Have Experimentalists Discovered Dark Matter?

3D map of the large-scale distribution of dark matter, reconstructed from measurements of weak gravitational lensing with the Hubble Space Telescope (Credit: Wikipedia)
3D map of the large-scale distribution of dark matter, reconstructed from measurements of weak gravitational lensing with the Hubble Space Telescope (Credit: Wikipedia)

Scientists have long known that dark matter is out there, silently orchestrating the universe’s movement and structure. But what exactly is dark matter made of? And what does a dark matter particle look like? That remains a mystery, with experiment after experiment coming up empty handed in the quest to detect these elusive particles.

The Bullet Cluster: HST image with overlays. The total projected mass distribution reconstructed from strong and weak gravitational lensing is shown in blue, while the X-ray emitting hot gas observed with Chandra is shown in red. (Credit: Wikipedia)
The Bullet Cluster: HST image with overlays. The total projected mass distribution reconstructed from strong and weak gravitational lensing is shown in blue, while the X-ray emitting hot gas observed with Chandra is shown in red. (Credit: Wikipedia)

With some luck, that may be about to change. With ten times the sensitivity of previous detectors, three recently funded dark matter experiments have scientists crossing their fingers that they may finally glimpse these long-sought particles. In recent conversations with The Kavli Foundation, scientists working on these new experiments expressed hope that they would catch dark matter, but also agreed that, in the end, their success or failure is up to nature to decide.

Read the Transcript: Kavil Foundation Dark Matter Transcript

“Nature is being coy,” said Enectali Figueroa-Feliciano, an associate professor of physics at the MIT Kavli Institute for Astrophysics and Space Research who works on one of the three new experiments. “There’s something we just don’t understand about the internal structure of how the universe works. When theorists write down all the ways dark matter might interact with our particles, they find, for the simplest models, that we should have seen it already. So even though we haven’t found it yet, there’s a message there, one that we’re trying to decode now.”

Dark matter particles known as axions streaming from the sun, converting in Earth’s magnetic field (red) to x-rays, which are detected by the XMM-Newton observatory. (Credit: University of Leicester)
Dark matter particles known as axions streaming from the sun, converting in Earth’s magnetic field (red) to x-rays, which are detected by the XMM-Newton observatory. (Credit: University of Leicester)

The first of the new experiments, called the Axion Dark Matter eXperiment, searches for a theoretical type of dark matter particle called the axion. ADMX seeks evidence of this extremely lightweight particle converting into a photon in the experiment’s high magnetic field. By slowly varying the magnetic field, the detector hunts for one axion mass at a time.

“We’ve demonstrated that we have the tools necessary to see axions,” said Gray Rybka, research assistant professor of physics at the University of Washington who co-leads the ADMX Gen 2 experiment. “With Gen2, we’re buying a very, very powerful refrigerator that will arrive very shortly. Once it arrives, we’ll be able to scan very, very quickly and we feel we’ll have a much better chance of finding axions – if they’re out there.”

According to supersymmetry, dark-matter particles known as neutralinos (aka WIMPs) annihilate each other, creating a cascade of particles and radiation. (Credit: Sky & Telescope / Gregg Dinderman)
According to supersymmetry, dark-matter particles known as neutralinos (aka WIMPs) annihilate each other, creating a cascade of particles and radiation. (Credit: Sky & Telescope / Gregg Dinderman)

The two other new experiments look for a different type of theoretical dark matter called the WIMP. Short for Weakly Interacting Massive Particle, the WIMP interacts with our world very weakly and very rarely. The Large Underground Xenon, or LUX, experiment, which began in 2009, is now getting an upgrade to increase its sensitivity to heavier WIMPs. Meanwhile, the Super Cryogenic Dark Matter Search collaboration, which has looked for the signal of a lightweight WIMP barreling through its detector since 2013, is in the process of finalizing the design for a new experiment to be located in Canada.

“In a way it’s like looking for gold,” said Figueroa-Feliciano, a member of the SuperCDMS experiment. “Harry has his pan and he’s looking for gold in a deep pond, and we’re looking in a slightly shallower pond, and Gray’s a little upstream, looking in his own spot. We don’t know who’s going to find gold because we don’t know where it is.”

Astronomers use the idea of dark matter to account for a substantial portion of the mass of our universe. An even greater amount of mass, they believe, is taken up with dark energy. Meanwhile, the visible stars and galaxies we see around us in space may be only a small part of the whole universe. (Credit: Wikimedia Commons.)
Astronomers use the idea of dark matter to account for a substantial portion of the mass of our universe. An even greater amount of mass, they believe, is taken up with dark energy. Meanwhile, the visible stars and galaxies we see around us in space may be only a small part of the whole universe. (Credit: Wikimedia Commons.)

