}

For an isolated electron An isolated electron has an angular momentum and a magnetic moment resulting from its spin. While an electron's spin is sometimes visualized as a rotation of a rigid body about an axis, the magnetic moment cannot be attributed to mass distributed identically to the charge in such a model since it is close to twice what this would predict. The correcting factor needed relative to classical relation is called the electron's g-factor, which is denoted ge:

γ e − = μ e − ℏ / 2 = − g e − e 2 m e = g e μ B ℏ , {\displaystyle \gamma _{{\text{e}}^{-}}={\frac {\mu _{{\text{e}}^{-}}}{\hbar /2}}=-g_{\text{e}}{\frac {-e}{2m_{\text{e}}}}=g_{\text{e}}{\frac {\mu _{\text{B}}}{\hbar }},}

where μe− is the electron's magnetic moment, ħ/2 is the angular momentum (spin) of the electron, and μB is the Bohr magneton. The gyromagnetic ratio due to electron spin is roughly twice that due to the orbiting of an electron. The electron gyromagnetic ratio is

γ e − {\displaystyle \gamma _{{\text{e}}^{-}}} = −1.76085962784(55)×1011 s−1⋅T−1 The ratio of the electron's Larmor frequency to the magnetic flux density is

γ ¯ e − = γ e − 2 π {\displaystyle {\bar {\gamma }}_{{\text{e}}^{-}}={\frac {\gamma _{{\text{e}}^{-}}}{2\pi }}} = −28024.9513861(87) MHz⋅T−1 The electron gyromagnetic ratio γ (and its g-factor ge) are in excellent agreement with theory; see Precision tests of QED for details. In the framework of relativistic quantum mechanics,

g e = − 2 ( 1 + α 2 π + ⋯ ) , {\displaystyle g_{\text{e}}=-2\left(1+{\frac {\alpha }{2\pi }}+\cdots \right),}

… excerpt ends here. Continue reading the full article.

Worked examples

Example 1 — a first encounter with Gyromagnetic ratio

Start with the simplest possible case. Write down what Gyromagnetic ratio claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In physics, the smallest case is usually a single object, a single equation or a single measurement. Check that every symbol or term in your sentence has a meaning in that case.

Example 2 — changing one variable

Take the situation from Example 1 and change exactly one quantity: double it, halve it, or set it to zero. Predict what should happen to Gyromagnetic ratio before you calculate. Comparing your prediction with the result is the fastest way to find out whether you understand the idea or only the words.

Example 3 — an exam-style question

Typical questions about Gyromagnetic ratio ask you to (a) state it precisely, (b) apply it to given data, and (c) explain a limitation. Practise writing all three answers in under five minutes; the third part is what separates a full-mark answer from an average one.

Applications of Gyromagnetic ratio

In research
Gyromagnetic ratio appears in physics research whenever the underlying quantities have to be modelled precisely. Papers usually cite it as a starting assumption and then explore where it breaks down.
In technology and industry
Engineering practice reuses Gyromagnetic ratio in design rules, simulations and safety margins. Knowing the idea lets you read a specification sheet and understand why the numbers look the way they do.
In the classroom
Gyromagnetic ratio is common in secondary-school and first-year university syllabi. It links to neighbouring topics Atomic physics, Nuclear magnetic resonance, Ratios, so understanding it makes those chapters shorter.
In everyday life
Look for Gyromagnetic ratio outside the textbook — in sport, cooking, traffic, electronics or the sky above you. An example you found yourself is remembered far longer than one you were given.
Ask Teacher Smith questions about this articleOpens your AI tutor with a question about “Gyromagnetic ratio” →

Affiliate

Preply — study more efficiently by working with a personal tutor. 50% off.

How to study Gyromagnetic ratio in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Gyromagnetic ratio means in your own words.
  3. Compare your version with the excerpt and mark what you missed.
  4. Work through the three examples above with pen and paper.
  5. Explain Gyromagnetic ratio out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Gyromagnetic ratio in simple terms?

In physics, the gyromagnetic ratio (also sometimes known as the magnetogyric ratio in other disciplines) of a particle or system is the ratio of its magnetic moment to its angular momentum, and it is often denoted by the symbol γ, gamma. Its SI unit is the reciprocal second per tesla (s−1⋅T−1) or…

Why does Gyromagnetic ratio matter?

Because it connects several physics ideas at once: it gives you a definition you can apply, a quantity you can calculate, and a way to check whether a result is plausible.

How should I study Gyromagnetic ratio?

Read the excerpt, restate it from memory, then work through the examples and applications listed on this page. The five-step study plan above takes about twenty minutes.

What does this page cover?

It gives you a compact reference excerpt plus original lgStudy explanations, examples, applications and study material on Gyromagnetic ratio.

Tags

  • Atomic physics
  • Nuclear magnetic resonance
  • Ratios

Keep exploring