S
supafunky
Guest
scientists and astronomers are searching for dark matter inside the known universe, but have they considered the universe could be being pulled from the outside?
supafunky":h2fdkcqu said:can you xplain what you mean by they act like there is dark matter within them?
acsinnz":o4y5jm8d said:Dark matter is I believe the invisible matter that we know is there as observation show a star wobble or blink. Beyond that there is dark gases and ions in the vacuum of space.
But dark energy should be renamed "the force pushing the universe apart" which may well be an electric magnoflux force with no mass in it whatsoever.
We haven't lost 70% of the universe really; only the gravitationalists have!
CliveS
There are a lot of researchers out there who are a lot smarter than me. I suspect that the extent and the effect of electric fields in space have been thoroughly studied. If it is possible to attribute some or all of the force of "dark energy" to the effect of electric fields I'm sure the scientific community would be overjoyed.acsinnz":3vtl5g1y said:There are, I am sure, electric fields in outer space also which may have the effect of being a force that pushes the universe apart. We cant ignore these electric fields forever! or can we?
CliveS
acsinnz":1bof9mmm said:Yes Saiph it is neutral in composition BUT the H+ ions are coming towards us from the sun and the electrons are going back towards the sun. That balances very well and would be electrically correct.
You give the impression that the H+ ions and electrons are just floating around with no where to go which is electrically incorrect as a couple would get together with the electrons and form a hydrogen gas molecule given half a chance.
CliveS
supafunky":2g5059bp said:scientists and astronomers are searching for dark matter inside the known universe, but have they considered the universe could be being pulled from the outside?
You can also enclose in the URL tag, like this :csmyth3025":1j6bh6go said:http://en.wikipedia.org/wiki/Plasma_(physics)
NOTE: for some reason this link keeps dropping the last parenthesis mark, which resuluts in directing you to a wiki query page. Just add the last parenthesis to the address in the url bar or click on the link to the correct page indicated in the query.
Chris
[url]http://en.wikipedia.org/wiki/Plasma_(physics)[/url]
[url=http://en.wikipedia.org/wiki/Plasma_(physics)]Plasma (physics)[/url]
Thank you for your nice post.csmyth3025":31byusjk said:Thanks for the tip EarthlingX
Chris
supafunky":o42zs29s said:scientists and astronomers are searching for dark matter inside the known universe, but have they considered the universe could be being pulled from the outside?
Dark flow is a term from astrophysics describing a peculiar velocity of galaxy clusters. The actual measured velocity is the sum of the velocity predicted by Hubble's Law plus a small and inexplicable (or dark) velocity flowing in a common direction.
The authors (A. Kashlinsky, F. Atrio-Barandela, D. Kocevski, and H. Ebeling) suggest that the motion may be a remnant of the influence of no-longer-visible regions of the universe prior to inflation. Telescopes cannot see events earlier than about 380,000 years after the big bang, when the universe became transparent (the Cosmic Microwave Background); this corresponds to the particle horizon at a distance of about 46 billion (4.6×1010) light years. Since the matter causing the net motion in this proposal is outside this range, it would in a certain sense be outside our visible universe; however, it would still be in our past light cone.
A. Kashlinsky1, F. Atrio-Barandela2, D. Kocevski3, H. Ebeling4
ABSTRACT
Peculiar velocities of clusters of galaxies can be measured by studying the fluctuations in the cosmic microwave background (CMB) generated by the scattering of the microwave photons by the hot X-ray emitting gas inside clusters. While for individual clusters such measurements result in large errors, a large statistical sample of clusters allows one to study cumulative quantities dominated by the overall bulk flow of the sample with the statistical errors integrating down. We present results from such a measurement using the largest all-sky X-ray cluster catalog combined to date and the 3-year WMAP CMB data. We found a strong and
coherent bulk flow on scales out to at least >» 300h¡1Mpc, the limit of our catalog. This flow is difficult to explain by gravitational evolution within the framework of the concordance ΛCDM model and may be indicative of the tilt exerted across the entire current horizon by far-away pre-inflationary inhomogeneities.