Rybka agreed, but added the more optimistic perspective that it’s also possible that all three experiments will find dark matter. “There’s nothing that would require dark matter to be made of just one type of particle except us hoping that it’s that simple,” he said. “Dark matter could be one-third axions, one-third heavy WIMPs and one-third light WIMPs. That would be perfectly allowable from everything we’ve seen.”

Yet the nugget of gold for which all three experiments search is a very valuable one. And even though the search is difficult, all three scientists agreed that it’s worthwhile because glimpsing dark matter would reveal insight into a large portion of the universe.

"Cold Dark Matter: An Exploded View" Art Print by Cornelia Parker.  An artistic interpretation of Dark Matter. (Credit: Cornelia Parker)
“Cold Dark Matter: An Exploded View” Art Print by Cornelia Parker. An artistic interpretation of Dark Matter. (Credit: Cornelia Parker)

“We’re all looking and somewhere, maybe even now, there’s a little bit of data that will cause someone to have an ‘Ah ha!’ moment,” said Harry Nelson, professor of physics at the University of California, Santa Barbara and science lead for the LUX upgrade, called LUX-ZEPLIN. “This idea that there’s something out there that we can’t sense yet is one of those things that sends chills down my spine.”

Via: Kavi Institute

 

 

 

Watch an Amazing Solar Flare

SDO captured a splendid example of expanding coronal loops seen in profile at the edge of the Sun (Oct. 14-15, 2014). The bright loops began to form and grow after a long-lasting M-class flare erupted. The arcs of the loops we see in extreme ultraviolet light are actually particles spiraling along magnetic field lines arcing above the active region that was the source of the flare. They are reorganizing the magnetic field after its disruption. To give a sense of scale, these huge loops are reaching out more than 15 times the size of Earth.

(Credit: Solar Dynamics Observatory/NASA)

 

Physics in the News

Wednesday, September 24, 2014

New Results from Planck: It Doesn’t Look Good For BICEP2

Dust map of the Universe. The region studied by BICEP2 is indicated by the rectangle in the right circle. (Credit: Planck Collaboration)
Dust map of the Universe. The region studied by BICEP2 is indicated by the rectangle in the right circle. (Credit: Planck Collaboration)
via universetoday

Artificial Atoms Talk … and Scientists Listen

n this illustration, the artificial atom on the right side of the image sends out sound waves that are picked up by the microphone on the left. (Credit: Philip Krantz)
n this illustration, the artificial atom on the right side of the image sends out sound waves that are picked up by the microphone on the left. (Credit: Philip Krantz)
via livescience

What’s Next for Inflation Cosmology – New Updates

(Credit: Andrei Linde)
A serious challenge to the discovery of gravity waves by the BICEP2 2014 results has appeared: the researchers had underestimated the amount of interstellar dust that could be contaminating their data. (Credit: MacRobert, Andrei Linde)
via skyandtelescope

Clear skies reveal water on distant Neptune-sized planet

Scientists have found definitive traces of water on a relatively small exoplanet. HAT-P-11b is the size of Neptune and has copious amounts of both water vapor and hydrogen in its atmosphere. (Credit: NASA)
Scientists have found definitive traces of water on a relatively small exoplanet. HAT-P-11b is the size of Neptune and four times the size of Earth. The exoplanet has copious amounts of both water vapor and hydrogen in its atmosphere. (Credit: NASA)
via bbc

Hugh Everett: The man who gave us the multiverse

via newscientist

What is the geometry of the universe?

Our current model of the early inflationary period predicts that the universe should be flat, and so far that has held up. If the universe actually is curved, then the inflationary period must have been more complex than we have thought. (Credit: Koberlien)
Our current model of the early inflationary period predicts that the universe should be flat, and so far that has held up. If the universe actually is curved, then the inflationary period must have been more complex than we have thought. (Credit: Koberlien)
via phys.org

Robot Octopus Takes to the Sea

via spectrum

Physics in the News

Friday, September 19, 2014

An anomaly in satellites’ flybys confounds scientists

An artist's rendition of Rosetta probe during a flyby. (Credit: ESA/C.Carreau)
When space probes, such as Rosetta and Cassini, fly over certain planets and moons, in order to gain momentum and travel long distances, their speed changes slightly for an unknown reason. A researcher has now analyzed whether or not a hypothetical gravitomagnetic field could have an influence. However, other factors such as solar radiation, tides, or even relativistic effects or dark matter could be behind this mystery. An artist’s rendition of Rosetta probe during a flyby. (Credit: ESA/C.Carreau)
via sciencedaily

