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Bright, powerful burst of gamma rays detected

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Multiple space and ground-based telescopes witnessed one of the brightest explosions in space when it reached Earth on October 9. The burst may be one of the most powerful ever recorded by telescopes.

Gamma-ray bursts, or GRBs, are the most powerful class of explosions in the universe, according to NASA. Scientists have dubbed this one GRB 221009A, and telescopes around the world continue to observe its aftermath.

“The exceptionally long GRB 221009A is the brightest GRB ever recorded and its afterglow is smashing all records at all wavelengths,” said Brendan O’Connor, a doctoral student at the University of Maryland and George Washington University in Washington, DC, in a statement.

“Because this burst is so bright and also nearby, we think this is a once-in-a-century opportunity to address some of the most fundamental questions regarding these explosions, from the formation of black holes to tests of dark matter models.”

Scientists believe the creation of the long, bright pulse occurred when a massive star in the Sagitta constellation — about 2.4 billion light-years away — collapsed into a supernova explosion and became a black hole. The star was likely many times the mass of our sun.

Gamma rays and X-rays rippled through the solar system and set off detectors installed on NASA’s Fermi Gamma-ray Space Telescope, the Neil Gehrels Swift Observatory and the Wind spacecraft, as well as ground-based telescopes like the Gemini South telescope in Chile.

Newborn black holes blast out powerful jets of particles that can move at close to the speed of light, releasing radiation in the form of X-rays and gamma rays. Billions of years after traveling across space, the black hole’s detonation finally reached our corner of the universe last week.

Studying an event like this can reveal more details about the collapse of stars, how matter interacts near the speed of light and what conditions may be like in distant galaxies. Astronomers estimate that such a bright a gamma ray burst may not appear again for decades.

The burst’s source sounds distant, but astronomically speaking it’s relatively close to Earth, which is why it was so bright and lasted for so long. The Fermi telescope detected the burst for more than 10 hours.

O’Connor was the leader of a team using the Gemini South telescope in Chile, operated by the National Science Foundation’s National Optical-Infrared Astronomy Research Laboratory, or NOIRLab, to observe the aftermath on October 14.

“In our research group, we’ve been referring to this burst as the ‘BOAT’, or Brightest Of All Time, because when you look at the thousands of bursts gamma-ray telescopes have been detecting since the 1990s, this one stands apart,” said Jillian Rastinejad, a doctoral student at Northwestern University in Illinois who led a second team using Gemini South.

Astronomers will use their observations to analyze the signatures of any heavy elements released by the star’s collapse.

The luminous burst also provided an opportunity for two devices aboard the International Space Station: the NICER (or Neutron star Interior Composition Explorer) X-ray telescope and Japan’s Monitor of All-sky X-ray Image, or MAXI. Combined, the two devices are called the Orbiting High-energy Monitor Alert Network, or OHMAN.

It was the first time the two devices, installed on the space station in April, were able to work together to detect a gamma-ray burst, and meant the NICER telescope was able to observe GRB 221009A three hours after it was detected.

“Future opportunities could result in response times of a few minutes,” said Zaven Arzoumanian, NICER science lead at Goddard Space Flight Center in Greenbelt, Maryland, in a statement.

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Mysterious Gamma Rays May Not Be Emanating From The Fermi Bubbles After All : ScienceAlert

A gamma-ray trickster has just been found in the vicinity of the Milky Way.

Energetic radiation previously associated with structures erupting from the Milky Way galactic center called the Fermi bubbles actually seems to instead be coming from something more distant.

The origins are instead thought to be millisecond pulsars in a small dwarf galaxy orbiting our own.

The discovery has implications for our understanding of the Fermi bubbles, but it also could have an impact on broader areas of research, such as the search for galactic dark matter.

The Fermi bubbles were discovered in 2010, and were a huge surprise, quite literally. They are gargantuan bubbles of high-energy gas emanating from the galactic center that extend above and below the galactic plane, for a total distance of 50,000 light-years, expanding at a rate of millions of miles an hour.

A visualization of the Fermi bubbles. (NASA’s Goddard Space Flight Center)

Whatever created them – the Milky Way’s supermassive black hole being a leading candidate – did so millions of years ago, and the bubbles have been blowing upwards and outwards ever since. They’re brighter in high-energy gamma radiation than the rest of the Milky Way’s disk.

Not all the radiation from the Fermi bubbles is evenly distributed. In particular, there is what is described as a “cocoon” of freshly accelerated cosmic rays in the southern lobe, interpreted on its discovery in 2011 as part of the superbubble environment.

Now, a team of astronomers, led by astrophysicist Roland Crocker of the Australian National University in Australia, has noticed something interesting.

