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

 

 

 

The Leonids are here

Leonid Meteor Shower Peaks Tonight: How to See It

The Leonids are a prolific meteor shower associated with the comet Tempel-Tuttle. The Leonids get their name from the location of their radiant in the constellation Leo: the meteors appear to radiate from that point in the sky. (Credit: Wiki)

The November path of the radiant of the 2014 Leonids. Credit: Starry Night Education Software.
The November path of the radiant of the 2014 Leonids. Credit: Starry Night Education Software.

The Leonid meteor shower is forecasted to peak Monday afternoon (Nov. 17) in the U.S. eastern time zone, so stargazers in the United States are advised to look to the skies between midnight and dawn on Monday and Tuesday morning for the best view, astronomers say.  This year, the Leonid meteor shower should treat skywatchers to beween 10 and 15 meteors per hour, NASA meteor expert Bill Cook, head of the Meteoroid Environment Office at the agency’s Marshall Space Flight Center in Huntsville, Alabama, told Space.com. For some meteor showers, that’s considered a decent rate.

Leonids Radiant Star Chart(PDF)

right
(Credit: freecharts.com)

NASA’s live stream will include a sky view from a telescope at Marshall Space Flight Center in Alabama. That stream will begin on Monday, Nov. 17 at 7:30 p.m. EST (0030 GMT Tuesday) and will continue until sunrise on Tuesday Nov. 18.

A meteor during the peak of the 2009 Leonid Meteor Shower. The photograph shows the meteor, afterglow, and wake as distinct components.(Credit: Wiki)
A meteor during the peak of the 2009 Leonid Meteor Shower. The photograph shows the meteor, afterglow, and wake as distinct components.(Credit: Wiki)

The Slooh live stream will begin on Monday, Nov. 17 at 8:00 p.m. EST (0100 GMT Tuesday) and will include more than just shots of the sky: Slooh will also broadcast audio of the “ionization sounds” created by the meteors. As the meteors streak through the sky, they briefly ionize the atmosphere. For a few seconds, the ionized region reflects short-wavelength radio waves, creating short blips and beeps of sound. Slooh’s broadcast will also include interviews with astronomers. (Credit: Calla Cofield and Spacce.com)

Skymap November 2014 (PDF)

east
(Credit: Farmers Almanac)

The waning-crescent moon will increase chances of a better view of the spectacle, according to NASA. This type of moon will create skies that are dark enough to view the meteors, which are characteristically bright and colorful.

Leonids Viewing Conditions Photo courtesy of AccuWeather.com
Leonids Viewing Conditions (Credit: AccuWeather.com)

“Widespread cloud cover across the eastern third of the U.S. will make it difficult to see the meteor shower Monday before dawn, except perhaps in central and south Florida. Skies should be much clearer Tuesday morning, though it may take until late at night for New England to clear out, and there will be clouds in south Florida and in the lake-effect snow belts of the Great Lakes. Clear skies will be the rule across the central and western U.S. both mornings, with only a few minor exceptions,” said Digital Meteorologist, Nick Wiltgen, from weather.com. (Credit: Carolyn Williams, weather.com)

This diagram maps the data gathered from 1994-2013 on small asteroids impacting Earth's atmosphere to create very bright meteors, technically called "bolides" and commonly referred to as "fireballs".  Sizes of red dots (daytime impacts) and blue dots (nighttime impacts) are proportional to the optical radiated energy of impacts measured in billions of Joules (GJ) of energy, and show the location of impacts from objects about 1 meter (3 feet) to almost 20 meters (60 feet) in size. Image (Credit: Planetary Science)
This diagram maps the data gathered from 1994-2013 on small asteroids impacting Earth’s atmosphere to create very bright meteors, technically called “bolides” and commonly referred to as “fireballs”. Sizes of red dots (daytime impacts) and blue dots (nighttime impacts) are proportional to the optical radiated energy of impacts measured in billions of Joules (GJ) of energy, and show the location of impacts from objects about 1 meter (3 feet) to almost 20 meters (60 feet) in size. Image (Credit: Planetary Science)
via scientificamerican