Particle detector finds hints of dark matter in space

The starboard truss of the International Space Station while Space Shuttle Endeavour docked with the station. The newly installed Alpha Magnetic Spectrometer (AMS) is visible at center left. (Credit: NASA)
The starboard truss of the International Space Station while Space Shuttle Endeavour docked with the station. The newly installed Alpha Magnetic Spectrometer (AMS) is visible at center left. (Credit: NASA)
via mit

Finding dark energy in the details

The dome of the Blanco Telescope, which houses DECam, the 570-megapixel CCD camera used for the Dark Energy Survey, at the Cerro Tololo Inter-American Observatory in Chile. (Credit: Reidar Hahn)
The dome of the Blanco Telescope, which houses DECam, the 570-megapixel CCD camera used for the Dark Energy Survey, at the Cerro Tololo Inter-American Observatory in Chile. (Credit: Reidar Hahn)
via simonsfoundation

The lonely landscape of Rosetta’s comet

The lonely landscape of Rosetta's comet
The lonely landscape of Rosetta’s comet – Comet 67P/Churyumov-Gerasimenko from a distance of just 29 kilometers (Credit: ESA)
via abc

Miranda: An icy moon deformed by tidal heating

Mosaic of southern hemisphere of Miranda, the innermost regular satellite of Uranus, with radius of 236 km. Projection is orthographic, centered on the south pole. Visible from left to right are Elsinore, Inverness, and Arden coronae. (Credit: NASA/Jet Propulsion Laboratory/Ted Stryk)
Mosaic of southern hemisphere of Miranda, the innermost regular satellite of Uranus, with radius of 236 km. Projection is orthographic, centered on the south pole. Visible from left to right are Elsinore, Inverness, and Arden coronae. (Credit: NASA/Jet Propulsion Laboratory/Ted Stryk)
via science2.0

Physical constant is constant even in strong gravitational fields

Picture of the laser system with which the hydrogen molecules were investigated on earth. (Credit: LaserLaB VU University Amsterdam/Wim Ubachs)
An international team of physicists has shown that the mass ratio between protons and electrons is the same in weak and in very strong gravitational fields. Pictured above is the laser system with which the hydrogen molecules were investigated on earth. (Credit: LaserLaB VU University Amsterdam/Wim Ubachs)
via phys.org

NASA’s Maven spacecraft will arrive at Mars this weekend

via nypost

Shrink-wrapping spacesuits

The MIT BioSuit, a skintight spacesuit that offers improved mobility and reduced mass compared to modern gas-pressurized spacesuits. (Credit: Jose-Luis Olivares/MIT)
The MIT BioSuit, a skintight spacesuit that offers improved mobility and reduced mass compared to modern gas-pressurized spacesuits. (Credit: Jose-Luis Olivares/MIT)
via mit

Physics in the News

Thursday, September 18, 2014

Have physicists just disproved string theory?

via mysteriousuniverse

New measurements from the AMS experiment unveil new territories in the flux of cosmic rays

Upper plot shows the slope of positron fraction measured by AMS (red circles) and a straight line fit at the highest energies (blue line). The data show that at 275±32 GeV the slope crosses zero. Lower plot shows the measured positron fraction as function of energy as well as the location of the maximum. (Credit CERN)
Upper plot shows the slope of positron fraction measured by AMS (red circles) and a straight line fit at the highest energies (blue line). The data show that at 275±32 GeV the slope crosses zero. Lower plot shows the measured positron fraction as function of energy as well as the location of the maximum. (Credit CERN)
via interactions

Nuclear spins control current in plastic LED: Step toward quantum computing, spintronic memory, better displays

An organic light-emitting diode, or OLED, glows orange when electrical current flows through it. University of Utah physicists used this kind of OLED -- basically a plastic LED instead of a conventional silicon semiconductor LED -- to show that they could read the subatomic 'spins' in the center or nuclei of hydrogen isotopes and use those spins to control current to the OLED. It is a step toward 'spintronic' devices such as faster computers, better data storage and more efficient OLEDs for TV, computer and cell phone displays. (Credit: Andy Brimhall, University of Utah)
An organic light-emitting diode, or OLED, glows orange when electrical current flows through it. It is a step toward ‘spintronic’ devices such as faster computers, better data storage and more efficient OLEDs for TV, computer and cell phone displays. (Credit: Andy Brimhall, University of Utah)
via phys.org

