Basic NMR physics – When a sample is placed in a strong external magnetic field (B0), how do nuclear spins behave at thermal equilibrium before excitation?

Difficulty: Easy

Correct Answer: They partially align with the magnetic field (with a slight excess in the lower-energy state)

Explanation:


Introduction / Context:
NMR relies on the interaction between nuclear magnetic moments and an applied static magnetic field (B0). At equilibrium, populations of nuclear spin states are distributed according to Boltzmann statistics. A small excess occupies the lower-energy state aligned with B0, generating a net magnetization vector along the field. This macroscopic magnetization is what the spectrometer manipulates and detects after radio-frequency excitation.


Given Data / Assumptions:

  • We consider spin-1/2 nuclei (e.g., 1H, 13C) at room temperature in a high-field magnet.
  • Thermal equilibrium is established prior to any RF pulse.
  • Net longitudinal magnetization (Mz) arises from a slight population difference.


Concept / Approach:
In B0, spin states split into two energy levels (Zeeman splitting). The lower-energy state corresponds to magnetic moments aligned with B0; the higher-energy state is anti-aligned. Because the energy gap is small compared to kT, the excess population is slight, but sufficient to create measurable net magnetization. No macroscopic “stopping” or instantaneous 90° rotation occurs until an RF pulse perturbs the equilibrium.


Step-by-Step Solution:

Apply B0 → spin energy levels split.Boltzmann distribution yields a small excess in the lower-energy, aligned state.Net magnetization Mz forms along B0.Subsequent RF pulses tip Mz into the transverse plane to generate FID signals.


Verification / Alternative check:
Increasing field strength increases the population difference and thus sensitivity. Cryogenic temperatures further enhance polarization, consistent with the equilibrium alignment model.


Why Other Options Are Wrong:

  • Spins do not stop; they precess at the Larmor frequency.
  • They do not all reverse direction spontaneously; populations reflect Boltzmann statistics.
  • Exact 90° orientation is an excitation outcome, not an equilibrium state.
  • Liquid-helium cooling is not required for alignment; room temperature polarization is sufficient for NMR.


Common Pitfalls:
Confusing equilibrium magnetization with post-pulse transverse magnetization; only the latter produces the detectable FID immediately after excitation.


Final Answer:
They partially align with the magnetic field (with a slight excess in the lower-energy state)

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