19 themes/skins available for your browsing pleasure. A variety of looks, 6 AC2 exclusives - Featuring SMACX, Civ6 Firaxis, and two CivII themes.[new Theme Select Box, bottom right sidebar - works for lurkers, too]
0 Members and 1 Guest are viewing this topic.
Physicists Debate Discovery of Gravitational Ripples from the Big BangSPACE.comBy Tanya Lewis, Staff Writer 5 hours agoThis artist's illustration depicts the creation of gravitational waves from two orbiting black holes as ripples in space-time. In March 2014, astronomers announced the first detection of long-sought gravitational wavesNEW YORK – The physics world was agog in March over the announcement that astronomers had possibly found ripples in space-time from the earliest moments of the universe. But some scientists now question whether the findings may be nothing more than galactic dust.If the finding of these ripples, or primordial gravitational waves, is confirmed, it would represent the best evidence yet for inflation, the idea that the universe underwent an explosive burst in size in the earliest fractions of a second after the Big Bang. If the findings are discounted, inflation could still be correct, but scientists must provide other evidence.A panel of well-known cosmologists debated the discovery and the model of cosmic inflation itself at an event here on Friday (May 30) at the World Science Festival, moderated by theoretical physicist Brian Greene of Columbia University in New York.A rapid expansionOne of the panelists, cosmologist Alan Guth of MIT, developed the hypothesis of inflation in 1980 to explain the large-scale structure of the universe. Another panelist, cosmologist Andrei Linde of Stanford University, helped develop the model of inflation.The Big Bang left behind remnant heat, known as the cosmic microwave background (CMB). Radio astronomer Robert Wilson, who was in the audience, discovered the CMB along with physicist Arno Penzias in 1964. The CMB contains tiny temperature variations, but is remarkably uniform, which might be expected if the universe expanded from a very small region.If inflation occurred, scientists suspect it might have left an imprint on the CMB, produced by gravitational waves, which would appear as a swirly pattern in the CMB. John Kovac, an astronomer at Harvard University — another of the panelists — and colleagues claimed to have detected this pattern in March using the BICEP2 instrument at the South Pole.Controversy brewingBut since Kovac's team announced its findings, the results have come under fire from scientists who question whether the team had ruled out other possible sources that would produce the same swirly signature, such as galactic dust. In fact, two independent analyses of the data now suggest it could be accounted for by dust in the Milky Way.In the panel discussion, Kovac admitted some uncertainty, but defended the findings. "The pattern is not there by random chance," Kovac said. His team has further analyzed their data and feels "very confident" the results were not spurious, he said.But not everyone took the controversy lightly, including cosmologist Paul Steinhardt of Princeton University, who helped develop the model of inflation but now believes in an alternative model of the universe that suggests the existence of higher dimensions. Steinhardt took issue with how Kovac's team characterized their findings in March, saying that they were too confident in their statements at the time.Other groups are also looking for these ripples from the Big Bang, including balloon-based and space-based telescopes. The European Space Agency's Planck satellite is expected to release its own data very soon, possibly in the next three weeks, and should offer strong evidence one way or the other.Exciting timesDespite having helped develop it, Steinhardt now questions inflation itself. He said the theory was in some ways not falsifiable, which veers closer to the realm of metaphysics.But inflation is still the most widespread theory for how the universe began, Alan Guth said. Andre Linde compared inflation to democracy, which has been called "the worst form of government there is, except for all the other forms."As the evening panel concluded, Linde steered the discussion to a more hopeful note, about what it means to be a part of the endeavor to understand the universe in these times."There's something very exciting happening right now," he said.
That's third grade science they're failing, right there...
Quote from: BUncle on June 06, 2014, 04:44:38 PMThat's third grade science they're failing, right there...I'm okay if they're not teaching baby building to third graders. The fact that so many adults don't know what they're doing, not so much.So, if many believe that the sun orbits the Earth, same as the moon, I'm presuming they don't know why we have seasons and years, either. Well, at least they don't think the Earth is flat.
