Agravity, short for ‘adimensional gravity’, is one of the most recent Theory of Everything proposals in a long line of such proposals that have come about ever since the problem of reconciling Gravity with the Standard Model was realized by physicists. It attempts to merge gravity with the Higgs interaction, and thus the rest of the Standard Model, by reconciling the huge difference between the Planck Scale and the relatively small masses of all the other particles. (Credit: SGTW, Daniels)
The decision to reformat Opportunity’s flash memory early next month is prompted by the multiple computer resets the rover has been experiencing. This month alone, Opportunity has had to be rebooted a dozen times, interrupting valuable time that should be taken up with carrying out science near the rim of Endeavour crater. (Credit: NASA, O’Neil)
“It’s fascinating that the early universe could make galaxies in this way and the modern universe just can’t anymore, and we’re really beginning to understand in a profound way how different the early universe was than it is now,” said Erica Nelson of Yale University. (Credit: Neslson)
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NASA’s Van Allen Probes orbit through two giant radiation belts surrounding Earth. Their observations help explain how particles in the belts can be sped up to nearly the speed of light. Image (Credit: NASA)
This is a scanning electron microscope image of an interplanetary dust particle that has roughly chondritic elemental composition and is highly rough (chondritic porous: “CP”). CP types are usually aggregates of large numbers of sub-micrometer grains, clustered in a random open order. (Credit: Donald E. Brownlee)
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Inflation explains the origin of the large-scale structure of the cosmos. Many physicists believe that inflation explains why the Universe appears to be the same in all directions (isotropic), why the cosmic microwave background radiation is distributed evenly, why the universe is flat, and why no magnetic monopoles have been observed. (Credit: NASA)
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Engineers just completed hot-fire testing with two 3-D printed rocket injectors. Certain features of the rocket components were designed to increase rocket engine performance. The injector mixed liquid oxygen and gaseous hydrogen together, which combusted at temperatures over 6,000 degrees Fahrenheit, producing more than 20,000 pounds of thrust. (Credit: NASA photo/David Olive)
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Three consecutive images of comet C/1979 Q1 plunging into the solar atmosphere on August 30, 1979. In these SOLWIND coronagraph images, the Sun is masked behind the solid disk in the center of the image. (Credit: NRL)
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Before the big explosion: The artist’s impression shows a binary star system where mass is transferred from a companion to a white dwarf. As soon as sufficient matter has collected on the surface of the dwarf star, this can trigger a nuclear explosion which in turn ignites the catastrophic nuclear burning and destroys the white dwarf – a type Ia supernova flares up. (Credit: ESA, Justyn R. Maund)
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Director of distilling, Bill Lumsden. Ardbeg Scottish whisky was sent into space three years ago in an experiment looking at the impact of gravity on how it matures. It will return to Earth September 12th. (Credit: Paul Dodds/Ardbeg/PA)
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NASA has warned that a new sunspot spewing powerful X-class flares is beginning to rotate to a position directly in line with Earth. (Credit: NASA)
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In the past decade an extraordinary claim has captivated cosmologists: that the expanding universe we see around us is not the only one; that billions of other universes are out there, too. (Credit: Slim Films, Ellis)
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Neutron-rich magnesium nuclei have a neutron halo that extends beyond the tightly packed core of the nucleus. (Credit: K. Yoneda, RIKEN Nishina Center for Accelerator-Based Science)
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On August 30th, 1984, the space shuttle Discovery launched on its first voyage to space. It wasn’t the first, but over the next 27 years it became the undeniable king of NASA’s shuttle program. (Credit: NASA)
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“This is a long-standing, really neat experimental idea,” says Paul Lett, of the National Institute of Standards and Technology in GaithersburgLett, “Now we have to see whether or not it will lead to something practical, or will remain just a clever demonstration of quantum mechanics.”(CreditBarreto-Lemos, Vergano)
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The Borexino neutrino detector uses a sphere filled with liquid scintillator that emits light when excited. This inner vessel is surrounded by layers of shielding and by about 2,000 photomultiplier tubes to detect the light flashes.(Credit: Borexino Collaboration)
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MOLECULAR MODEL In the molecular model, quark-antiquark pairs form two color-neutral mesons that become weakly linked as a molecule.DIQUARK MODEL The particles form quark-quark and antiquark-antiquark pairs, which are forced to combine to balance their color charges.
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A computer model shows one scenario for how light is spread through the early universe on vast scales (more than 50 million light years across). Astronomers will soon know whether or not these kinds of computer models give an accurate portrayal of light in the real cosmos. (Credit: Andrew Pontzen/Fabio Governato)
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Radio/optical composite of the Orion Molecular Cloud Complex showing the OMC-2/3 star-forming filament. GBT data is shown in orange. Uncommonly large dust grains there may kick-start planet formation. (Credit: S. Schnee, et al.; B. Saxton, B. Kent (NRAO/AUI/NSF)
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In one potential method to realize superabsorption, a superabsorbing ring absorbs incident photons, giving rise to excitons. (Credit: Higgins, et al.)