Physics in the News

Saturday, October 11, 2014

Leaky galaxies lead researchers to better understand the universe

 This is Sanchayeeta Borthakur, assistant research scientist in the Department of Physics and Astronomy at the Johns Hopkins University. (Photo Credit: JHU)
Sanchayeeta Borthakur, an assistant research scientist in the Department of Physics and Astronomy in the university’s Krieger School of Arts and Sciences, reports in a paper published online Oct. 9 in the journal Science that an indicator used for studying star-forming galaxies that leak radiation is an effective measurement tool for other scientists to use. (Credit: JHU)
via sciencecodex

L.A. Museum Adds the Last Payload to Shuttle Endeavour

141010-shuttle_c92e33917bf64aaa38d9790b47f34c7f.nbcnews-ux-1240-800
During an event titled “Go for Payload,” the California Science Center in Los Angeles hoisted a Spacehab module into the open hold of the retired space shuttle Endeavour. The logistics module’s addition, together with several other real and replica parts, marked a major milestone towards the center’s plans to display the NASA winged orbiter in a vertical, launch-ready configuration. (Pearlman, CollectSpace.com)
via nbcnews

Topological defects in the fabric of space and time

A cosmic string is a very long (possibly as long as the diameter of the visible universe), very thin (less than the width of a proton) high-density object formed during the early moments of the big bang. (Credit: Stae Trek,  Paramount Pictures)
A cosmic string is a very long (possibly as long as the diameter of the visible universe), very thin (less than the width of a proton) high-density object formed during the early moments of the big bang. (Credit: Stae Trek, Paramount Pictures)
via phys.org

The Moon and the Oh-My-God Particle

Close up artist rendition. Image of the Australian SKA LFAA (Low Frequency Aperture Array) instrument. These dipole antenna which will number in their hundreds of thousands will survey the radio sky in frequencies as low at 50Mhz (Credit: SKA Organisation)
Close up artist rendition. Image of the Australian SKA LFAA (Low Frequency Aperture Array) instrument. These dipole antenna which will number in their hundreds of thousands will survey the radio sky in frequencies as low at 50Mhz (Credit: SKA Organisation)
via popularmechanics

On the front lines of the Higgs boson search

Prof. Butterworth, leading physicist on the ATLAS experiment at CERN and head of physics and astronomy at University College London, said the two colliding proton beams at CERN were the highest energy particle beams ever used in a laboratory. In order for the high momentum beams to be bent into a circle, its curvature had to be gentle enough for superconducting magnets to be able to control the beams. (Credit: hep.ucl.ac.uk/~jmb/publications)
Prof. Butterworth, leading physicist on the ATLAS experiment at CERN and head of physics and astronomy at University College London, said the two colliding proton beams at CERN were the highest energy particle beams ever used in a laboratory. (Credit: hep.ucl.ac.uk/~jmb/publications)
via phys.org

Peering backward to the big bang with the CTC and COSMOS

(NASA, Shellard,)
Recent analysis of CMB observations confirm predictions that a period of enormously fast exponential expansion, which cosmologists call inflation, occurred in the early universe. During inflation, very small changes, or quantum fluctuations, were imprinted into the fabric of space-time. (NASA, Shellard,)
via hpcwire

Answers to questions posed by cosmology to philosophy

 the philosophy of cosmology. He commented that the field is not well formulated yet, and proposed that one way to build a sound foundation for the field would be to identify the key questions worthy of its attention. Carroll nominated 10 such questions. Credit: Carroll)
Sean Caroll purposes 10 questions regarding the ‘not well formulated’ Philosophy of Cosmology. (Credit: Carroll)
via sciencenews