The location of the cocoon is directly coincident with the location of another object – the core of Sagittarius dwarf spheroidal galaxy, a satellite of the Milky Way that is in the process of being torn apart and subsumed by the larger galaxy.

This, on its own, would be a pretty big co-inky-dink, with a very low probability of around 1 percent. But it gets even more interesting. The cocoon and the Sagittarius galaxy also have similar shapes and orientations.

Of course, distance in space can be extremely hard to gauge. Unless you know precisely how much light something is emitting, it’s hard to know how far away it is.

If you see something emitting gamma radiation in a larger gamma radiation structure, it’s probably natural to assume that the two are related. But two things with similar shape and orientations lining up directly in our line of sight would be, well, really peculiar.

Not impossible, but there might be a more likely explanation – such as a link between those two objects.

So the researchers decided to revisit the cocoon, and see if the dwarf galaxy could possibly be an alternative explanation for the gamma radiation observed therein.

They modeled the emission over a range of explanations, including the intra-bubble cocoon and the Sagittarius galaxy, and found that, by quite some significance, the Sagittarius galaxy was the most likely emitter of the gamma radiation in the Fermi cocoon.

The next question, naturally, was what could be producing it. In the Milky Way, gamma rays are predominantly generated by collisions between cosmic rays and the gas in the interstellar medium.

This is not possible for the Sagittarius galaxy. The smaller satellite galaxy is gravitationally falling into the Milky Way, and has been for some time; as such its gas has been neatly stripped away, probably around 2 to 3 billion years ago.

Nor have any massive, short-lived stars been dying in spectacular supernovae; these are born from gas, and, well. There is none.

The most likely explanation, the team found, is millisecond pulsars. These are neutron stars (the collapsed, ultra-dense cores of dead massive stars) with extremely fast spin rates, on millisecond scales; as they spin, they emit jets of radiation from their poles – including gamma radiation.

These would be compatible with the most recent episodes of star formation in the Sagittarius galaxy, and have the same spatial distribution as the rest of the stellar population.

Although the gamma radiation seems bright compared to other galaxies such as Andromeda, this would be possible if the pulsars were 7 to 8 billion years old, and low in metal content – consistent with the rest of the Sagittarius population, the researchers say.

This finding suggests that dwarf spheroidal galaxies like Sagittarius might produce more gamma radiation than expected.

If so, they could confound searches for dark matter signals, one of which is hypothesized to be an excess of gamma radiation emitted as dark matter particles and antiparticles mutually annihilate each other.

The possibility, the researchers say, should prompt a closer look at these small, faint galaxies, to see if we need to revise our understanding of dwarf spheroidal galaxies, and the old populations of stars they contain.

The research has been published in Nature Astronomy.

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The Vanishing Variants: Lessons from Gamma, Iota and Mu

In early 2021, scientists in Colombia discovered a worrisome new coronavirus variant. This variant, eventually known as Mu, had several troubling mutations that experts believed could help it evade the immune system’s defenses.

Over the following months, Mu spread swiftly in Colombia, fueling a new surge of Covid-19 cases. By the end of August, it had been detected in dozens of countries, and the World Health Organization had designated it a “variant of interest.”

“Mu was starting to make some noise globally,” said Joseph Fauver, a genomic epidemiologist at the University of Nebraska Medical Center and an author of a recent study on the variant.

And then it fizzled. Today, the variant has all but vanished.

For every Delta or Omicron there is a Gamma, Iota or Mu, variants that drove local surges but never swept to global dominance. And while understanding Omicron remains a critical public health priority, there are lessons to be learned from these lesser lineages, experts say.

“This virus has no incentive to stop adapting and evolving,” said Joel Wertheim, a molecular epidemiologist at the University of California San Diego. “And seeing how it did that in the past will help us prepare for what it might do in the future.”

Studies of the also-rans have shed light on surveillance gaps and policy blunders — providing more evidence that America’s international travel bans were not effective — and on what makes the virus successful, suggesting that in the early phase of the pandemic, transmissibility was more important than immune evasion.

The research also highlights how much context matters; variants that make an impact in some places never gain a foothold in others. As a result, predicting which variants will surge to dominance is difficult, and staying on top of future variants and pathogens will require comprehensive, nearly real-time surveillance.

“We can gain a lot by looking at the viral genomic sequence and saying, ‘This one is probably worse than another one,’” Dr. Wertheim said. “But the only way to really know is to watch it spread, because there are a whole lot of potentially dangerous variants that never took hold.”

The coronavirus is constantly changing, and most new variants never get noticed or named. But others raise alarms, either because they quickly become more common or because their genomes look ominous.

