. 24/7 Space News .
STELLAR CHEMISTRY
Zooming in on dark matter
by Staff Writers
Durham UK (SPX) Sep 03, 2020

Projected dark matter density map, created using a simulation measuring 2.4 billion light years on each side. . The intermediate square (top right) is just under a million light years across. The smallest square (bottom left) is the deepest zoom: it is only 783 light years across, equivalent to 500 times the size of the solar system. In the intermediate square(top right) the largest dark matter haloes have a mass similar to that of a rich galaxy cluster (a million trillion times the mass of the Sun). In the smallest square (bottom right) the smallest clearly visible haloes have a mass comparable to that of the Earth (0.000003 the mass of the Sun).

Cosmologists have zoomed in on the smallest clumps of dark matter in a virtual universe - which could help us to find the real thing in space.

An international team of researchers, including Durham University, UK, used supercomputers in Europe and China to focus on a typical region of a computer-generated universe.

The zoom they were able to achieve is the equivalent of being able to see a flea on the surface of the Moon.

This allowed them to make detailed pictures and analyses of hundreds of virtual dark matter clumps (or haloes) from the very largest to the tiniest.

Dark matter particles can collide with dark matter anti-particles near the centre of haloes where, according to some theories, they are converted into a burst of energetic gamma-ray radiation.

Their findings, published in the prestigious journal Nature, could mean that these very small haloes could be identified in future observations by the radiation they are thought to give out.

Co-author Professor Carlos Frenk, Ogden Professor of Fundamental Physics at the Institute for Computational Cosmology, at Durham University, UK, said: "By zooming in on these relatively tiny dark matter haloes we can calculate the amount of radiation expected to come from different sized haloes.

"Most of this radiation would be emitted by dark matter haloes too small to contain stars and future gamma-ray observatories might be able to detect these emissions, making these small objects individually or collectively 'visible'.

"This would confirm the hypothesised nature of the dark matter, which may not be entirely dark after all."

Most of the matter in the universe is dark (apart from the gamma radiation they emit in exceptional circumstances) and completely different in nature from the matter that makes up stars, planets and people.

The universe is made of approximately 27 per cent dark matter with the rest largely consisting of the equally mysterious dark energy. Normal matter, such as planets and stars, makes up a relatively small five per cent of the universe.

Galaxies formed and grew when gas cooled and condensed at the centre of enormous clumps of this dark matter - so-called dark matter haloes.

Astronomers can infer the structure of large dark matter haloes from the properties of the galaxies and gas within them.

The biggest haloes contain huge collections of hundreds of bright galaxies, called galaxy clusters, weighing a 1,000 trillion times more than our Sun.

However, scientists have no direct information about smaller dark matter haloes that are too tiny to contain a galaxy. These can only be studied by simulating the evolution of the Universe in a large supercomputer.

The smallest are thought to have the same mass as the Earth according to current popular scientific theories about dark matter that underlie the new research.

The simulations were carried out using the Cosmology Machine supercomputer, part of the DiRAC High-Performance Computing facility in Durham, funded by the Science and Technology Facilities Council (STFC), and computers at the Chinese Academy of Sciences.

By zooming-in on the virtual universe in such microscopic detail, the researchers were able to study the structure of dark matter haloes ranging in mass from that of the Earth to a big galaxy cluster.

Surprisingly, they found that haloes of all sizes have a very similar internal structure and are extremely dense at the centre, becoming increasingly spread out, with smaller clumps orbiting in their outer regions.

The researchers said that without a measure scale it was almost impossible to tell an image of a dark matter halo of a massive galaxy from one of a halo with a mass a fraction of the Sun's.

Co-author Professor Simon White, of the Max Planck Institute of Astrophysics, Germany, said: "We expect that small dark matter haloes would be extremely numerous, containing a substantial fraction of all the dark matter in the universe, but they would remain mostly dark throughout cosmic history because stars and galaxies grow only in haloes more than a million times as massive as the Sun.

"Our research sheds light on these small haloes as we seek to learn more about what dark matter is and the role it plays in the evolution of the universe."

Research paper


Related Links
Durham University
Stellar Chemistry, The Universe And All Within It


Thanks for being there;
We need your help. The SpaceDaily news network continues to grow but revenues have never been harder to maintain.

With the rise of Ad Blockers, and Facebook - our traditional revenue sources via quality network advertising continues to decline. And unlike so many other news sites, we don't have a paywall - with those annoying usernames and passwords.

