Extremely dim 'Intra-group light’ may be displaced stars gathered in stellar orphanage. Image: Shutterstock/N_Sakarin.
Extremely dim 'Intra-group light’ may be displaced stars gathered in stellar orphanage. Image: Shutterstock/N_Sakarin.

Australian astronomers offer a Python-based technique to analyze intra-group light

Pioneering a new technique, researchers have peered into the extremely faint light that exists between galaxies to describe the history and state of orphan stars.

An international team of astronomers has turned a new technique onto the faint light between galaxies – known as ‘intra-group light’ – to characterize the stars that dwell there.

Lead author of the study, Dr. Cristina Martínez-Lombilla from the School of Physics at UNSW Science, said “We know almost nothing about intra-group light. Light 'between' the galaxies – the 'intra-group light' – however dim, is radiated from stars stripped from their home galaxy. Image: Supplied.

“The brightest parts of the intra-group light are ~50 times fainter than the darkest night sky on Earth. It is extremely hard to detect, even with the largest telescopes on Earth – or in space.”

Using their sensitive technique, which eliminates light from all objects except that from the intra-group light, the researchers not only detected the intra-group light but were able to study and tell the story of the stars that populate it.

“We analyzed the properties of the intra-group stars – those stray stars between the galaxies. We looked at the age and abundance of the elements that composed them and then we compared those features with the stars still belonging to galaxy groups,” Dr. Martínez-Lombilla said.

“We found that the intra-group light is younger and less metal-rich than the surrounding galaxies.”

Rebuilding the story of intra-group light

Not only were the orphan stars in the intra-group light ‘anachronistic’ but they appeared to be of a different origin to their closest neighbors. The researchers found the character of the intra-group stars appeared similar to the nebulous ‘tail’ of a further away galaxy.

The combination of these clues allowed the researchers to rebuild the history – the story – of the intra-group light and how its stars came to be gathered in their own stellar orphanage.

“We think these individual stars were at some points stripped from their home galaxies and now they float freely, following the gravity of the group,” said Dr. Martínez-Lombilla. “The stripping, called tidal stripping, is caused by the passage of massive satellite galaxies – similar to the Milky Way – that pull stars in their wake.”

This is the first time the intra-group light of these galaxies has been observed.

“Unveiling the quantity and origin of the intra-group light provides a fossil record of all the interactions a group of galaxies has undergone and provides a holistic view of the system's interaction history,” Dr Martínez-Lombilla said.

“Also, these events occurred a long time ago. The galaxies [we’re looking at] are so far away, that we're observing them as they were 2.5 billion years ago. That is how long it takes for their light to reach us.”

By observing events from a long time ago, in galaxies so far away, the researchers are contributing vital data points to the slow-burning evolution of cosmic events.

Tailored image treatment procedure

The researchers pioneered a unique technique to achieve this penetrating view.

“We have developed a tailored image treatment procedure that allows us to analyze the faintest structures in the Universe,” said Dr Martínez-Lombilla.

“It follows the standard steps for the study of faint structures in astronomical images – which implies 2D modeling and the removal of all light except that coming from the intra-group light. This includes all the bright stars in the images, the galaxies obscuring the intra-group light, and a subtraction of the continuum emission from the sky.

“What makes our technique different is that it is fully Python-based so it is very modular and easily applicable to different sets of data from different telescopes rather than being just useful for these images.

“The most important outcome is that when studying very faint structures around galaxies, every step in the process counts, and every undesirable light should be accounted for and removed. Otherwise, your measurements will be wrong.

The techniques presented in this study are a pilot, encouraging future analyses of intra-group light, Dr. Martínez-Lombilla said.

“Our main long-term goal is to extend these results to a large sample of groups of galaxies. Then we can look at statistics and find out the typical properties regarding the formation and evolution of the intra-group light and these extremely common systems of groups of galaxies.

“This is key work for preparing the next generation of deep all-sky surveys such as those to be performed with the Euclid space telescope and the LSST with the Vera C. Rubin Observatory.”

 

Japanese scientists develop the most accurate model of how the shape of coronavirus affects its transmission

Since the start of the COVID-19 pandemic, images of the coronavirus, SARS-CoV-2, have been seared in our minds. But the way we picture the virus, typically as a sphere with spikes, is not strictly accurate. Microscope images of infected tissues have revealed that coronavirus particles are actually ellipsoidal, displaying a wide variety of squashed and elongated shapes. The microscope images of coronavirus reveals that they have ellipsoidal shapes. The scientists modeled these different shapes to see how it impacts the speed that the particles rotate. This image appeared in the research paper published in Physics of Fluids.