Both were true of Mu as it spread in Colombia. “It contained a couple of mutations that people had been watching very closely,” said Mary Petrone, a genomic epidemiologist at the University of Sydney and an author of the new Mu paper. Several of the mutations in its spike protein had been documented in other immune-evasive variants, including Beta and Gamma.

In the new study, which has not yet been published in a scientific journal, scientists compared Mu’s biological characteristics to those of Alpha, Beta, Delta, Gamma and the original virus. Mu did not replicate faster than any other variant, they found, but it was the most immune-evasive of the bunch — more resistant to antibodies than any known variant besides Omicron, Dr. Fauver said.

By analyzing the genomic sequences of Mu samples collected from all over the world, the researchers reconstructed the variant’s spread. They concluded that Mu had likely emerged in South America in mid-2020. It then circulated for months before it was detected.

Genomic surveillance in many parts of South America was “patchy and incomplete,” said Jesse Bloom, an expert in viral evolution at the Fred Hutchinson Cancer Research Center in Seattle. “If there had been better surveillance in those regions, possibly it would have been easier to make a faster assessment of how worried to be about Mu.”

Mu presented another challenge, too. It happened to have a type of mutation, known as a frameshift mutation, that was rare in coronavirus samples. Such mutations were flagged as errors when scientists, including Dr. Fauver, tried to upload their Mu sequences to GISAID, an international repository of viral genomes used to keep tabs on new variants.

That complication created delays in the public sharing of Mu sequences. The time that elapsed between when a virus sample was collected from a patient and when it was made publicly available on GISAID was consistently longer for Mu cases than for Delta cases, the researchers found.

“The genome itself was basically creating artificial surveillance gaps,” Dr. Fauver said. “It resulted, at least in our experience, in us not getting data out for weeks when normally we’re trying to get it out in days.”

(GISAID’s quality-control systems are important, the researchers stressed, and the repository has fixed the issue.)

Combine these surveillance gaps with Mu’s immune evasiveness and the variant seemed poised to take off. But that is not what happened. Instead, Mu radiated from South and Central America to other continents but did not circulate widely once it got there, the scientists found. “That was an indication that this variant was not as fit necessarily in maybe the North American and European populations as we had expected,” Dr. Petrone said.

That was likely because Mu found itself competing with an even more formidable variant: Delta. Delta was not as skilled at dodging antibodies as Mu, but it was more transmissible. “So, in the end, Delta spread more widely,” Dr. Bloom said.

Studying successful variants tells only half the story. “Variants that do not become dominant are, in a way, negative controls,” Dr. Petrone said. “They tell us what didn’t work, and, in doing so, help to fill in knowledge gaps around variant fitness.”

Delta overtook several immune-evasive variants besides Mu, including Beta, Gamma and Lambda. This pattern suggests that immune evasion alone was not enough to allow a variant to outdo a highly transmissible version of the virus — or at least it wasn’t during the early phase of the pandemic, when few people had immunity.

But vaccinations and multiple waves of infection have changed the immune landscape. A highly immune-evasive variant should now have more of an edge, scientists said, which is likely part of the reason Omicron has been so successful.

Another recent study suggested that in New York City immune-evasive Gamma tended to do better in neighborhoods with higher levels of pre-existing immunity, in some cases because they were hit hard in the first Covid wave. “We can’t view a new variant in a vacuum, because it comes about in the shadow of all of the variants that came before it,” said Dr. Wertheim, who was an author of the study.

Indeed, the clash of variants past reveals that success is highly dependent on context. For example, New York City may have been the birthplace of the Iota variant, which was first detected in virus samples collected in November 2020. “And so it got a foothold early on,” said Dr. Petrone. Even after the more transmissible Alpha variant arrived, Iota remained the city’s dominant variant for months, before eventually fading away.

But in Connecticut, where Iota and Alpha both appeared in January 2021, things unfolded differently. “Alpha just kind of took off immediately, and Iota didn’t stand a chance,” said Dr. Petrone, who led a study of the variants in the two regions.

A similar pattern is already beginning to play out with Omicron’s multiple lineages. In the United States, BA.2.12.1, a subvariant first identified in New York, has taken off, while in South Africa, BA.4 and BA.5 are driving a new surge.

That’s another reason to study variants that waned, said Sarah Otto, an evolutionary biologist at the University of British Columbia. A variant that was poorly matched for a certain time and place could take off in another. Indeed, Mu’s misfortune might have simply been that it emerged too soon. “There might not have been enough people that had immunity to really give that variant a boost,” Dr. Otto said.

