Zeeman effect

Everyday term

In plain words

The splitting of an energy level by a magnetic field. An electron’s makes it a tiny magnet; in a field, the state whose magnet lines up with the field drops in energy and the opposite one rises, so one level becomes two, further apart the stronger the field. How strongly a state responds is its g-factor – about 2 for a bare electron spin. In the the two respond in opposite directions, so a field shifts the light emitted from each the opposite way, and a magnetic layer underneath can do the same without any field.

Going deeper

Three panels. A field splits a level: energy against magnetic field, one level fanning into two straight lines, one rising and one falling, separated by g μB B. Valleys pull apart: the emission peak of monolayer WSe₂ without a field, dashed, and in a field split into a σ+ peak from the K valley and a σ− peak from the K′ valley. A magnet does it too: a WSe₂ layer on magnetised CrI₃ showing the same split peaks with no field applied. a field splits a level ↑ ↓ gμB B energy ↑ field → a spin level in a field the split grows with the field; its slope is the g-factor g ≈ 2 for a bare spin valleys pull apart σ+, K σ−, K′ energy → dashed: no field light from each valley shifts the opposite way ≈0.25 meV per tesla in WSe₂ a magnet does it too WSe₂ CrI₃, magnetised the magnet splits the valleys as a 13 T field would and flips with the magnet
A magnetic field lowers the energy of a state whose magnetic moment lines up with it and raises the opposite one, by an amount set by the g-factor. In monolayer WSe2 the two valleys shift in opposite directions, so light of each handedness moves apart; a neighbouring magnet such as CrI3 splits them as a 13-tesla field would.

One level becomes two

A magnetic field acts on anything that carries a . An electron’s spin is such a moment, so in a field the two spin states, which otherwise have the same energy, separate: one lowers its energy by lining up with the field, the other rises. The gap grows in proportion to the field, as g μB B, where μB, the Bohr magneton, is about 58 microelectronvolts per tesla and g, the g-factor, is close to 2 for a free electron’s spin. Electrons moving round atoms add an orbital moment, which is why the spectral lines of atoms split in a field into characteristic patterns.

In a crystal the bands reshape these moments, and carriers, and defects acquire g-factors of their own – small, large or even negative. Measuring how a line splits in a field therefore says what kind of state produced it.

Valleys in a field

In the transition metal dichalcogenides the valleys at K and K′ carry opposite magnetic moments, from the d orbitals of the metal atoms and from the shape of the bands, so a field perpendicular to the layer shifts them in opposite directions – the valley Zeeman effect. Each valley absorbs and emits light of one circular polarisation, so the effect shows up directly in : in WSe2 the two circularly polarised exciton peaks move apart by about 0.25 meV per tesla, close to what the d-orbital moments predict, while the splits more than a quarter more (Srivastava and colleagues, 2015). A field also tunes how much of the light’s the emission keeps, a magnetic handle on the valley (Aivazian and colleagues, 2015).

The splitting is small – a few millielectronvolts even at 10 T – which is why such experiments run cold, where the peaks are narrow. have g-factors of their own, large enough to tell how the two layers are stacked.

Zeeman without a field

A neighbouring magnet can split levels as a field would, through the across the interface. A monolayer of WSe2 on a thin of the CrI3 shows a valley splitting equivalent to an exchange field of nearly 13 T, and both the splitting and the polarisation of its light switch when the magnetisation of the CrI3 flips (Zhong and colleagues, 2017) – which also makes the WSe2 a sensitive optical probe of the magnet’s domains.

can act the same way. In monolayers such as MoS2 and NbSe2, pins electron spins out of the plane with opposite signs in the two valleys – an effective Zeeman field of tens of tesla built into the bands, and the origin of , which survives in-plane fields far beyond the usual limit.

For specialists

The linear splitting ΔE = g μB B of states with a magnetic moment in a field B, with μB = 57.9 μeV T−1; for a free electron spin g ≈ 2, while orbital moments and give carriers and excitons effective g-factors that differ widely and can be negative. In monolayer WSe2 the K and K′ exciton lines split by about 0.25 meV T−1, about 4.3 μB B, close to the 4 μB expected from the d-orbital moments of the , while the trion splits more than a quarter more, an effect of exchange. Proximity to the ferromagnet CrI3 splits the WSe2 valleys as an exchange field of nearly 13 T would, switching with the magnetisation, and spin–valley locking acts as a built-in Zeeman field of tens of tesla in Ising superconductors.

Where this comes from

  1. Valley Zeeman effect in elementary optical excitations of monolayer WSe2 Srivastava et al. · Nature Physics 11, 141 (2015)
  2. Magnetic control of valley pseudospin in monolayer WSe2 Aivazian et al. · Nature Physics 11, 148 (2015)
  3. Van der Waals engineering of ferromagnetic semiconductor heterostructures for spin and valleytronics Zhong et al. · Science Advances 3, e1603113 (2017) cited by 28

In the news

The newest items in the site’s news feed that use the term, one from each source.

Journal Advanced Functional Materials

Steering no Dimerization Through Boron‐Enhanced Spin–Orbit Coupling in Ultrathin PdCuB Nanosheets for Durable N2‐Selective Nitrate Reduction

The selectivity bottleneck of electrochemical nitrate‐to‐N2 conversion is kinetic rather than thermodynamic: dimerization of two adsorbed *NO intermediates is spin‐forbidden, imposing a kinetic barrier invisible to conventional thermodynamic analyses. Spin–orbit coupling (SOC) offers the principal channel for the…

Theory

Search the news for this term