Now, a global research team, including scientists from Queen’s University, Canada, and the Okinawa Institute of Science and Technology (OIST), Japan, have modeled how the different elliptical shapes affect the way these viral particles rotate within fluids, impacting how easily the virus can be transmitted. The study was published recently in Physics of Fluids.

“When coronavirus particles are inhaled, these particles move around within the passageways in the nose and lungs,” said Professor Eliot Fried, who leads the Mechanics and Materials Unit at OIST. “We are interested in studying to what extent they are mobile in these environments.”

The specific type of movement that the scientists modeled is known as rotational diffusivity, which determines the rate at which the particles rotate as they move through a fluid (in the coronavirus case, droplets of saliva). Particles that are smoother and more hydrodynamic encounter less drag resistance from the fluid and rotate faster. For coronavirus particles, this rotational speed affects how well the virus can attach to and infect cells.

“If the particles rotate too much, they might not spend enough time interacting with the cell to infect it, and if they rotate too little, they might not be able to interact in a necessary way,” explained Prof. Fried.

In the study, the scientists modeled both prolate and oblate ellipsoids of revolution. These shapes differ from spheres (which have three axes of identical length) in just one of their axes, with prolate shapes having one longer axis, whilst oblate shapes have one shorter axis. Taken to the extreme, prolate shapes elongate into rod-like shapes, whilst oblate shapes squash into coin-like shapes. But for coronavirus particles, the differences are more subtle.

The scientists also made the model the most realistic yet, by adding the spike proteins onto the surface of the ellipsoids. Previous research from Queen’s University and OIST showed that the presence of triangular-shaped spike proteins lowers the speed at which the coronavirus particles rotate, potentially increasing their ability to infect cells.

Here, the scientists modeled the spike proteins in a simpler way – with each spike protein represented by a single sphere on the surface of the ellipsoids. 

“We then figured out the arrangement of the spikes on the surface of each ellipsoidal shape by assuming that they all contain the same charge,” explained Dr. Vikash Chaurasia, a postdoctoral researcher in the OIST Mechanics and Materials Unit. “Spikes with identical charges repel each other and prefer to be as far from each other as possible. They, therefore, end up evenly distributed across the particle in a way that minimizes this repulsion.”

In their model, the researchers found that the more a particle differs from a spherical shape, the slower it rotates. This could mean that the particles are better able to align and attach to cells.

The model is still simplistic, the researchers acknowledge, but it brings us one step closer to understanding the transport properties of the coronavirus and could help pin down one of the factors key to its infective success.

TU Delft discovers the one-way superconductor, thought to be impossible

Associate professor Mazhar Ali and his research group at TU Delft, the oldest and largest Dutch public technical university, located in Delft, Netherlands, have discovered one-way superconductivity without magnetic fields, something that was thought to be impossible ever since its discovery in 1911 – up till now. The discovery makes use of 2D quantum materials and paves the way towards superconducting computing. Superconductors can make electronics hundreds of times faster, all with zero energy loss. Ali: “If the 20th century was the century of semi-conductors, the 21st can become the century of the superconductor.” Artist Impression of a superconducting chipDuring the 20th century many scientists, including Nobel Prize winners, have puzzled over the nature of superconductivity, which was discovered by Dutch physicist Kamerlingh Onnes in 1911 (read more about this in the frame below). In superconductors, a current goes through a wire without any resistance, which means inhibiting this current or even blocking it is hardly possible – let alone getting the current to flow only one way and not the other. That Ali’s group managed to make superconducting one-directional – necessary for computing – is remarkable: one can compare it to inventing a special type of ice that gives you zero friction when skating one way, but insurmountable friction the other way.

Superconductor: super-fast, super-green
The advantages of applying superconductors to electronics are twofold. Superconductors can make electronics hundreds of times faster, and implementing superconductors into our daily lives would make IT much greener: if you were to spin a superconducting wire from here to the moon, it would transport the energy without any loss. For instance, the use of superconductors instead of regular semi-conductors might save up to 10% of all western energy reserves according to NWO.

The (Im)possibility of applying superconducting
In the 20th century and beyond, no one could tackle the barrier of making superconducting electrons go in just one direction, which is a fundamental property needed for computing and other modern electronics (consider for example diodes that go one way as well). In normal conduction the electrons fly around as separate particles; in superconductors, they move in pairs of twos, without any loss of electrical energy. In the 70s, scientists at IBM tried out the idea of superconducting computing but had to stop their efforts: in their papers on the subject, IBM mentions that without non-reciprocal superconductivity, a computer running on superconductors is impossible.

Interview with Mazhar Ali

Q: Why, when one-way direction works with normal semi-conduction, has one-way superconductivity never worked before?