Getting sharp images from dull detectors

Coherent light passes through a pair of slits (top center).  The two resulting concentric trains of waves will interfere, resulting in a fixed pattern when measured by a detector (top right).  Non-coherent thermal light passes through slits and meets with a beam splitter (green plane), which reflects half the waves toward one detector and the other half toward a second detector (lower left).  Each of the detectors records a temporary interference pattern (lower right).  (Credit: JQI/Kelley )
Coherent light passes through a pair of slits (top center). The two resulting concentric trains of waves will interfere, resulting in a fixed pattern when measured by a detector (top right). Non-coherent thermal light passes through slits and meets with a beam splitter (green plane), which reflects half the waves toward one detector and the other half toward a second detector (lower left). Each of the detectors records a temporary interference pattern (lower right). (Credit: JQI/Kelley )
via umd

NASA: More spacewalks for ISS crew

via floridatoday

This Week’s Sky at a Glance, October 10 – 18

The waning Moon and Orion tip to the southwest as dawn brightens. (The Moon in these scenes is always shown three times its actual apparent size.. (Credit: Sky and Telescope)
The waning Moon and Orion tip to the southwest as dawn brightens. (The Moon in these scenes is always shown three times its actual apparent size.. (Credit: Sky and Telescope)
via skyandtelescope

Physics in the News

Wednesday, October 8, 2014

NuSTAR telescope discovers shockingly bright dead star

Astronomers have found a pulsating dead star beaming with the energy of about 10 million Suns, which is the brightest pulsar ever recorded..  A rare and mighty pulsar (pink) can be seen at the center of galaxy M82 in this new multi-wavelength portrait. NASA's NuSTAR mission discovered the "pulse" of the pulsar — a type of dead star — using is high-energy X-ray vision.
Astronomers have found a pulsating dead star beaming with the energy of about 10 million Suns, which is the brightest pulsar ever recorded.. A rare and mighty pulsar (pink) can be seen at the center of galaxy M82 in this new multi-wavelength portrait. NASA’s NuSTAR mission discovered the “pulse” of the pulsar — a type of dead star — using is high-energy X-ray vision.
via astronomy

Hypothetical new cosmological model known as Higgsogenesis (PDF)

The term Higgsogenesis refers to the first appearance of Higgs particles in the early universe, just as baryogenesis refers to the appearance of baryons (protons and neutrons) in the early moments after the big bang. While baryogenesis is a fairly well understood process, Higgsogenesis is still very hypothetical. (Credit: CERN/Lucas Taylor, Koberlein)
The term Higgsogenesis refers to the first appearance of Higgs particles in the early universe, just as baryogenesis refers to the appearance of baryons (protons and neutrons) in the early moments after the big bang. While baryogenesis is a fairly well understood process, Higgsogenesis is still very hypothetical. (Credit: CERN/Lucas Taylor, Koberlein)
via phys.org

Dark matter half what we thought, say scientists (PDF)

A new measurement of dark matter in the Milky Way has revealed there is half as much of the mysterious substance as previously thought.  The above is an artist's impression of the Milky Way and its dark matter halo (shown in blue, but in reality invisible). Credit: ESO/L. Calçada
A new measurement of dark matter in the Milky Way has revealed there is half as much of the mysterious substance as previously thought. The above is an artist’s impression of the Milky Way and its dark matter halo (shown in blue, but in reality invisible). (Credit: ESO/L. Calçada)
via sciencedaily

Astronomers see right into heart of exploding star

 (Credit: Bill Saxton, NRAO/AUI/NSF)
An international team of astronomers has been able to see into the heart of an exploding star, by combining data from telescopes that are hundreds or even thousands of kilometres apart. (Credit: Bill Saxton, NRAO/AUI/NSF)
via manchester

