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Abell 3376: Einstein's Theory Fights off Challengers
Abell 3376
Abell 3376
Abell 3376

  • Via different methods, two separate teams have tested gravity and General Relativity using Chandra observations of galaxy clusters

  • The results from each show that Einstein's famous theory works even on some of the largest scales

  • Such studies are necessary to understand the evolution of the Universe and the nature of dark energy, one of the biggest mysteries in science

Two different teams have reported using Chandra observations of galaxy clusters to study the properties of gravity on cosmic scales and test Einstein's theory of General Relativity. Such studies are crucial for understanding the evolution of the universe, both in the past and the future, and for probing the nature of dark energy, one of the biggest mysteries in science.

This composite image of the galaxy cluster Abell 3376 shows X-ray data from the Chandra X-ray Observatory and the ROSAT telescope in gold, an optical image from the Digitized Sky Survey in red, green and blue, and a radio image from the VLA in blue. The "bullet-like" appearance of the X-ray data is caused by a merger, as material flows into the galaxy cluster from the right side. The giant radio arcs on the left side of the image may be caused by shock waves generated by this merger.

The growth of galaxy clusters like Abell 3376 is influenced by the expansion rate of the universe - controlled by the competing effects of dark matter and dark energy - and by the properties of gravity over large scales. By contrast, observations of supernovas or the large-scale distribution of galaxies, which measure cosmic distances, depend only on the expansion rate of the universe and are not sensitive to the properties of gravity.

In the first of the new studies of gravity, an alternative theory to General Relativity called "f(R) gravity" was tested. In this theory, the acceleration of the expansion of the universe does not come from an exotic form of energy but from a modification of the gravitational force. Mass estimates of galaxy clusters in the local universe were compared with model predictions for f(R) gravity. Data from geometrical studies, such as supernova work, were also used. Using this comparison between theory and observation, no evidence was found that gravity is different from General Relativity on scales larger than 130 million light years. This limit corresponds to a hundred-fold improvement on the bounds of the modified gravitational force's range that can be set without using the cluster data.

In the second study, a comparison was made between X-ray observations of how rapidly galaxy clusters have grown over cosmic time to the predictions of General Relativity. Once again, data from geometrical studies such as distances to supernovas and galaxy clusters were incorporated. Nearly complete agreement was seen between observation and theory, arguing against any alternative gravity models with a different rate of growth. In particular "DGP gravity" (named after its inventors Gia Dvali, Gregory Gabadadze, and Massimo Porrati) predicts a slower rate of cluster growth than General Relativity, because gravity is weakened on large scales as it leaks into an extra dimension. Like f(R) gravity, the DGP model is designed to avoid the need for an exotic form of energy causing cosmic acceleration.

Chandra observations of galaxy clusters have previously been used to show that dark energy has stifled the growth of these massive structures over the last 5 billion years and to provide independent evidence for the existence of dark energy by offering a different way to measure cosmic distances.

Fast Facts for Abell 3376:
Credit  X-ray (NASA/CXC/SAO/A. Vikhlinin; ROSAT), Optical (DSS), Radio (NSF/NRAO/VLA/IUCAA/J.Bagchi)
Release Date  April 14, 2010
Scale  Image is 29 arcmin across (about 5 million light years across).
Category  Groups & Clusters of Galaxies
Coordinates (J2000)  RA 06h 02m 10.00s | Dec -39 57' 20.99"
Constellation  Columba
Observation Date  03/16/2002
Observation Time  13 hours 20 min
Obs. ID  3202
Instrument  ACIS
References Schmidt, F. et al. 2009, Phys Rev D, 80, 083505; Rapetti, D. et al. 2010, MNRAS (in press); arXiv:0911.1787v1
Color Code  X-ray (Gold); Optical (Red, Green, Blue); Radio (Blue)
Radio
Optical
X-ray
Distance Estimate  About 614 million light years
Visitor Comments (15)

Great information. I got lucky and found your site from a random Google search. Fortunately for me, this topic just happens to be something that I've been trying to find more info on for research purposes. Keep up the great work and thanks a lot.

Posted by J D on Monday, 02.21.11 @ 17:38pm


chandra.harvard.edu did it again. Incredible writing.

