Physicist John Negele will discuss how quarks and gluons interact using lattice field theory on supercomputers. The tiny particles behave differently than larger particles, requiring a unique approach to study them.
The Atacama Large Millimeter/submillimeter Array (ALMA) will provide astronomers with unprecedented views of the origins of stars, galaxies, and planets. ALMA's high-resolution capabilities will enable scientists to unravel longstanding mysteries in astronomy.
The American Institute of Physics awarded prizes to four winners for their outstanding science writing. Quantum mechanics expert Tim Folger won for his article on the effect of gravity on a speck of dust, while physicist James Trefil received an award for explaining dark matter and dark energy in the universe's future.
For the first time, astronomers have directly visualized the distribution of dark matter in a supercluster, allowing for the detection of irregular clumps and detailed shapes. This breakthrough study, led by UBC researcher Catherine Heymans, uses NASA's Hubble Space Telescope to map the Abell 901/902 supercluster.
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Researchers used supercomputing power to simulate the early Universe and identify potential methods for measuring dark energy. The study's findings will help design a proposed satellite mission called SPACE, which aims to unveil the nature of dark energy and its role in the Universe's accelerating expansion.
The GLAST satellite, a gamma-ray telescope, has arrived at the Naval Research Laboratory in Washington for testing before its launch later in 2008. The mission will study extreme environments in the universe, identifying unknown sources of gamma rays.
The Gamma-ray Large Area Space Telescope (GLAST) spacecraft has successfully completed two environmental tests and is now undergoing thermal and vacuum testing at the Naval Research Laboratory. The satellite will study extreme universe phenomena, including black holes and gamma-ray bursts.
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A team of UWM researchers is analyzing data from the Laser Interferometer Gravitational-wave Observatory, searching for signs of Einstein's predicted gravitational waves. The team is using advanced computational power to sort through massive amounts of data generated by LIGO facilities.
Researchers find liquid-like behavior in granular particles bouncing off a target, similar to quark-gluon plasma experiments. The discovery provides insight into phenomena beyond equilibrium states, revealing classical concepts influencing quantum-scale events.
Researchers at University of Bonn use computer simulations to understand how star clusters are formed from interstellar gas clouds and evolve over time. The study finds that small clusters are easily destroyed by radiation from stars, while heavy clusters survive longer.
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Cosmology@Home allows people worldwide to participate in cutting-edge cosmology research by donating their unused computing cycles. Participating computers calculate the observable predictions of millions of theoretical models with different parameters, which are then compared with actual data.
Astronomers have detected a huge burst of radio energy from the distant universe, suggesting a new area of study in astrophysics. The burst was so bright that it saturated equipment and could be equivalent to a large power station running for two billion years.
A groundbreaking study reveals that the first stars formed at the start of the Universe depend on dark matter's nature. The research suggests that some of these primordial stars can still be found in the Milky Way galaxy today.
The discovery of geologic time revolutionized our understanding of the world, allowing scientists to date rocks and calculate the age of the Earth. This breakthrough, achieved by Arthur Holmes in the early 20th century, had a profound impact on fields like plate tectonics and evolution.
The National Research Council recommends the Joint Dark Energy Mission, supported by NASA and DOE, to study dark energy's role in the universe's expansion. The mission aims to map the sky with unprecedented resolution and study Type Ia supernovae to shed light on this mysterious entity.
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Researchers from the Weizmann Institute of Science have observed a rare and detailed view of a Type Ia supernova event, revealing the remnants of a red giant star that fed a white dwarf. This unique observation supports a widely accepted model of these explosions.
A new study using Chandra finds that younger, more distant galaxy clusters contain far more actively growing supermassive black holes than older, nearby ones. This rapid growth allows these black holes to thrive and influence their host galaxies.
Researchers discovered clear changes in interstellar material absorption, indicating the existence of gaseous shells around a white dwarf. The system was likely composed of a white dwarf feeding on its red giant companion, leading to the supernova explosion. This finding strongly supports the Type Ia supernova scenario.
The GLAST team is testing the satellite in a 'clean room' to prevent contamination due to dust and humidity. The clean environment ensures the sensitive instruments are protected during development, construction, and testing.
The ATLAS upgrade, called CARIBU, will enable researchers to accelerate beams of short-lived radioactive isotopes and study unstable nuclei. This will help scientists better understand the universe's heavy elements, including those created in supernovae explosions.