But the next variant of concern could be a descendant of, or something similar to, an immune-evasive lineage that never quite took hold, she said.

Looking back at previous variants can also provide insight into what worked — or didn’t — in containing them. The new Gamma study, provides further evidence that international travel bans, at least as the United States implemented them, are unlikely to prevent a variant’s global spread.

Gamma was first identified in Brazil in late 2020. In May of that year, the United States barred most non-U.S. citizens from traveling into the country from Brazil, a restriction that remained in place until November 2021. Yet Gamma was detected in the United States in January 2021 and soon spread to dozens of states.

Because Gamma never came to dominate worldwide, studying its spread provided a “cleaner” picture of the effectiveness of travel bans, said Tetyana Vasylyeva, a molecular epidemiologist at the University of California San Diego and an author of the study. “When it comes to studying variants like, let’s say, Delta — something that has caused a major outbreak in every place — it is really difficult at times to find patterns, because it happens on a very large scale and very fast,” she said.

In an ongoing global health emergency, with a virus that changes fast, there is an understandable impulse to focus on the future, Dr. Fauver said. And as the world’s attention turned to Delta and then Omicron, he and his colleagues discussed whether to continue their study of old-news Mu.

“We were like, ‘Does anyone care about Mu anymore?’” Dr. Fauver recalled. “But we think there’s still room for high-quality studies that ask questions about previous variants of concern and try to look back on what happened.”

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Something’s Glowing at The Galactic Core, And We Could Be Closer to Solving The Mystery

Something deep in the heart of the Milky Way galaxy is glowing with gamma radiation, and nobody can figure out for sure what it might be.

Colliding dark matter has been proposed, ruled out, and then tentatively reconsidered.

 

Dense, rapidly rotating objects called pulsars were also considered as candidate sources of the high-energy rays, before being dismissed as too few in number to make the sums work.

A study by researchers from Australia, New Zealand and Japan could breathe new life into the pulsar explanation, revealing how it might be possible to squeeze some serious intense sunshine from a population of spinning stars without breaking any rules.

Gamma radiation isn’t your typical hue of sunlight. It requires some of the Universe’s most energetic processes to produce. We’re talking black holes colliding, matter being whipped towards light speed, antimatter combining with matter kinds of processes.

Of course, the center of the Milky Way has all of these things in spades. So when we gaze into the heavens and consider all of the crashing bits of matter, spiraling black holes, whizzing pulsars, and other astrophysical processes, we’d expect to see a healthy gamma glow.

But when researchers used NASA’s Fermi telescope to measure the intense shine within the heart of our galaxy about ten years ago, they found there was more of this high-energy light than they could account for: what’s known as the Galactic Centre Excess.

 

One exciting possibility involves unseen bits of matter bumping together in the night. These weakly interacting massive particles – a hypothetical category of dark matter commonly described as WIMPs – would cancel each other out as they smoosh together, leaving nothing but radiation to mark their presence.

It’s a fun explanation to consider, but is also light on evidence.

“The nature of dark matter is entirely unknown, so any potential clues garner a lot of excitement,” says astrophysicist Roland Crocker from the Australian National University.

“But our results point to another important source of gamma ray production.”

That source is the millisecond pulsar.

To make one, take a star much bigger than our own and let its fires die down. It will eventually collapse into a dense ball not much wider than a city, where its atoms pack together so tightly, many of its protons are slowly baked into neutrons.

This process generates super-strong magnetic fields that channel incoming particles into fast-flowing streams glowing with radiation.

Since the object is rotating, these streams swivel around from the star’s poles like the Universe’s biggest lighthouse beacons – so it appears to pulse with energy. Pulsing stars that spin hundreds of times a second are known as millisecond pulsars, and we know a lot about the conditions under which they’re likely to form.

 

“Scientists have previously detected gamma-ray emissions from individual millisecond pulsars in the neighborhood of the Solar System, so we know these objects emit gamma rays,” says Crocker.

To emit them, however, they’d need a generous amount of mass to feed on. Most pulsar systems in the center of the Milky Way are thought to be too puny to emit anything more energetic than X-rays, though.

That might not always be the case, however, especially if the dead stars they emerged from are of a particular variety of ultra-massive white dwarf.

According to Crocker, if enough of these heavyweights were to turn into pulsars and hold onto their binary partners, they would provide just the right amount of gamma radiation to match observations.

“Our model demonstrates that the integrated emission from a whole population of such stars, around 100,000 in number, would produce a signal entirely compatible with the Galactic Centre Excess,” says Crocker.

Being a purely theoretical model, it’s an idea that now needs a generous dose of empirical evidence. Unlike suggestions based on dark matter, however, we already know exactly what to look for.