Posted by Johnie Buck on Monday, 05.31.10 @ 05:43am


Dear Len,
The redshifts of the galaxies in the cluster are used, along with a model for the expansion of the universe as dominated by dark energy and dark matter. The details are complicated, but in general the larger the redshift the larger the distance.
P. Edmonds for CXC

Posted by P. Edmonds on Wednesday, 04.28.10 @ 12:12pm


Dear Ved,
This work is testing the *possibility* that the acceleration in the expansion of the universe is because of the modification of gravity. The crucial point is that so far no evidence has been found requiring changes to General Relativity.
P. Edmonds for CXC

Posted by P. Edmonds on Wednesday, 04.28.10 @ 12:09pm


Dear Georges,
Thanks for your good question. To be more precice, the expansion rate is
not sensitive to the properties of gravity when acting over very large scales. For example, in a model of the universe people can change the way gravity acts over large scales so that it differs from the predictions of General Relativity. This reproduces accelerated expansion without the need for dark energy, but this changes the way galaxy clusters grow. So far such deviations from General Relativity have not been seen.
P. Edmonds for CXC

Posted by P. Edmonds on Wednesday, 04.28.10 @ 12:06pm


Dear John,
This is an interesting idea, but even if some mechanism was able to generate magnetic fields over very large scales, it wouldn't be able to have a significant affect since matter on these scales will be electrically neutral. On these scales gravity dominates over magnetic forces.
P.Edmonds for CXC

Posted by P. Edmonds on Wednesday, 04.28.10 @ 12:03pm


Please explore our web-site particularly the field guide,
http://www.chandra.harvard.edu/field_guide.html

and for more information about Chandra visit
http://www.chandra.harvard.edu/about/

CXC

Posted by CXC on Wednesday, 04.28.10 @ 11:17am


Would it be possible to have more information about Chandra? Like a portable transmitter like those who are doing that.

Also more info on aerospace assistive medical technologies.

Thank you

Posted by Diego Thornton on Wednesday, 04.21.10 @ 16:48pm


I wonder if anyone ever thought that maybe this Dark Matter Dark Energy is nothing more than all the magnetic forces in the universe pushing and pulling everything around and being such a large magnetic force would be very difficult to detect since it would be on such an epic scale there is not a technology out yet to prove against this theory.

Posted by John on Saturday, 04.17.10 @ 14:32pm


Very nice articles thanks

Posted by Marcel on Thursday, 04.15.10 @ 13:00pm


Interesting article. But your comment about the expansion rate being not sensitive to the properties of gravity is somewhat puzzling. After all, the expansion rate is none other than the Hubble parameter, which is expressed in terms of the energy density rho divided by the square of the gravitational constant G, in addition to lambda and the curvature parameter k. So how could it be said to be insensitive to the properties of gravity?

Posted by Georges Melki on Thursday, 04.15.10 @ 01:21am


Dear sir
As you mentioned that expansion of the universe is not because of exotic energy but from the modification of gravity force. Is it not so that gravity force is also Energy it is all over in the universe?
If I am wrong please forgive me for the mistake.
thanks and best regards

Posted by Ved Parkash on Thursday, 04.15.10 @ 00:27am


How can one tell the difference between 100 million light years away and 10 or 600 million light years away.

I am constantly befuddled by the distances away and across in light years.

I would love a poster of the latest Abell 3376, if it become available.

Posted by Len Gyson on Wednesday, 04.14.10 @ 22:22pm


Wish my life could continue for another 60 years - just to see what we discover. Keep up the good work and I hope sufficient funds will continue so you can continue. Your studies are worth every penny. My hat is off to each of you. Health, Hope, Happiness Mike

Posted by Mike Giambra on Wednesday, 04.14.10 @ 21:48pm


This article and the conclusions are just wonderful to behold too bad I cannot send an email to Albert Einstein letting him know that he was right all along and the inescapable conclusion that the expansion constant is in fact and not an error of understanding on the part of the old man Congratulations to the teams that have done this fine work

Posted by Neil Fiertel on Wednesday, 04.14.10 @ 20:38pm


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