Hungarian Inventions Codexery

Neutron supermirror

Layered reflector enhancing neutron beam critical angle via diffraction.

Neutron supermirror

A neutron supermirror is a precisely fabricated, layered surface designed to reflect neutron beams. It represents a specific type of multilayer neutron reflector where the thickness of each layer varies. The idea was first put forward by Ferenc Mezei, who drew on earlier techniques developed for X-rays.

These mirrors are made by coating a smooth base with alternating layers of materials that have strongly different properties, such as nickel and titanium. A single layer of a high-refractive-index material like nickel can reflect neutrons entirely at very shallow angles, up to a certain critical angle. For natural nickel, this critical angle in degrees is roughly 0.1 times the neutron’s wavelength in angstroms.

To achieve a larger effective critical angle, the mirror uses diffraction from its stacked layers, though this introduces some losses. The resulting critical angle in degrees becomes about 0.1 times the wavelength times a factor called the "m-value," which is measured relative to natural nickel. Common m-values range from 1 to 3, but for applications needing high beam divergence—such as focusing optics near a neutron source, choppers, or experimental areas—an m-value of 6 is readily available.

Nickel has a positive scattering cross section, while titanium has a negative one, and both have low absorption. This makes the nickel-titanium combination the most efficient for neutron work. However, the number of required layers grows rapidly with the m-value—roughly proportional to m raised to a power between 2 and 4—which significantly drives up cost. This factor heavily influences the economic decisions behind designing neutron instruments.

Field
Neutron optics
Known for
Reflecting neutron beams with enhanced critical angle via multilayers
Key material
Nickel-titanium (Ni–Ti) alternating layers
M value range
1–3 common; m=6 readily available for high divergence
Critical angle formula
0.1·λ·m degrees (λ in angstroms)

Lore & Background

Neutron supermirrors are produced by depositing alternating layers of strongly contrasting substances, such as nickel and titanium, on a smooth substrate. A single layer of high-refractive-index material like nickel exhibits total external reflection at small grazing angles up to a critical angle θ_c. For nickel with natural isotopic abundances, θ_c in degrees is approximately 0.1·λ, where λ is the neutron wavelength in angstroms.

A mirror with a larger effective critical angle can be made by exploiting diffraction (with non-zero losses) that occurs from stacked multilayers. The critical angle of total reflection becomes approximately 0.1·λ·m, where m is the 'm-value' relative to natural nickel. Values of m in the range of 1–3 are common; in specific areas for high divergence, m=6 is readily available.

Nickel has a positive scattering cross section, and titanium has a negative scattering cross section, and in both elements the absorption cross section is small, which makes Ni–Ti the most efficient technology with neutrons. The number of Ni–Ti layers needed increases rapidly as ∝ m^z, with z in the range 2–4, which affects cost.

Reader's Guide

Neutron supermirrors are significant because they allow neutron beams to be reflected at larger angles than possible with a single material, enabling more compact and efficient neutron instruments. By using multilayers with varying thicknesses, the effective critical angle is increased by a factor m, with m typically between 1 and 3, and up to 6 in specialized applications. The Ni–Ti combination is the most efficient due to the contrasting scattering cross sections and low absorption. However, the number of layers grows rapidly with m (∝ m^z, z=2–4), driving up cost and influencing the economic strategy of neutron instrument design. This technology is crucial for neutron guides, focusing optics, and other beam-handling components in research facilities.

Did You Know?

More in Hungarian inventions 1-24

Spotted an error? Know more?

Reader corrections go straight into our review queue. Suggest an edit · How this site is sourced

Comments

Loading…
Open in the interactive codex →