John Roach
for National Geographic News
Published March 22, 2010
The Coma Galaxy Cluster, which appears to participate in the mysterious motion known as dark flow.
"Dark flow" is no fluke, suggests a new study that strengthens the case for unknown, unseen "structures" lurking on the outskirts of creation.
In 2008 scientists reported the discovery of hundreds of galaxy clusters streaming in the same direction at more than 2.2 million miles (3.6 million kilometers) an hour.
This mysterious motion can't be explained by current models for distribution of mass in the universe. So the researchers made the controversial suggestion that the clusters are being tugged on by the gravity of matter outside the known universe.
Now the same team has found that the dark flow extends even deeper into the universe than previously reported: out to at least 2.5 billion light-years from Earth.
After using two additional years' worth of data and tracking twice the number of galaxy clusters, "we clearly see the flow, we clearly see it pointing in the same direction," said study leader Alexander Kashlinsky, an astrophysicist at NASA's Goddard Space Flight Center in Maryland.
"It looks like a very coherent flow."
The find adds to the case that chunks of matter got pushed outside the known universe shortly after the big bang—which in turn hints that our universe is part of something larger: a multiverse.
SpaceFellowship
March 11, 2010
The colored dots are clusters within one of four distance ranges, with redder colors indicating greater distance. Colored ellipses show the direction of bulk motion for the clusters of the corresponding color. Images of representative galaxy clusters in each distance slice are also shown. Credit: NASA/Goddard/A. Kashlinsky, et al.
...Analysis by Ian O'Neill
Sat Oct 2, 2010 06:55 AM ET
The scales are mind-boggling and the physics is cutting edge, so how do you go about simulating the collision of two galactic clusters? Using some of the most powerful computers in the world, researchers at Argonne National Laboratory near Chicago Ill. have done just that.
[youtube]http://www.youtube.com/watch?v=opP7ttCCC20[/youtube]The code simulates the interaction of both normal matter and dark matter. The normal matter interacts, mixes and generates turbulence as the collision progresses. For this component of the simulation they use a hydrodynamic code -- it's basically the science of how two liquids or gases mix. As the two clouds of dark matter inside each cluster can only interact gravitationally (the dark matter particles cannot collide, or scatter, via any other mechanism), each particle is modeled individually. This an N-body code.
Once the simulation is sent on its way, the mixing of normal matter is simulated along with the dark matter. As the dark matter cores from both clusters reach an equilibrium state, orbiting inside the post-collision cluster, its motion gravitationally mixes the normal matter.
"The dark matter cores slip past and through each other,whereas the two gas components interact and mix," narrator Carrie Eder explains during the collision visualization.
"It is also clearly seen that the mixing of the gas is driven completely by the violent orbital motion of the dark matter cores."
Here is the simulation in all its glory:
ArgonneNationalLab | August 09, 2010
Since structure in the universe forms in a bottom-up fashion, with smaller structures merging to form larger ones, modeling the merging process in detail is crucial to our understanding of cosmology. At the current epoch, we observe clusters of galaxies undergoing mergers. It is seen that the two major components of galaxy clusters, the hot intracluster gas and the dark matter, behave very differently during the course of a merger. Using the N-body and hydrodynamics capabilities in the FLASH code, we have simulated a suite of representative galaxy cluster mergers, including the dynamics of both the dark matter, which is collisionless, and the gas, which has the properties of a fluid. 3-D visualizations such as these demonstrate clearly the different behavior of these two components over time.
Credits:
John Zuhone (Harvard-Smithsonian Center for Astrophysics), Don Lamb (Flash Center, U of C), Jonathan Gallagher (Flash Center U of C)
This work was supported in part by the DOE NNSA ASC ASAP and by the NSF. This work also used computational resources at the ALCF at ANL awarded under the INCITE program, which is supported by the DOE Office of Science.
This simulation was completed in part using the computational resources of the Argonne Leadership Computing Facility at Argonne National Laboratory, which is supported by the Office of Science of the U.S. Department of Energy under contract: DE-AC02-06CH11357.
This visualization was produced using the visualizationand analysis resources of the Argonne Leadership Facility that is supported by the Department of Energy's Office of Science.