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Category: cosmology – Page 176

Searching for dark matter with the world’s most sensitive radio

Since the 1960s there has been plenty of evidence to support the existence of dark matter through astrophysical and cosmological observations, and at this point we’re very confident that it exists. The question remains, though: what is dark matter actually made of?

Throughout the decades there have been many candidates for , such as weakly interacting (WIMPs), neutrinos, and primordial black holes. Candidates like WIMPs were originally theorized because they have properties that address issues in other parts of physics. Another candidate that could answer some thorny physics questions is called the .

Axions were originally theorized as a solution to a question known as the Strong CP Problem, but physicists also realized that axions could be produced in a way that would satisfy requirements for them to be dark matter. These are the particles that the DMRadio experiments search for.

Using an atomic clock to help find evidence of dark matter

A combined team of physicists from the University of Sussex and the National Physical Laboratory, both in the U.K., has been designing experiments to identify ultra-light dark matter particles. In their paper published in the open-access New Journal of Physics, the group describes how they are attempting to use the high precision of atomic clocks to detect ultra-light dark matter particle “kicks” that would lead to time variations and, in so doing, would show evidence of dark matter.

Currently, dark matter is not something that has been shown to exist—instead it is more of a placeholder that has been created to explain observations of deviations from the Standard Model of physics—like certain gravitational effects on galaxies. Since its development as a theory back in the early 1930s, physicists around the world have been developing theories and experiments to prove that it exists.

Sadly, despite a lot of time and effort, no such proof has been found. In this new effort, the team in the U.K. is working on a novel way to add credence to dark matter theories—using atomic clocks to detect ultra-light dark matter particles.

New ring galaxy discovered by Indian astronomers

By analyzing the data from the Dark Energy Camera Legacy Survey (DECaLS), astronomers from the Christ University in Bangalore, India, have serendipitously discovered a new ring galaxy, which received designation DES J024008.08–551047.5 and may belong to the rare class of polar ring galaxies. The finding was reported in a paper published August 29 on the pre-print server arXiv.

The so-called polar ring galaxies (PRGs) are systems composed of an S0-like galaxy and a polar ring, which remain separate for billions of years. In general, these outer polar rings, composed of gas and stars, are aligned roughly in a perpendicular orientation with respect to the major axis of the central host galaxy.

However, although more than 400 PRG candidates have been discovered to date, only dozens of them have been confirmed as real polar ring by follow-up spectroscopic observations.

For The First Time, The Roiling Mass Circling a Monster Black Hole Has Been Measured

An active supermassive black hole is one of the greatest wonders in the cosmos.

A dense, invisible object that can be billions of times the mass of our Sun is surrounded by a vast, churning disk and torus of material, blazing with light as it swirls down onto the black hole center. But how big do these structures grow?

For the first time, an unambiguous detection of near-infrared light reveals the outskirts of the massive accretion disk surrounding a supermassive black hole hundreds of millions times our Sun’s mass, in a galaxy called III Zw 002 some 1.17 billion light-years away.

Supermassive black hole accretion disk seen ‘on the edge’ for 1st time

Astronomers have observed the outer edge of a disk of matter surrounding a feeding supermassive black hole for the first time.

These observations could help scientists better measure the structures that surround these cosmic monsters, understand how black holes feed on those structures and put together how this feeding influences the evolution of galaxies that house such phenomena.

Black hole ‘seeds’ discovered in the early universe for 1st time ever

Astronomers may have discovered the first evidence of heavy black hole “seeds” in the early universe.

These so-called seeds could help explain how some supermassive black holes with masses equivalent to millions, or even billions, times that of the sun could have grown quickly enough to exist less than 1 billion years after the Big Bang.

Potentially, heavy black hole seeds are black holes with masses around 40 million time that of our sun. They are believed to form from the direct collapse of a massive cloud of gas, unlike your typical black hole that’s born when a massive star reaches the end of its life and collapses under its own gravity. Galaxies theorized to host such heavy black hole seeds are referred to as Outsize Black Hole Galaxies (OBGs).

‘Twisty’ new theory of gravity suggests information can escape black holes after all

There’s a proverb in astronomy that goes something like, “black holes have no hair.” This indicates that black holes are extremely straightforward entities under the framework of general relativity. The only necessary characteristics of a black hole are its mass, electric charge, and spin rate. You now know everything there is to know about black holes just from those three numbers. That is to say, they are bare; they lack any further data.

This feature of black holes has been a major source of frustration for astronomers trying to figure out the inner workings of these cosmic behemoths. However, understanding black holes and their inner workings is impossible due to the absence of any kind of “hair” on their surfaces. Unfortunately, black holes continue to be among the universe’s most elusive and baffling features.

The present knowledge of general relativity, however, is essential to the “no-hair” black hole notion. The emphasis of this relativity illustration is on the curved nature of space-time. Any object with enough mass or energy to bend space-time around it will provide that object directions for movement.

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