Mazhar Ali:
 “Electrical conduction in semiconductors, like Si, can be one-way because of a fixed internal electric dipole, so a net built-in potential they can have.  The textbook example is the famous "pn junction"; where we slap together two semiconductors: one has extra electrons (-) and the other has extra holes (+). The separation of charge makes a net built-in potential that an electron flying through the system will feel. This breaks the symmetry and can result in "one-way" properties because forward vs backward, for example, are no longer the same. There is a difference in going in the same direction as the dipole vs going against it; similar to if you were swimming with the river or swimming up the river.”

“Superconductors never had an analog of this one-directional idea without magnetic field; since they are more related to metals (i.e. conductors, as the name says) than semiconductors, which always conduct in both directions and don't have any built-in potential. Similarly, Josephson Junctions (JJs), which are sandwiches of two superconductors with non-superconducting, classical barrier materials in-between the superconductors, also haven't had any particular symmetry-breaking mechanism that resulted in a difference between "forward" and "backward".

Q: How did you manage to do what first seemed impossible?

Ali:
 “It was really the result of one of my group's fundamental research directions. In what we call "Quantum Material Josephson Junctions" (QMJJs), we replace the classical barrier material in JJs with a quantum material barrier, where the quantum material's intrinsic properties can modulate the coupling between the two superconductors in novel ways. The Josephson Diode was an example of this: we used the quantum material Nb3Br8, which is a 2D material like graphene that has been theorized to host a net electric dipole, as our quantum material barrier of choice and placed it between two superconductors.”

“We were able to peel off just a couple atomic layers of this Nb3Br8 and make a very, very thin sandwich  - just a few atomic layers thick - which was needed for making the Josephson diode, and was not possible with normal 3D materials. Nb3Br8 is part of a group of new quantum materials being developed by our collaborators, Professor Tyrel McQueen and his group at Johns Hopkins University in the USA, and was a key piece in us realizing the Josephson diode for the first time.”   

Q: What does this discovery mean in terms of impact and applications?

Ali:
 “Many technologies are based on old versions of JJ superconductors, for example, MRI technology. Also, quantum computing today is based on Josephson Junctions. Technology that was previously only possible using semi-conductors can now potentially be made with superconductors using this building block. This includes faster computers, as in computers with up to terahertz speed, which is 300 to 400 times faster than the computers we are now using. This will influence all sorts of societal and technological applications. If the 20th century was the century of semi-conductors, the 21st can become the century of the superconductor.”

“The first research direction we have to tackle for commercial application is raising the operating temperature. Here we used a very simple superconductor that limited the operating temperature. Now we want to work with the known so-called "High Tc Superconductors", and see whether we can operate Josephson diodes at temperatures above 77 K since this will allow for liquid nitrogen cooling. The second thing to tackle is the scaling of production. While it’s great that we proved this works in nanodevices, we only made a handful. The next step will be to investigate how to scale production to millions of Josephson diodes on a chip.”

Q: How sure are you of your case?

Ali:  “There are several steps which all scientists need to take to maintain scientific rigor. The first is to make sure their results are repeatable. In this case, we made many devices, from scratch, with different batches of materials, and found the same properties every time, even when measured on different machines in different countries by different people. This told us that the Josephson diode result was coming from our combination of materials and not some spurious result of dirt, geometry, machine or user error or interpretation.”

“We also carried out "smoking gun" experiments that dramatically narrow the possibility for interpretation. In this case, to be sure that we had a superconducting diode effect we actually tried "switching" the diode; as in we applied the same magnitude of current in both forward and reverse directions and showed that we actually measured no resistance (superconductivity) in one direction and real resistance (normal conductivity) in the other direction.”

“We also measured this effect while applying magnetic fields of different magnitudes and showed that the effect was clearly present at 0 applied field and gets killed by an applied field. This is also a smoking gun for our claim of having a superconducting diode effect at a zero-applied field, a very important point for technological applications. This is because magnetic fields at the nanometer scale are very difficult to control and limit, so for practical applications, it is generally desired to operate without requiring local magnetic fields.”

Q: Is it realistic for ordinary computers (or even the supercomputers of KNMI and IBM) to make use of superconducting?

Ali: “Yes it is! Not for people at home, but for server farms or supercomputers, it would be smart to implement this. Centralized computation is really how the world works nowadays. Any and all intensive computation is done at centralized facilities where localization adds huge benefits in terms of power management, heat management, etc. The existing infrastructure could be adapted without too much cost to work with Josephson diode-based electronics. There is a very real chance, if the challenges discussed in the other question are overcome, that this will revolutionize centralized and supercomputing!”