Over billions of years, small black holes can slowly grow into the supermassive variety by taking on mass from their surroundings and by merging with other black holes. But this slow process can't explain the problem of supermassive black holes existing in the early universe. New findings may help to test a model that solves this problem.
Leslie Rosenberg and his colleagues are about to go hunting. Their quarry: A theorized-but-never-seen elementary particle called an axion. The search will be conducted with a recently retooled, extremely sensitive detector that is currently in a testing and shakeout phase at the University of Washington’s Center for Experimental Nuclear Physics and Astrophysics.
Semiconductors have had a nice run, but for certain applications, such as astrophysics, they are being edged out by superconductors. Ben Mazin, asst. prof. of physics at the Univ. of California, Santa Barbara, has developed a superconducting detector array that measures the energy of individual photons.
Doom may be averted for the Smith Cloud, a gigantic streamer of hydrogen gas that is on a collision course with the Milky Way Galaxy. Astronomers have discovered a magnetic field deep in the cloud’s interior, which may protect it during its meteoric plunge into the disk of our galaxy. This discovery could help explain how so-called high velocity clouds remain mostly intact during their mergers with the disks of galaxies.
Astronomers have calculated the odds that, sometime during the next 50 years, a supernova occurring in our home galaxy will be visible from Earth. The good news: They’ve calculated the odds to be nearly 100% that such a supernova would be visible to telescopes in the form of infrared radiation. The bad news: The odds are much lower that the shining stellar spectacle would be visible to the naked eye in the nighttime sky.
Nearly a mile underground in an abandoned gold mine, one of the most important quests in physics has so far come up empty in the search for the elusive substance known as dark matter, scientists announced Wednesday. But physicists on the project were upbeat, saying they had developed a new, more sensitive method of searching for the mysterious material that has mass but cannot be seen. They planned to keep looking.
New evidence of heavy elements spread evenly between the galaxies of the giant Perseus cluster supports the theory that the universe underwent a turbulent and violent youth more than 10 billion years ago. That explosive period was responsible for seeding the cosmos with the heavy elements central to life itself.
In August, Massachusetts Institute of Technology researchers identified an exoplanet with an extremely brief orbital period: The team found that Kepler 78b, a small, intensely hot planet 400 light-years from Earth, circles its star in just 8.5 hrs. Now this same team has found that Kepler 78b shares another characteristic with Earth: its mass.
Dark matter, believed by physicists to outweigh all the normal matter in the universe by more than five to one, is by definition invisible. But certain features associated with dark matter might be detectable, according to some of the many competing theories describing this elusive matter. Now scientists have developed a tool that could test some of these predictions and thus prove, or disprove, one of the leading theories.
At a cosmologically crisp 1 K (-458 F), the Boomerang Nebula is the coldest known object in the Universe—colder, in fact, than the faint afterglow of the Big Bang, which is the natural background temperature of space. Astronomers using the Atacama Large Millimeter/submillimeter Array telescope have taken a new look at this ghostly object to learn more about its frigid properties and to determine its true shape.
The journey of light from the very early universe to modern telescopes is long and winding. The ancient light traveled billions of years to reach us, and along the way, its path was distorted by the pull of matter, leading to a twisted light pattern. This twisted pattern of light, called B-modes, has at last been detected and will lead to better maps of matter across our universe.
For the threat of meteor strikes large or small, early detection is key, and evacuation may be the only defense needed within the next 1,000 years, according to an asteroid impact expert. The best investment in asteroid defense is not in weapons to deflect them, but in telescopes and surveys to find them.
The universe is a vast and mysterious place, but thanks to high-performance computing technology scientists around the world are beginning to understand it better. They are using supercomputers to simulate how the Big Bang generated the seeds that led to the formation of galaxies such as the Milky Way.
In a 3-m-dia hollow aluminum sphere, Cary Forest, a Univ. of Wisconsin-Madison physics prof., is stirring and heating plasmas to 500,000 F to experimentally mimic the magnetic field-inducing cosmic dynamos at the heart of planets, stars and other celestial bodies. Ninety-three million miles away, the sun's magnetic field is churning and undulating as the star experiences the height of the so-called solar maximum.
Francois Englert of Belgium and Peter Higgs of Britain won the 2013 Nobel Prize in physics for their theoretical discoveries on how subatomic particles acquire mass. Their theories are key to explaining the building blocks of matter and the origins of the universe. They were confirmed last year by the discovery of the so-called Higgs particle, also known as the Higgs boson, at CERN, the Royal Swedish Academy of Sciences said.
At first glance, Mars’ clouds might be mistaken for those on Earth. Given what scientists know about the Red Planet’s atmosphere, these clouds likely consist of either carbon dioxide or water-based ice crystals. But it’s difficult to know the precise conditions that give rise to such clouds without sampling directly from a Martian cloud. Researchers at Massachusetts Institute of Technology have now done the next-best thing.
A new look at the early solar system introduces an alternative to a long-taught, but largely discredited, theory that seeks to explain how biomolecules were once able to form inside of asteroids. In place of the outdated theory, researchers at Rensselaer Polytechnic Institute propose a new theory to explain the ancient heating of the asteroid belt.
A fleet of orbiting x-ray telescopes has been used by an international team of scientists in the discovery of a "millisecond pulsar" star with a dual identity. The star readily shifts back and forth between two mutually exclusive styles of pulsed emissions, one in x-rays, the other in radio waves. The discovery, the scientists say, reveals a long-sought intermediate phase in the life of these powerful objects.
For astrophysicists, the interplay of hydrogen and the clouds of dust that fill the voids of interstellar space has been an intractable puzzle of stellar evolution. The dust, astronomers believe, is a key phase in the lifecycle of stars, which are formed in dusty nurseries throughout the cosmos. But how the dust interacts with hydrogen and is oriented by the magnetic fields in deep space has proved a theoretical challenge. Until now.
Kids grumble about homework. But their complaints will hold no water with a group of theoretical physicists who’ve spent almost 50 years solving one homework problem: a calculation of one type of subatomic particle decay aimed at helping to answer the question of why the early universe ended up with an excess of matter. Without that excess, the matter and antimatter created in the Big Bang would have completely annihilated one another.
Imagine the distance between the sun and the star nearest to it—a star called Alpha Centauri. That’s a distance of about 4 light years. Now, imagine as many as 10,000 of our suns crammed into that relatively small space. That is about the density of a galaxy that was recently discovered by an international team of astronomers led by a Michigan State Univ. faculty member.
Since the discovery of the Van Allen radiation belts in 1958, space scientists have believed these belts encircling the Earth consist of two doughnut-shaped rings of highly charged particles. In February of 2013, a team of scientists reported the surprising discovery of a previously unknown third radiation ring. In new research, scientists have successfully modeled and explained the unprecedented behavior of this third ring.
To get a better understanding of the subatomic soup that filled the early universe, and how it “froze out” to form the atoms of today’s world, scientists are taking a closer look at the nuclear phase diagram. Like a map that describes how the physical state of water morphs from solid ice to liquid to steam with changes in temperature and pressure, the nuclear phase diagram maps out different phases of the components of atomic nuclei.
Like the wind adjusting course in the middle of a storm, scientists have discovered that the particles streaming into the solar system from interstellar space have most likely changed direction over the last 40 years. Such information can help us map out our place within the galaxy surrounding us, and help us understand our place in space.
The origin of cosmic rays in the universe has confounded scientists for decades. But a study by researchers using data from the IceCube Neutrino Observatory at the South Pole reveals new information that may help unravel the longstanding mystery of exactly how and where these “rays”, which are actually high-energy particles, are produced.