This research was published in Nature Astronomy.  

 

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Mysterious Glow Caught in Our Galaxy’s Center Really Could Be Due to Dark Matter

The center of the Milky Way is mysteriously glowing.

Sure, there’s a whole bunch of stars there, along with a black hole 4 million times the mass of the Sun – but subtract the light from all that, and we’re still left with this mysterious excess gamma radiation that suffuses the region.

 

It’s called the Galactic Center GeV Excess (GCE), and it’s puzzled scientists since its discovery by physicists Lisa Goodenough and Dan Hooper in 2009. In data from NASA’s Fermi telescope, they found excess gamma radiation – some of the most energetic light in the Universe – and we haven’t been able to directly detect whatever is causing it.

Now physicist Mattia Di Mauro of the National Institute for Nuclear Physics in Italy has thrown his hat into the ring. His analysis, he said, points back at dark matter as the GCE culprit (this was first floated as an explanation by Goodenough and Hooper).

We don’t know what dark matter is, just that there’s a mysterious mass out there responsible for gravitational effects that can’t be explained by the stuff we can detect directly – the normal matter such as stars, dust, gas, and galaxies.

For example, galaxies rotate much faster than they should if they were just being gravitationally influenced by the normal matter in them; gravitational lensing – the bending of spacetime around massive objects – is far stronger than it should be. Whatever is creating this additional gravity is beyond our ability to detect directly.

 

We know dark matter only by the gravitational effect it has on other objects, and there is a lot of it out there. Roughly 80 percent of all matter in the Universe is dark matter, even though we can’t see a scrap of it.

Goodenough and Hooper proposed that, if certain dark matter particles called WIMPS (weakly interacting massive particles) and their antiparticles were to collide, they would annihilate each other, exploding in a shower of other particles, including gamma-ray photons. This explanation, they said, fit the data surprisingly well. Other physicists were not convinced, one even calling the explanation “shaky”.

In 2018, another team of scientists proposed that very old, dead stars called pulsars that we haven’t yet seen could be causing the excess. This is plausible, because the galactic center is crowded, dusty, and very energetic – it would be pretty easy to miss a star or several.

Recent studies also found that the distribution of the GCE isn’t smooth – as you would expect from dark matter annihilation – but sort of clumpy and speckled, which the pulsar team interpreted as consistent with point sources, like stars.

 

Then another team came along and ruled that speckly gamma radiation could be produced by dark matter, putting it back on the table. Yet more researchers then generated a series of exhaustive models of the galactic center with dark matter annihilation using a range of masses across the most commonly searched regimes. They found that WIMPs were unlikely to be the cause of the GCE.

Back to Di Mauro. His study compares data from the Fermi telescope over the last 11 years against measurements of other astronomical anomalies recorded by the Pamela cosmic ray detector aboard the Resurs-DK No.1 satellite and the Alpha Magnetic Spectrometer experiment aboard the ISS.

In particular, his study uses the broadest set of data from Fermi collected over the last year, and minimizes the uncertainties introduced by background radiation. This has provided, Di Mauro said, information about the spatial distribution of the GCE that can help rule out various explanations.

“If the excess was, for example, caused by the interaction between cosmic rays and atoms, we would expect to observe its greater spatial distribution at lower energies and its lower diffusion at higher energies due to the propagations of cosmic particles,” he explained.

“My study, on the other hand, underlines how spatial distribution of the excess does not change as a function of energy.”

This, he said, had never been observed before, and could be explained by dark matter, since we think that dark matter particles should have similar energies.

“The analysis clearly shows that the excess of gamma rays is concentrated in the galactic center, exactly what we would expect to find in the heart of the Milky Way if dark matter is in fact a new kind of particle,” he said.

As for what that particle is, it’s still a huge mystery. In a second preprint paper, Di Mauro and his colleague Martin Wolfgang Winkler of Stockholm University in Sweden have attempted to bring it out of the shadows by searching for a gamma-ray excess in nearby dwarf spheroidal galaxies. They didn’t find one, but that null detection has enabled constraints on the mass of the dark matter particle.

These constraints, they said, are compatible with the GCE.

So does this mean dark matter is causing the GCE? No – but it means we can’t say dark matter isn’t causing it, either. Basically, the whole thing is as puzzling as it’s ever been, and we’re going to need some pretty fascinating science (and a lot more observations, probably) to even begin to untangle it.

We can feel a great disturbance in the force, like many physicists rubbing their hands together in anticipatory glee.

Di Mauro’s research has been published in Physical Review D, and the second paper is available on arXiv.

 

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