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Finding clouds of water floating in the atmosphere of an alien world is a significant find. Now, astronomers have reported preliminary findings that water clouds have been detected in the atmosphere of a brown dwarf, a mere 7.3 light-years from Earth. (Credit: NASA, JPL-Caltech, O’neil)
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NASA mechanical engineer, Brian Trease, worked with Brigham Young University doctoral student Shannon Zirbel, and collaborated with origami expert Robert Lang, who has long been active in promoting it in science, and BYU professor Larry Howel, to combine different traditional folds for an 82-foot solar array that whirls down to 8.9 feet. (Credit: BYU, Meier)
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“If we find a noise we can’t get rid of, we might be detecting something fundamental about nature – a noise that is intrinsic to space-time,” said Physicist Aaron Choi, the holometer project’s lead scientist. (Credit: NASA, ESA)
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In this picture, which combines views from Hubble and the Keck-II telescope on Hawaii (using adaptive optics), you can see a foreground galaxy that is acting as the gravitational lens. The galaxy resembles how our home galaxy, the Milky Way, would appear if seen edge-on. But around this galaxy there is an almost complete ring — the smeared out image of a star-forming galaxy merger far beyond. (Credit: NASA, ESA)
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With a circumference of 52km, the “Higgs Factory” would be almost twice the size of Europe’s equivalent, and significantly more powerful. The Chinese said it is due to be completed by 2028. Image above is the Large Hadron Collider. (Credit: Getty)
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This diagram shows how the effect of gravitational lensing around a normal galaxy focuses the light coming from a very distant star-forming galaxy merger to created a distorted, but brighter view. (Credit: ESA/ESO/M. Kornmesser)
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As seen under an optical microscope, the heterostructures have a triangular shape. The two different monolayer semiconductors can be recognized through their different colors. (Credit: U of Washington)
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“It’s the most distant object for which the spin has been directly measured. The universe is about 13.7 billion years old, so this is going significantly back towards when the epoch of furious galaxy formation was happening,” says, Astrophysicist, Mark Reynolds.
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This image sometimes circulates on Facebook, with the claim that Mars will appear as big and bright as a full moon on August 27, 2014. It’s a hoax. Don’t believe it. Mars never appears as large as a full moon in Earth’s sky. (Credit: Unknown)
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A optical microscope image of the spintronic device (top view). The top electrode (tg) and cobalt electrodes (1 to 5) are yellow. The boron nitride layers (in green) encapsulate the graphene flake, which is outlined by the dotted line. Credit: Fundamental Research on Matter (Credit: FOM)
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Alessandro Strumia of the University of Pisa, pictured speaking at a conference in 2013, has co-developed a scale-symmetric theory of particle physics called “agravity.” (Credit: Thomas Lin/Quanta Magazine)
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X-ray interference pattern measured while studying complex nano-layer structures. The sketch inserted illustrates the path of the x-ray beam relative to the surface of the sample. (Credit: Sebastian Macke)
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Three weeks after launching the AsiaSat-8 communications satellite, SpaceX is primed to deliver its sibling, AsiaSat-6, into geostationary transfer orbit at an altitude of 22,236 miles (35,786 km) on Wednesday, 27 August. (Credit: AsiaSat)
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Relative intensity (top row) and pre-trial significance (bottom row) of the cosmic-ray flux in the vicinity of Region A (left), Region B (center), and Region C (right). (Credit: Abeysekara et al)
The very first stars in the Universe might have been hundreds of times more massive than the Sun. (Credit: National Astronomical Observatory of Japan)
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Jonathan Menard, a principal research physicist and program director for the National Spherical Torus Experiment (NSTX), and Masa Ono, a principal research physicist and project director of the NSTX, stand in front of the experiment during a tour of the facility. The device has been shut down since 2011 while it undergoes a $94 million upgrade that will make it the most powerful device of its kind in the world. (Credit NSTX)
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The agency intends to deploy the spacecraft, codename Liquidator, to clear up the geostationary orbit over the equator, which is 36 thousand kilometers above sea level. (Credit: Roscosmos)
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“When you start to make electronics smaller and denser, not only are you making much more heat in the same amount of volume, but it’s much harder for the heat to flow outward,” says Peter Nalbach, a theoretical physicist at the University of Hamburg, Germany. (Credit: Mehau Kulyk/Getty)
via popularmechanics
Researchers hope to create a massive online “brain” that can help all robots navigate and even understand the world around them. “The purpose,” says Saxena, who dreamed it all up, “is to build a very good knowledge graph—or a knowledge base—for robots to use. (Credit: Thinkstock, Hernandez )
via wired
Probability density of an Efimov trimer state at different three-body geometries that are characterized by the polar angle — indicated by the trimer legends. The key feature in the probability density is that unlike ordinary molecular binding that mostly has a single geometry, the Efimov trimer covers have a broad range of geometries. The atoms in such states behave more like in a fluid drop. (Credit: Yujun Wang, Kansas State University)