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A MU physicist argues that the Lunar Laser Ranging (LLR) technique is not effective in measuring the gravitomagnetic field. The LLR method relies on processing data with two sets of mathematical equations, but it can introduce errors due to gauge freedom and insufficient analytic control.
The new VERITAS telescope array will enable the detection of an increased number of gamma ray sources, potentially including indirect dark matter detection. The instrument's sensitive instrumentation has an energy threshold of about 100 GeV and can identify sources with an intensity of about 1 photon per minute.
Art McDonald and his SNO team have won the Benjamin Franklin Medal in Physics for their discovery that neutrinos change flavour and have mass, modifying the Standard Model of particle physics. The award recognizes their outstanding scientific achievement in understanding the nature of matter and the universe.
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Researchers have developed a new method for testing the reliability of tests, improving the accuracy of risk estimates and enabling better product quality control. The new approach takes into account the severity of errors, providing a more realistic measure of reliability.
Astrophysicists at the University of Illinois propose a new method to measure the fine-structure constant using relic radiation from the birth of the universe. This technique could help explain dark energy and constrain a
Richard Bond, a renowned cosmologist at the University of Toronto, has won the Gerhard Herzberg Canada Gold Medal for Science and Engineering. His research has provided crucial insights into the universe's current structure, shedding light on dark matter and its role in shaping the cosmos.
Physicists Xiao-Gang Wen and Michael Levin propose a new state of matter where electrons are entangled in string-nets. Their model predicts the emergence of conventional particles and fractionally charged quasiparticles, which behave according to Maxwell's equations.
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Physicist Burton Richter says new experiments will answer some questions but raise others about the universe's composition and expansion. He emphasizes the need for prioritizing crucial research to advance our understanding of dark matter, dark energy, and the Standard Model.
Researchers propose explanation for formation of dwarf spheroidals, faint galaxies composed almost entirely of dark matter. Simulations suggest environmental effects, including ram pressure and tidal shocking, strip away luminous matter, leaving behind dark-matter shadow.
Researchers at University of Wisconsin-Madison devise approach to 'see' extra dimensions by deciphering cosmic energy released in the universe's violent birth. The method provides evidence for testing string theory's existence and predicts specific shapes for the six hidden dimensions.
Scientists at Max Planck Institute for Astrophysics have discovered a way to make a picture of everything that gravitates in the Universe using radio telescopes. By analyzing radio waves emitted from the early Universe, they can create high-resolution images of cosmic mass distribution, surpassing current galaxy distortions.
A RAND Corporation study suggests the US should focus on undermining support for Islamic terrorism within Muslim nations to defeat the global jihadist movement. The report emphasizes the importance of attacking the ideology's core principles and severing links between terrorist groups.
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Fermilab will continue to provide opportunities for discovery in particle physics with the Tevatron and neutrino experiments. The new management structure brings together scientific leadership and management experience of the University of Chicago and URA.
Astrophysicists have resolved a long-standing issue with the Big Bang theory by studying gas movements in stars. Computer models revealed that low mass stars destroy helium 3 before it can be released into space, resolving the discrepancy.
Researchers created a mathematical code that describes how low-mass stars destroy helium-3 during evolution. This process resolves the discrepancy between helium-3 abundance and the Big Bang theory, providing insights into the universe's early stages.
A University of Southern California-led research group used X-ray crystallography to study the struggle between LTag, a cancer-causing protein, and p53, a key tumor suppressor. The study found that LTag inhibits p53's role by tying up six molecules, but p53 fights back by preventing virus replication.
Astronomers have discovered the faintest stars in a globular star cluster using Hubble's Advanced Camera for Surveys. The study reveals insights into the age, origin, and evolution of NGC 6397, which is estimated to be nearly 12 billion years old.
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The COBE experiments confirmed the universe was born in a big bang, shedding light on its structure. Variations in the CMB revealed tiny but regular temperature fluctuations that exist everywhere in the cosmos.
SNAP, a NASA-supported mission, aims to measure the expansion history of the universe and investigate dark energy. Using two independent techniques, it will analyze thousands of Type Ia supernovae and independently probe the growth structure of the universe.
Researchers at Ohio State University have discovered a new method for calculating intergalactic distances, which implies that the Hubble constant may be significantly off the mark. The Triangulum Galaxy is estimated to be 15% farther away from our galaxy than previously measured, potentially making the universe 15% bigger and older.
