Nanostructured filaments produce luminous waves that twist as they move

Scientists at the University of Michigan say the twisted shape of the nanostructured filaments allows them to generate bright, twisted light.



Planck's law ignores, but does not prohibit, circular polarization of blackbody radiation (BBR). BBRs consisting of nanostructured filaments with twisted shapes made of nanocarbon or metal have strong ellipticity between 500 and 3000 nanometers. The submicrometer-scale chirality of these filaments meets the dimensional requirements imposed by the fluctuation dissipation theorem, which requires symmetry breaking between absorption and emissivity according to Kirchhoff's law. The resulting BBRs exhibit emission anisotropy and brightness that are 10–100 times superior to conventional chiral photon emitters. Image credit: Lu others., doi: 10.1126/science.adq4068.

“When producing twisted light using traditional methods such as electroluminescence or photon emission, it is difficult to generate sufficient brightness,” said Dr. Jun Lu, a researcher at the University of Michigan.

“We gradually realized that there is actually a very old way of producing these photons, which does not rely on the excitation of photons and electrons, but is similar to the light bulb that Edison developed. .”

“Every object that has some heat, including yourself, constantly emits photons in the spectrum associated with its temperature.”

“If an object is the same temperature as its surroundings, it will also absorb the same amount of photons. Since black absorbs all photon frequencies, this is idealized as blackbody radiation.”

Although the filament of a tungsten bulb is much warmer than its surroundings, the law that defines blackbody radiation (Planck's law) provides a good approximation of the spectrum of photons that a tungsten bulb transmits.

The photons we see as a whole look like white light, but when we pass light through a prism, we see a rainbow of different photons inside.

This radiation is also why it appears bright in thermal images, but even room-temperature objects can appear dark because they are constantly emitting and receiving blackbody photons.

Usually, the shape of the object that emits radiation is not much considered. In most cases, objects can be imagined as spheres.

However, while the shape does not affect the spectrum of different photon wavelengths, it can affect another property: polarization.

Photons from a blackbody source are typically randomly polarized, and their waves can oscillate along any axis.

New research reveals that blackbody radiation can also be twisted if the emitter is twisted on the micro or nanoscale, with the length of each twist similar to the wavelength of the emitted light.

The strength of the twist of light, or its elliptical polarization, is determined by two main factors. One is how close the wavelength of the photon is to the length of each twist, and the other is the electronic properties of the material (in this case, nanocarbon or metal).

Twisted light is also called “chiral” because the clockwise and counterclockwise rotations are mirror images of each other.

The study was done to demonstrate the premise of a more applied project that the Michigan team wants to pursue: using chiral blackbody radiation to identify objects.

They envision robots and self-driving cars that can see like a mantis shrimp, distinguishing light waves in different directions of rotation and degrees of twist.

“Advancing the physics of blackbody radiation through chiral nanostructures is at the heart of this research. Such emitters are all around us,” said Professor Nicholas Kotov of the University of Michigan.

“For example, these findings could be important in helping autonomous vehicles tell the difference between a deer and a human. Deer fur curls differently than our fabric, so even though the wavelengths are similar, Helicity emits a different light.”

The main advantage of this method of producing twisted light is its brightness, which is up to 100 times brighter than other approaches, but the light contains a wide spectrum of both wavelengths and twists.

The authors have ideas on how to address this, including exploring the possibility of building lasers that rely on twisted light-emitting structures.

They want to further explore the infrared spectrum. The peak wavelength of blackbody radiation at room temperature is approximately 10,000 nanometers or 0.01 millimeter.

“This is a noisy spectral region, but elliptical polarization could potentially enhance the contrast,” Professor Kotov says.

of the team work Published in a magazine science.

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Jun Lu others. 2024. Bright circularly polarized blackbody radiation from twisted nanocarbon filaments. science 386 (6728): 1400-1404;doi: 10.1126/science.adq406

Source: www.sci.news

Astronomers Uncover Magnetic Filaments Surrounding the Central Black Hole in Messier 77’s Accretion Disk

Messier 77 is a relatively nearby and well-known bright spiral galaxy with a supermassive black hole at its center.

Messier 77 concept by artist. It is characterized by its powerful black hole and accretion disk, as well as the polarized light of water masers located outside the Milky Way. Image credit: NSF / AUI / NRAO / S. Dagnello.