Among the artian hills: Curiosity Rover peers at rocks of Mount Sharp

After a couple of years of racing towards Mount Sharp (Aeolis Mons), now it’s time for the Curiosity rover to get a better look at its Martian surroundings. Rover tracks and Martian sand as seen from the rear hazcam of NASA’s Curiosity rover. (Credit: NASA/JPL-Caltech)
After a couple of years of racing towards Mount Sharp (Aeolis Mons), now it’s time for the Curiosity rover to get a better look at its Martian surroundings. Rover tracks and Martian sand as seen from the rear hazcam of NASA’s Curiosity rover. (Credit: NASA/JPL-Caltech)
via universetoday

Two new strange and charming particles appear at LHC

Two new particles have been discovered by the LHCb experiment at CERN's Large Hadron Collider near Geneva, Switzerland. One of them has a combination of properties that has never been observed before. : Dave Stock)
Two new particles have been discovered by the LHCb experiment at CERN’s Large Hadron Collider near Geneva, Switzerland. One of them has a combination of properties that has never been observed before. (Credit: Dave Stock)
via newscientist

 The cosmic signal that might have changed human civilization

The image above shows a graphic which was produced by the SETI from the data of the Wow signal. A signal (Gaussian, triplet or pulse) arises only in a single narrowband channel. All other channels contain noise. Up to now we do not know cosmic phenomena which would generate such signals. It would seem improbable that they have no artificial origin. The picture shows a computer generated example of a strong Gaussian signal.
The image above shows a graphic which was produced by the SETI from the data of the Wow signal. A signal (Gaussian, triplet or pulse) arises only in a single narrowband channel. All other channels contain noise. Up to now we do not know cosmic phenomena which would generate such signals. It would seem improbable that they have no artificial origin. The picture shows a computer generated example of a strong Gaussian signal.
via dailygalaxy

World’s longest neutrino beam will explore why the universe still exists

This quirk of subatomics could have huge implications for our understanding of the universe, specifically how the current inequality between matter and antimatter came to be. Answering that could, in turn, provide a better insight as to why reality did not simply blink out of existence immediately after the Big Bang as a universe's worth of matter and antimatter negated one another's existences (
This quirk of subatomics could have huge implications for our understanding of the universe, specifically how the current inequality between matter and antimatter came to be. Answering that could, in turn, provide a better insight as to why reality did not simply blink out of existence immediately after the Big Bang as a universe’s worth of matter and antimatter negated one another’s existences (Credit: Tarantola, Fermilab, )
via gizmodo

What a difference a  neutron makes

For the first time, scientists have demonstrated that modified hydrogen bonding is sufficient to switch solid-state electronic properties. (Credit: University of Tokyo. ,Tan)
For the first time, scientists have demonstrated that modified hydrogen bonding is sufficient to switch solid-state electronic properties. (Credit: University of Tokyo. ,Tan)
via asianscientist

 

Physics in the News

Wednesday, October 8, 2014

UW fusion reactor concept could be cheaper than coal

The UW’s current fusion experiment, HIT-SI3. It is about one-tenth the size of the power-producing dynomak concept. (Credit: U of Washington)
The UW’s current fusion experiment, HIT-SI3. It is about one-tenth the size of the power-producing dynomak concept. (Credit: U of Washington)
via washington.edu

Researchers achieve quantum teleporting

via azoquantum

Tipping the spherical cow: The initial conditions of star formation

Gas column density 5 Myr after stars begin forming in the “real” Clouds (left panels) and corresponding Spheres (right panels). The Spheres begin forming stars 5-6 Myr after t=0, so the figure shows simulations at a similar stage of star formation. Clouds show more widespread star formation, and alignment of their major gas filaments along the larger-scale structures present in the galaxy. Part of Figure 2 from Rey-Raposo, Dobbs & Duarte-Cabral 2014.
Gas column density 5 Myr after stars begin forming in the “real” Clouds (left panels) and corresponding Spheres (right panels). The Spheres begin forming stars 5-6 Myr after t=0, so the figure shows simulations at a similar stage of star formation. Clouds show more widespread star formation, and alignment of their major gas filaments along the larger-scale structures present in the galaxy. (Credit: Rey-Raposo, Dobbs & Duarte-Cabral 2014)
via astrobites