Quote from: Rusty Edge on June 06, 2014, 06:09:45 PMQuote from: BUncle on June 06, 2014, 04:44:38 PMThat's third grade science they're failing, right there...I'm okay if they're not teaching baby building to third graders. The fact that so many adults don't know what they're doing, not so much.So, if many believe that the sun orbits the Earth, same as the moon, I'm presuming they don't know why we have seasons and years, either. Well, at least they don't think the Earth is flat.Some of these individuals appear to be ignorant of many basic scientific facts. Does Gallup call many of the same people year after year asking these types of questions? Can I make it anymore clear? One thousand and twenty-six people are not a representative sampling of everyone in the United States of America.
Remember a LOT of people in a representative sample are going to be GEEZERS, 65+, who were educated in the 1950's or earlier, lots of these things were either unknown or were not considered 'basic' back then. Then account for their decades of non-usage and their senile brains and it would be a miracle if most seniors know ANY science what so ever.
I don't find it misleading, it is a valid test, perhaps not a test of the same quality as the SNIa as you claim but doesn't mean it can be ignored. While I agree that GRBs are very new phenomena the Quasar is quite old and their should be no shortage of study on them, granted Quasars are not believed to be standard candles, but this isn't required because they pulsate and we can simply look at the average pulsation rate vs Redshift and the time-dilation would readily pop-out of a large sample size if it was really their, we should have more faith in that large data set then the vastly smaller and perhaps overly pruned set of SNIa's?
Outside of time-dilation their is another property of expanding space geometry which is very simple and direct, distant objects should appear to have their angular size stretched and the surface brightness diminished in proportion to the spacial expansion. This is call the Tolman surface-brightness. When galaxies are examined we also fails to get the effect BB theory requires, and the defense offered that galaxies were brighter and smaller in the past it just the right amount to cancel out the expected effects is quite a stretch.
To run down some of the other big piece of evidence and show that they aren't really as strong as described.Redshift - Light could easily be stretched by another phenomenon in empty space, this is called 'Tired Light' and while we have no theoretical model for WHY such a thing might happen we can test between them by looking for time-dilation which would occur in BB but not in a Tired Light model. But the existence of Redshift in and of itself simply rules out any model which lacks one of the two mechanisms that could produce it.
The SN 2003fg (designated SNLS-03D3bb by the Canada-France-Hawaii Supernova Legacy Survey and sometimes called the "Champagne Supernova"), was an aberrant type Ia supernova discovered in 2003 and described in the journal Nature on September 21 of 2006.[1] It was nicknamed after the 1996 song "Champagne Supernova" by English rock band Oasis.[2]It may potentially revolutionize thinking about the physics of supernovae because of its highly unusual nature, in particular the mass of its progenitor. According to the current understanding, white dwarf stars go supernova type Ia when they approach 1.4 solar masses (1.4 times the mass of the Sun), termed the Chandrasekhar limit; the explosion occurs when the central density grows to a critical 2 × 109 g/cm3. The mass added to the star is believed to be donated by a companion star, either from the companion's stellar wind or the overflow of its Roche lobe as it evolves.[3]However, the progenitor of SN 2003fg reached two solar masses before exploding, more massive than thought possible. The primary mechanism invoked to explain how a white dwarf can exceed the Chandrasekhar mass is unusually rapid rotation; the added support effectively increases the critical mass. An alternative explanation is that the explosion resulted from the merger of two white dwarfs. The evidence indicating a higher than normal mass comes from the light curve and spectra of the supernova—while it was particularly overluminous the kinetic energies measured from ejecta signatures in the spectra appeared smaller than usual. The explanation is that more of the total kinetic energy budget was expended climbing out of the deeper than usual potential well.[4]This is important because the brightness of type Ia supernovae was thought to be essentially uniform, making them useful "standard candles" in measuring distances in the universe. Such an aberrant type Ia supernova could throw distances and other scientific work into doubt; however, the light curve characteristics of SNLS-03D3bb were such that it would never have been mistaken for an ordinary high-redshift Type Ia supernova.The discovery was made on the Canada-France-Hawaii Telescope and the Keck Telescope, both on Mauna Kea in Hawaii, and announced by researchers at the University of Toronto.[1] The supernova occurred in a galaxy some 4 billion light-years from Earth.