Messier 77 is a barred spiral galaxy located 62 million light-years away in the constellation Cetus.

Also known as NGC 1068, LEDA 10266, and Cetus A, it has an apparent magnitude of 9.6.

Messier 77 was discovered in 1780 by French astronomer Pierre Méchain, who initially identified it as a nebula. Méchain then relayed this discovery to his colleague, the French astronomer Charles Messier.

Messier believed that the extremely bright objects he saw were clusters of stars, but as technology advanced, their true status as a galaxy was recognized.

At 100,000 light-years in diameter, Messier 77 is one of the largest galaxies in the Messier catalog, and its gravity is enough to twist and distort other galaxies nearby.

It is also one of the closest galaxies to active galactic nuclei (AGNs).

These active galaxies are among the brightest objects in the universe, emitting light in many if not all wavelengths, from gamma rays and X-rays to microwaves and radio waves.

But Messier 77's accretion disk is hidden by a thick cloud of dust and gas, despite being a popular target for astronomers.

Several light-years in diameter, the outer accretion disk is dotted with hundreds of different water maser sources that have been hinting at deeper structures for decades.

Masers are clear beacons of electromagnetic radiation that shine at microwave or radio wavelengths. In radio astronomy, water masers, observed at a frequency of 22 GHz, are particularly useful because they can shine through many of the dusts and gases that block the wavelengths of light.

Bucknell University astronomer Jack Gallimore and his colleagues began observing Messier 77 with two goals in mind: astronomical mapping of the galaxy's radio continuum and measuring the polarization of water masers.

“Messier 77 is a bit of a VIP among active galaxies,” says Dr. CM Violette Impellizzeri, an astronomer at the Leiden Observatory.

“There's an accretion disk right next to the black hole, and it's unusually powerful. And because it's so close, it's been studied in great detail.”

But the study authors looked at Messier 77 in an entirely new way.

Their observations were recently upgraded High sensitivity array (HSA) consists of the Karl G. Jansky Very Large Array, the Very Long Baseline Array, and NSF's NRAO telescope at the Green Bank Telescope.

By measuring the water maser's polarization and the continuous radio emission from Messier 77, they reveal the compact radio source, now known as NGC 1068*, and the mysterious extended structure of the fainter emission. I created a map to

Mapping the astronomical distribution of galaxies and their water masers reveals that they are spread along structural filaments.

“These new observations reveal that the maser spot filaments are actually arranged like beads on a string,” Dr. Gallimore said.

“We were stunned to see that there was an apparent offset, or displacement angle, between the radio continuum, which describes the structure of the galaxy's core, and the position of the maser itself.”

“The configuration is unstable, so we're probably looking at a magnetically ejected source.”

Measuring the polarization of these water masers with HSA revealed significant evidence of a magnetic field.

“No one has ever seen polarization in water masers outside of our galaxy,” Dr. Gallimore said.

“Similar to the loop structures seen as prominences on the Sun's surface, the polarization patterns of these water masers clearly indicate that there is also a magnetic field at the root of these light-year-scale structures.”

“Looking at the filaments and making sure the polarization vector is perpendicular to the filaments is key to confirming that they are magnetically driven structures. It's exactly what you expected. It’s a thing.”

Previous studies of the region have suggested patterns, usually related to magnetic fields, but such conclusions were until recently beyond the scope of observational techniques.

The discovery reveals evidence for a compact central radio source (the galaxy's supermassive black hole), distinct polarization of water masers indicating structure within Messier 77's magnetic field, and spectacular extended signatures across the radio frequency continuum. It became.

Taken together, these findings indicate that magnetic fields are the underlying driving force for these phenomena.

However, many mysteries remain. For example, within the radio continuum map there is a diffuse, faint protrusion that the team has dubbed the foxtail foxtail, extending northward from the central region.

“When we set out on this, we said to ourselves, 'Let's really push the limits and see if we can get good continuum and polarization data,' and those goals were both It was a success,” Dr. Gallimore said.

“Using the NSF NRAO High Sensitivity Array, we detected the polarization of a water megamaser for the first time. We also created a very surprising continuum map, which we are still trying to understand.”

a paper The results will be explained today. Astrophysics Journal Letter.

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Jack F. Gallimore others. 2024. Discovery of polarized water vapor megamaser emission in molecular accretion disks. APJL 975, L9; doi: 10.3847/2041-8213/ad864f

Source: www.sci.news