Our news coverage takes time and effort to publish 365 days a year.

If you find our news sites informative and useful then please consider becoming a regular supporter or for now make a one off contribution.
SpaceDaily Monthly Supporter
$5+ Billed Monthly


paypal only
SpaceDaily Contributor
$5 Billed Once


credit card or paypal


STELLAR CHEMISTRY
Case for axion origin of dark matter gains traction
Princeton NJ (SPX) Jun 26, 2020
In a new study of axion motion, researchers propose a scenario known as "kinetic misalignment" that greatly strengthens the case for axion/dark matter equivalence. The novel concept answers key questions related to the origins of dark matter and provides new avenues for ongoing detection efforts. This work, published in Physical Review Letters, was conducted by researchers at the Institute for Advanced Study, University of Michigan, and UC Berkeley. The existence of dark matter has been confirmed ... read more

Comment using your Disqus, Facebook, Google or Twitter login.



Share this article via these popular social media networks
del.icio.usdel.icio.us DiggDigg RedditReddit GoogleGoogle

STELLAR CHEMISTRY
NASA seeks next class of Flight Directors for human spaceflight missions

Boeing's Starliner makes progress ahead of flight test with astronauts

The Seventh Meeting of the Japan-U.S. Comprehensive Dialogue on Space: Joint Statement

Russian cosmonaut sheds light on how ISS crew deals with suspected air leak

STELLAR CHEMISTRY
DARPA completes key milestone on Hypersonic Air-breathing Weapons program

Starship could attempt near-earth orbit test flight next year, Elon Musk says

SpaceX launches satellite for Argentina into polar orbit

New launch opportunity begins on Sept 1 for small sats mission

STELLAR CHEMISTRY
China releases recommended Chinese names for Mars craters

Follow Perseverance in real time on its way to Mars

Sustained planetwide storms may have filled lakes, rivers on ancient mars

Deep learning will help future Mars rovers go farther, faster, and do more science

STELLAR CHEMISTRY
Mars-bound Tianwen 1 hits milestone

China's Mars probe over 8m km away from Earth

China seeks payload ideas for mission to moon, asteroid

China marching to Mars for humanity's better shared future

STELLAR CHEMISTRY
Gogo announces entry into agreement to sell its Commercial Aviation unit to Intelsat for $400M in Cash

Dragonfly Aerospace emerges from SCS Aerospace Group

Satellite constellations could hinder astronomical research, scientists warn

Africa is investing more in space and satellite industry

STELLAR CHEMISTRY
L3Harris Technologies selected to build space antenna for mobile telecom satellite

Altius Space Machines to develop innovative technologies for satellite servicing

Making Perwave

Purdue, US Army to collaborate on next-generation energetic materials

STELLAR CHEMISTRY
Manchester experts' breakthrough narrows intelligent life search in Milky Way

Bacteria could survive travel between Earth and Mars when forming aggregates

Fifty new planets confirmed in machine learning first

Tracing the cosmic origin of complex organic molecules with their radiofrequency footprint

STELLAR CHEMISTRY
Technology ready to explore subsurface oceans on Ganymede

Large shift on Europa was last event to fracture its surface

The Sun May Have Started Its Life with a Binary Companion

Ganymede covered by giant crater









The content herein, unless otherwise known to be public domain, are Copyright 1995-2024 - Space Media Network. All websites are published in Australia and are solely subject to Australian law and governed by Fair Use principals for news reporting and research purposes. AFP, UPI and IANS news wire stories are copyright Agence France-Presse, United Press International and Indo-Asia News Service. ESA news reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. All articles labeled "by Staff Writers" include reports supplied to Space Media Network by industry news wires, PR agencies, corporate press officers and the like. Such articles are individually curated and edited by Space Media Network staff on the basis of the report's information value to our industry and professional readership. Advertising does not imply endorsement, agreement or approval of any opinions, statements or information provided by Space Media Network on any Web page published or hosted by Space Media Network. General Data Protection Regulation (GDPR) Statement Our advertisers use various cookies and the like to deliver the best ad banner available at one time. All network advertising suppliers have GDPR policies (Legitimate Interest) that conform with EU regulations for data collection. By using our websites you consent to cookie based advertising. If you do not agree with this then you must stop using the websites from May 25, 2018. Privacy Statement. Additional information can be found here at About Us.