New technology that guides light through glass, developed by researchers from Polytechnique Montréal, could make our smartphones even smarter (PDF)

his revolutionary work could open up new real estate in the phone by embedding the glass with layer upon layer of sensors, including ones that could take your temperature, assess your blood sugar levels if you're diabetic or even analyze DNA.
This revolutionary work could open up new real estate in the phone by embedding the glass with layer upon layer of sensors, including ones that could take your temperature, assess your blood sugar levels if you’re diabetic or even analyze DNA. (Credit: Jerome Lapointe, Mathieu Gagné, Ming-Jun Li, and Raman Kashyap)
via mediacastermagazine

Milky Way mysteries mapped

The NASA/ESA Hubble Space Telescope has produced this finely detailed image of the beautiful spiral galaxy NGC 6384. This galaxy lies in the constellation of Ophiuchus (The Serpent Bearer), not far from the centre of the Milky Way on the sky. The positioning of NGC 6384 means that we have to peer at it past many dazzling foreground Milky Way stars that are scattered across this image. In 1971, one member of NGC 6384 stood out against these bright foreground stars when one of its stars exploded as a supernova. This was a Type Ia supernova, which occurs when a compact star that has ceased fusion in its core, called a white dwarf, increases its mass beyond a critical limit by gobbling up matter from a companion star. A runaway nuclear explosion then makes the star suddenly as bright as a whole galaxy. While many stars have already come to the ends of their lives in NGC 6384, in the centre, star formation is being fuelled by the galaxy’s bar structure; astronomers think such galactic bars funnel gas inwards, where it accumulates to form new stars. This picture was created from images take with the Wide Field Channel of Hubble’s Advanced Camera for Surveys. An image taken through a blue filter (F435W, coloured blue) was combined with an image taken through a near-infrared filter (F814W, coloured red). The total exposure times were 1050 s through each filter and the field of view is about 3 x 1.5 arcminutes. (Credit NASA)
The NASA/ESA Hubble Space Telescope has produced this finely detailed image of the beautiful spiral galaxy NGC 6384. This galaxy lies in the constellation of Ophiuchus (The Serpent Bearer), not far from the centre of the Milky Way on the sky. The positioning of NGC 6384 means that we have to peer at it past many dazzling foreground Milky Way stars that are scattered across this image. (Credit NASA/ESA)
via nationalgeographic

Very large telescope findings could force physicists to rethink the Big Bang

he problem was first identified some time ago. Dubbed the “cosmological lithium discrepancy,” the issue is very simple: everything we know about the Big Bang, supernovae, and the dynamics of stars, tells us that we should find a very specific concentration of lithium in the universe at large — but the universe actually seems to contain far less than that amount. (Credit: NASA, HUbble)
via geek.com

Asteroid tracking program has only 10 percent chance of success

European Space Agency's Giotto probe returned 2333 images during the Comet Halley encounter of March 13-14, 1986. All were recorded before the closest approach of 596 km at 00:03:02 UTC on 14 March 1986; the last from a distance of 1180 km, 15 seconds before closest approach. (Credit: MPAE, Dr H.U. Keller.
European Space Agency’s Giotto probe returned 2333 images during the Comet Halley encounter of March 13-14, 1986. All were recorded before the closest approach of 596 km at 00:03:02 UTC on 14 March 1986; the last from a distance of 1180 km, 15 seconds before closest approach. (Credit: MPAE, Dr H.U. Keller.
via inquisitr

Mystery U.S. government satellite is now in orbit

av_clio_l3917201432422AM63-1552x1940
An Atlas V rocket lifts off with the mysterious CLIO satellite. The rocket was carrying a satellite known only as CLIO, which it delivered into an unidentified (though probably geosynchronous) orbit. (Credit: ULA)
via forbes

Physics team uses pixel sensitivity of smartphone as a random generator for encryption

Random number generator setup: a camera is fully and homogeneously illuminated by a LED. The raw binary representation of pixel values are concatenated and passed through a randomness extractor. This extractor outputs quantum random numbers. (Credit: arXiv:1405.0435 [quant-ph])
Random number generator setup: a camera is fully and homogeneously illuminated by a LED. The raw binary representation of pixel values are concatenated and passed through a randomness extractor. This extractor outputs quantum random numbers. (Credit: arXiv:1405.0435 [quant-ph])
via phys.org

What is the Universe? Physics has some mind-bending answers

Science says the universe could be a hologram, a computer program, a black hole or a bubble—and there are ways to check (NASA, ESA, SAO, CXC, JPL-Caltech, and STScI)
Science says the universe could be a hologram, a computer program, a black hole or a bubble—and there are ways to check. (Credit: NASA, ESA, SAO, CXC, JPL-Caltech, and STScI)
via smithsonianmag