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Blackest Black Ever: Ultra-thin Material Absorbs Almost 100% Of Light

Date:
July 2, 2009
Source:
Leiden University
Summary:
It appears to be a paradox: ultra-thin material that absorbs all incident light. Nonetheless, it does exist. Researchers have demonstrated that at a thickness of 4.5 nanometer niobiumnitride (NbN) is ultra-absorbent. They have recorded a light absorption of almost 100%, while the best light absorption to date was 50%. This research brings the ideal light detector a step closer.

How much light is reflected and how much is absorbed depends on two factors: the angle at which the light falls onto the material, and the polarisation (the direction of oscillation) of the light.
Credit: Image courtesy of Leiden University

It appears to be a paradox: ultra-thin material that absorbs all the incident light. Nonetheless, it does exist.

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Ideal light detector

Two researchers, Eduard Driessen, MSc, and Dr Michiel de Dood, have demonstrated that at a thickness of 4.5 nanometer niobiumnitride (NbN) is ultra-absorbent. They have recorded a light absorption of almost 100%, while the best light absorption to date was 50%. This research brings the ideal light detector a step closer.

A cell made of this material can already collect light and convert it into an electrical signal. The high number of downloads indicates that this research is very special.

Angles and polarisation

Materials that could potentially absorb a lot of light have the problem that they reflect the incident light; they are generally very good mirrors. But how much light is reflected and how much is absorbed depends on two factors: the angle at which the light falls onto the material, and the polarisation (the direction of oscillation) of the light. Light has two kinds of polarisation: s and p polarisation.

Polaroid sunglasses make good use of this characteristic. The light absorption of a thin slice of NbN is at its maximum if the light falls on it at an angle of 35 and only consists of s-polarised light. The absorption achieved is then 94%. The p-polarised light is reflected in full. At an angle of 46 the absorption for both polarisation directions is 80%, which is still extremely good.

Applications

This discovery gave Driessen and De Dood the idea for building a special detector. They want to use this detector to view individual light particles, photons. To date this has been very difficult because the absorption was not high enough. The most important part of the detector is a lattice of ultra-absorbent NbN filaments. When an s-light particle falls on the lattice, it is absorbed. A p-particle is reflected. This p-particle can then in turn be collected by a second detector so that all the light is detected.

Calculations show that the wavelength (colour) of the light particle has hardly any influence. The detector can therefore also be used for particles with completely different wavelengths, such as detection systems for telecommunications and infra-red equipment.

The research is being carried out in collaboration with the TU Delft and will be part-funded by the Netherlands Organisation for Scientific Research (NWO) and the Foundation for Fundamental Materials Research (FOM).


Story Source:

The above story is based on materials provided by Leiden University. Note: Materials may be edited for content and length.


Journal Reference:

  1. E. F. C. Driessena and M. J. A. de Dood. The perfect absorber. Applied Physics Letters, Online April 29, 2009 DOI: 10.1063/1.3126062

Cite This Page:

Leiden University. "Blackest Black Ever: Ultra-thin Material Absorbs Almost 100% Of Light." ScienceDaily. ScienceDaily, 2 July 2009. <www.sciencedaily.com/releases/2009/06/090630082647.htm>.
Leiden University. (2009, July 2). Blackest Black Ever: Ultra-thin Material Absorbs Almost 100% Of Light. ScienceDaily. Retrieved January 26, 2015 from www.sciencedaily.com/releases/2009/06/090630082647.htm
Leiden University. "Blackest Black Ever: Ultra-thin Material Absorbs Almost 100% Of Light." ScienceDaily. www.sciencedaily.com/releases/2009/06/090630082647.htm (accessed January 26, 2015).

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