The Large Hadron Collider has begun circulating protons through its full circumference, a significant milestone in the field of particle physics. The event was celebrated with a pajama party at Fermilab's Remote Operations Center, where researchers and engineers gathered to mark the occasion.
The University of Utah is joining the third Sloan Digital Sky Survey to map distant galaxies, understand galaxy evolution, and discover planets with suitable environments for life. The survey will also help scientists test theories about dark energy and explore the mysteries of the universe.
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Researchers at Carnegie Institution find unusual new form of carbon in meteorites, which could affect measurements of the universe's expansion and dark energy models. The discovery may have implications for understanding Type1a supernovae and the accelerating expansion of the universe.
Astronomers have measured the distribution and motions of thousands of galaxies in the distant Universe using ESO's VLT. This study provides a powerful way to tackle the mystery of dark energy, with results supporting the simplest form of dark energy.
The Hubble Space Telescope has discovered a double Einstein ring, caused by the bending of light from two distant galaxies behind a massive foreground galaxy. The discovery offers insights into dark matter and the nature of distant galaxies.
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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.
Three quarters of the universe is dark energy, a mysterious substance that repels gravity. New space missions and improved observation methods will help uncover its secrets.
The National Research Council recommends pursuing the Joint Dark Energy Mission as the first mission in the 'Beyond Einstein' program, which aims to study dark energy. The report also suggests investing additional funds in technology development of the Laser Interferometer Space Antenna (LISA) program.
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.
Astronomers found a gigantic hole in the Universe, spanning nearly a billion light-years, empty of stars, galaxies, gas, and dark matter. The void's existence was confirmed by studying data from the NRAO VLA Sky Survey, which revealed a significant drop in galaxy count in a region southwest of Orion.
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A paper by Lawrence Krauss and Robert Scherrer suggests that matter will dominate over radiation in an ever-expanding universe dominated by dark energy. This means that ordinary matter particles, such as protons and neutrons, will remain stable for trillions of years, potentially allowing life to endure forever.
The South Pole Telescope has achieved its first light, successfully collecting test observations and paving the way for cosmological research. The $19.2 million telescope is designed to pierce the mystery of dark energy, which drives the universe's evolution.
Researchers at Ohio State University have discovered a new high-energy state in DNA that helps dissipate UV energy. The 'dark state', which can last for 10-150 picoseconds, is found in single nucleotides and dissolves energy through 10-50% of the time. This discovery may provide insights into DNA damage and repair mechanisms.
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The University of Chicago's Center for Astrophysical Thermonuclear Flashes will perform the world's most advanced simulations of exploding white dwarf stars using 2.5 million hours of processing time. The goal is to understand the nature of dark energy, a mysterious force dominating the universe.
Researchers using NASA's Hubble Space Telescope found dark energy was present and accelerating the universe's expansion at least 9 billion years ago. This discovery provides a crucial clue to understanding dark energy's strength and permanence.
The International Astronomical Union has elected Catherine Cesarsky as its new president, effective for the next three years. The IAU will play a key role in promoting astronomy globally, especially during the proposed International Year of Astronomy in 2009.
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.
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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.
Astrophysicist Saul Perlmutter wins prestigious International Feltrinelli Prize for his groundbreaking research on dark energy and the accelerating expansion of the universe. The prize recognizes Perlmutter's contributions to our understanding of the universe's mysterious force, dark energy.
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.
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.
A team of researchers discovered that dark energy behaves similarly to Einstein's cosmological constant with a precision of 10%, contradicting several theoretical predictions. The study uses innovative camera technology and observations from multiple telescopes worldwide.
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Physicists Eric Linder and Robert Caldwell separate dark energy scenarios through satellite searches, offering a way to distinguish among dark energy possibilities. The Joint Dark Energy Mission experiments may be able to determine which scenario is correct.
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.
Cosmologists propose that the universe's acceleration can be explained by inflationary theory, which generates cosmic ripples that drive expansion. This solution relies on Einstein's General Relativity and doesn't require new ingredients like dark energy.
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A team of researchers has found evidence of dark energy in the universe's cosmic neighborhood, with billions of galaxies emerging from a sea of dark energy. The findings provide supporting evidence for the presence of dark energy, which is causing the universe to accelerate in expansion.
University of Pennsylvania astrophysicist Licia Verde outlines a multi-disciplinary approach to studying dark energy. The investigation draws on data from galaxy surveys, supernovae, and the Cosmic Microwave Background, providing clues about this enigmatic component.
Dark energy drives universe expansion, but its effects are complex and not fully understood. String theory offers a potential explanation, suggesting the existence of 'pocket universes' with distinct physical laws.
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Researchers are exploring alternative explanations for dark energy, including the possibility of modified gravity laws and a multiverse. String theory suggests that the value of the cosmological constant may be very small, while another speaker proposes using
Dvali suggests extra dimensions allow gravitons to escape, altering space-time continuum and accelerating cosmic expansion. This theory predicts observable deviations at shorter distances than predicted by modified gravity hypothesis.
Researchers propose a new theory linking neutrinos' slight mass to the accelerating universe expansion through dark energy and accelerons. The theory suggests that neutrinos interact with accelerons, resulting in a force that fuels the expansion of the universe.
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Theoretical physicist Robert J. Scherrer proposes a model that explains dark matter and dark energy as two sides of the same coin, using an exotic form of energy called scalar fields. This unifying idea avoids previous problems and could potentially explain the mysterious phenomena.
The American Association for the Advancement of Science names WMAP satellite and Sloan Digital Sky Survey as key discoveries confirming a dark, expanding universe dominated by 73% dark energy. Scientists also identified genes increasing mental illness risk and reported global warming impacts.
A new study analyzing Type 1A supernovae measured with the Hubble Space Telescope sheds light on the nature of dark energy. The results confirm that the universe is expanding at an increasing rate, reinforcing initial discoveries made five years ago.
The study confirms the accelerating expansion of the universe due to dark energy, with data from 11 distant supernovae. It provides more precise measures of matter and dark energy composition in the universe.
Researchers conclude dark energy is the dominant form of energy in the universe, contradicting observations of distant supernovae. The accelerating expansion of the universe can be explained by the presence of negative pressure in a vacuum, supporting the existence of dark energy.
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Cosmologists suggest universe may collapse in 10-20 billion years due to dark energy, reversing the popular view of a runaway universe. The Stanford team's model predicts the universe will slow down and contract, leading to a cosmic 'big crunch',
Researchers using galaxy cluster surveys can measure the equation of state of dark energy, which would provide clues about its nature and origin. By studying scaling relations and X-ray emission, scientists hope to determine the essence of dark energy.
The universe consists mostly of mysterious dark matter and dark energy, which make up 95% of its mass. Ordinary matter accounts for only 5%, a finding confirmed by observations of the cosmic microwave background.
Researchers use 'Cosmic Triangle' to plot evidence for accelerated universe expansion and high mass density of dark energy. The findings rule out models with low or negative mass density, pointing towards a flat universe dominated by dark energy.
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