Breakthrough allows researchers to watch molecules “wiggle”

Difference electron density maps showing the comparison of control and HATRX data for thaumatin. (Credit: University of Leeds)
via rdmag

Monster galaxies resort to cannibalism to keep growing

Larger galaxies are unable to create new stars at a rapid enough pace so they start to “eat” stars in neighboring galaxies. (Photo By Nasa/Getty Images)
Larger galaxies are unable to create new stars at a rapid enough pace so they start to “eat” stars in neighboring galaxies. (Photo By Nasa/Getty Images)
via cbs

Aliens may be too distant for contact

The SETI Institute's Allen Telescope Array (ATA) is hunting for radio signals from hypothetical intelligent alien life in our galaxy. (Credit: SETI) Institute
The SETI Institute’s Allen Telescope Array (ATA) is hunting for radio signals from hypothetical intelligent alien life in our galaxy. (Credit: SETI) Institute
via aninews

How NASA plans to utilize lasers in order to draw 3D maps of the earth’s forests

NASA has a new project underway called GEDI. The sole purpose of GEDI is to point a laser-based device at Earth from the International Space Station in order to map out forests in 3D, eventually determining the amount of carbon in Earth’s forests. (Credit: NASA's Goddard Space)
NASA has a new project underway called GEDI. The sole purpose of GEDI is to point a laser-based device at Earth from the International Space Station in order to map out forests in 3D, eventually determining the amount of carbon in Earth’s forests. (Credit: NASA’s Goddard Space)
via industrytap

Sierra Nevada protest halts production of SpaceX and Boeing space taxis

 The Wait For Space A look through the open hatch of SpaceX's Dragon V2 capsule, one of two designs chosen for NASA's Commercial Crew Transportation Capability program. Both Boeing and SpaceX have been told to halt production of their space taxi designs until a protest filed by the Sierra Nevada Corporation has been resolved. (Credit: NASA)
A look through the open hatch of SpaceX’s Dragon V2 capsule, one of two designs chosen for NASA’s Commercial Crew Transportation Capability program. Both Boeing and SpaceX have been told to halt production of their space taxi designs until a protest filed by the Sierra Nevada Corporation has been resolved. (Credit: NASA)
via popsci

Three win Nobel for super-zoom microscopes

German winner of the Nobel Prize for chemistry Stefan Hell gestures at a small party with his colleagues in Goettingen, Germany, Wednesday, Oct. 8, 2014. Hell shares the prize with Americans Eric Betzig and William E. Moerner for developing ways to dramatically improve the resolution of optical microscopes. Hell developed the underlying technology for R&D 100 Awards-winning super-resolution microscopes from Leica. (Credit AP/dpa, Swen Pfoertner)
German winner of the Nobel Prize for chemistry Stefan Hell gestures at a small party with his colleagues in Goettingen, Germany, Wednesday, Oct. 8, 2014. Hell shares the prize with Americans Eric Betzig and William E. Moerner for developing ways to dramatically improve the resolution of optical microscopes. Hell developed the underlying technology for R&D 100 Awards-winning super-resolution microscopes from Leica. (Credit AP/dpa, Swen Pfoertner)
via rdmag

Newly discovered letter gives a rare glimpse into Einstein’s personal views on life

he Einstein Papers Project, a group of scholars devoted to collecting and transcribing Einstein’s works and publishing The Collected Papers of Albert Einstein both online and in printed format, have collected thousands of Einstein’s letters, both those from him and to him. But this exchange is new. (Credit: The Telegraph)
The Einstein Papers Project, a group of scholars devoted to collecting and transcribing Einstein’s works and publishing The Collected Papers of Albert Einstein both online and in printed format, have collected thousands of Einstein’s letters, both those from him and to him. But this exchange is new. (Credit: The Telegraph)
via inquisitr