The CERN Council has adopted a European strategy for particle physics, providing for European engagement and leadership. This marks an important step for the field, as the world's particle physicists embark on a new adventure with the Large Hadron Collider project.
Researchers used a supercomputer to calculate interactions among neutrons and protons from quark and gluon properties, providing insight into how nuclear forces emerge. This breakthrough paves the way for understanding how finely tuned the universe is and could reveal essential information about carbon-based life.
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Saul Perlmutter, Adam Riess, and Brian Schmidt share the prize for their work on measuring changes in the universe's expansion rate. Their discovery has implications for understanding dark energy and its impact on galaxy distances.
Adam Riess, a 36-year-old astronomer at Johns Hopkins University, has won the $1 million Shaw Prize for his work on dark energy, a phenomenon that accounts for 70 percent of the universe. He shares the award with Saul Perlmutter and Brian Schmidt, who worked on competing teams to measure the expansion rate of the universe.
New X-ray data from Chandra reveals that magnetic fields are responsible for the prodigious amounts of radiation emitted by super-massive black holes. The discovery uses a scale model in our galaxy to understand how all black holes work, including those powering quasars.
Researchers at JILA improved molecular measurement precision, enabling tests of the fine structure constant's evolution over time. This could reveal changes in the strength of electromagnetic interactions.
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Researchers have discovered the Universe's strongest magnetic field, generated by violent collisions between neutron stars. The discovery sheds light on the mysterious short Gamma-ray bursts, which are the most powerful explosions in the universe. Scientists believe that strong magnetic fields play a crucial role in their formation.
Scientists have new evidence for the 'inflation' scenario that describes the universe's sudden growth from submicroscopic to astronomical size in its first trillionth of a second. The WMAP satellite data show a faint polarization signal, which was weaker than expected, but still supports the inflation prediction.
A study using hundreds of images from two deep sky surveys found that more than half of the largest galaxies in the nearby universe have collided and merged with another galaxy. The mergers occur quickly, leaving faint features difficult to detect, but confirm predictions for large-scale structure formation. Ongoing study will reveal i...
Researchers confirm that Einstein's cosmological constant behaves like dark energy, driving the acceleration of the universe. The study uses innovative imaging data from the Supernova Legacy Survey, which reveals a precision of 10% and challenges theoretical ideas about dark energy.
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Florida State University research physicist Edmund G. Myers is using a state-of-the-art Penning trap to measure the precise difference in mass of tritium and helium-3 atoms, which will help pin down the mass of the electron neutrino.
Physicists Andreas Karch and Lisa Randall propose that the relaxation principle in the early universe led to the formation of three- or seven-dimensional realities. These dimensions could be hidden from our perception, with our three-dimensional reality being just one of them.
A team of scientists led by Alan E.E. Rogers successfully detected deuterium using a radio telescope array, a significant breakthrough in understanding the universe's origins. The detection has implications for understanding dark matter and cosmic baryon density.
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A recent study by NASA's Chandra X-ray Observatory suggests that the sun contains nearly three times more neon than previously believed. This discovery has solved a critical problem with understanding how the sun works. The increased amount of neon plays a crucial role in energy flow from nuclear reactions to space.
A study suggests that abandoning livestock can significantly reduce global warming, with animal agriculture emitting 21% of all human-caused carbon dioxide. This shift in diet would have no adverse effects on health and could potentially meet Kyoto treaty targets for reducing emissions.
The American Association for the Advancement of Science has identified 125 major questions that scientists have yet to answer, including the nature of dark matter and the biological basis of consciousness. The journal's special issue marks its 125th anniversary and explores these fundamental gaps in scientific knowledge.
Scientists at Ohio State University discovered that bumpy surfaces on interstellar dust grains can explain the formation of molecular hydrogen, the most abundant element in the universe. By simulating different surfaces, researchers found that only bumpy textures enable two hydrogen atoms to bond in space.
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Researchers improve measurement of Casimir force, influencing small objects more than gravity, with implications for nanotechnologists. The study confirms gravity behaves as expected, ruling out exceptions to Newton's theories.
Researchers using the DEEP2 Galaxy Redshift Survey observe a fundamental constant unchanged over 7 billion years. The fine structure constant affects atomic interactions and light emission, with no variation detected in distant galaxies.
Research by Dr. Michael Murphy suggests that the fine structure constant, governing electromagnetic forces, may have changed over time by about one part in two-hundred-thousand during the last 10 billion years. This finding challenges existing knowledge and could have significant implications for our understanding of the universe.