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lowenz
28-10-2009, 19:41
http://www.universetoday.com/2009/10/28/einstein-still-rules-says-fermi-telescope-team/

While the Fermi Space Telescope has mapped the gamma ray sky with unprecedented resolution and sensitivity, it now has been able to take a measurement that has provided rare experimental evidence about the very structure of space and time, unified as space-time. Einstein's theory of relativity states that all electromagnetic radiation travels through a vacuum at the same speed. Fermi detected two gamma ray photons which varied widely in energy; yet even after traveling 7 billion years, the two different photons arrived almost at instantaneously.

On May 10, 2009, Fermi and other satellites detected a so-called short gamma ray burst, designated GRB 090510. Astronomers think this type of explosion happens when neutron stars collide. Ground-based studies show the event took place in a galaxy 7.3 billion light-years away. Of the many gamma ray photons Fermi's LAT detected from the 2.1-second burst, two possessed energies differing by a million times. Yet after traveling some seven billion years, the pair arrived just nine-tenths of a second apart.

"This measurement eliminates any approach to a new theory of gravity that predicts a strong energy dependent change in the speed of light," Michelson said. "To one part in 100 million billion, these two photons traveled at the same speed. Einstein still rules."

"Physicists would like to replace Einstein's vision of gravity — as expressed in his relativity theories — with something that handles all fundamental forces," said Peter Michelson, principal investigator of Fermi's Large Area Telescope, or LAT, at Stanford University in Palo Alto, Calif. "There are many ideas, but few ways to test them."

Many approaches to new theories of gravity picture space-time as having a shifting, frothy structure at physical scales trillions of times smaller than an electron. Some models predict that the foamy aspect of space-time will cause higher-energy gamma rays to move slightly more slowly than photons at lower energy.

GRB 090510 displayed the fastest observed motions, with ejected matter moving at 99.99995 percent of light speed. The highest energy gamma ray yet seen from a burst — 33.4 billion electron volts or about 13 billion times the energy of visible light — came from September's GRB 090902B. Last year's GRB 080916C produced the greatest total energy, equivalent to 9,000 typical supernovae.

T3d
28-10-2009, 20:41
c'è qualche mio collega che sta seguendo il corso di relatività generale e sta violentemente battendo la testa contro tensori a n-mila indici :D

non sembrano nemmeno formule, sono proprio geroglifici :sofico:

lowenz
28-10-2009, 20:53
c'è qualche mio collega che sta seguendo il corso di relatività generale e sta violentemente battendo la testa contro tensori a n-mila indici :D

non sembrano nemmeno formule, sono proprio geroglifici :sofico:
Infatti lo scoglio pratico della relatività è quello :asd:

lowenz
29-10-2009, 16:22
Altro articolo a riguardo :D

http://physicsworld.com/cws/article/news/40834

lowenz
18-03-2010, 20:23
Se possibile unire con questo vecchio thread!
http://www.hwupgrade.it/forum/showthread.php?t=1501314

Altra notizia fresca!

http://www.universetoday.com/2010/03/18/this-is-getting-boring-general-relativity-passes-yet-another-big-test/

Published in 1915, Einstein's theory of general relativity (GR) passed its first big test just a few years later, when the predicted gravitational deflection of light passing near the Sun was observed during the 1919 solar eclipse.
In 1960, GR passed its first big test in a lab, here on Earth; the Pound-Rebka experiment. And over the nine decades since its publication, GR has passed test after test after test, always with flying colors (check out this review for an excellent summary).
But the tests have always been within the solar system, or otherwise indirect.
Now a team led by Princeton University scientists has tested GR to see if it holds true at cosmic scales. And, after two years of analyzing astronomical data, the scientists have concluded that Einstein's theory works as well in vast distances as in more local regions of space.

The scientists' analysis of more than 70,000 galaxies demonstrates that the universe – at least up to a distance of 3.5 billion light years from Earth – plays by the rules set out by Einstein in his famous theory. While GR has been accepted by the scientific community for over nine decades, until now no one had tested the theory so thoroughly and robustly at distances and scales that go way beyond the solar system.
Reinabelle Reyes, a Princeton graduate student in the Department of Astrophysical Sciences, along with co-authors Rachel Mandelbaum, an associate research scholar, and James Gunn, the Eugene Higgins Professor of Astronomy, outlined their assessment in the March 11 edition of Nature.
Other scientists collaborating on the paper include Tobias Baldauf, Lucas Lombriser and Robert Smith of the University of Zurich and Uros Seljak of the University of California-Berkeley.
The results are important, they said, because they shore up current theories explaining the shape and direction of the universe, including ideas about dark energy, and dispel some hints from other recent experiments that general relativity may be wrong.
"All of our ideas in astronomy are based on this really enormous extrapolation, so anything we can do to see whether this is right or not on these scales is just enormously important," Gunn said. "It adds another brick to the foundation that underlies what we do."
GR is one, of two, core theories underlying all of contemporary astrophysics and cosmology (the other is the Standard Model of particle physics, a quantum theory); it explains everything from black holes to the Big Bang.
In recent years, several alternatives to general relativity have been proposed. These modified theories of gravity depart from general relativity on large scales to circumvent the need for dark energy, dark matter, or both. But because these theories were designed to match the predictions of general relativity about the expansion history of the universe, a factor that is central to current cosmological work, it has become crucial to know which theory is correct, or at least represents reality as best as can be approximated.
"We knew we needed to look at the large-scale structure of the universe and the growth of smaller structures composing it over time to find out," Reyes said. The team used data from the Sloan Digital Sky Survey (SDSS), a long-term, multi-institution telescope project mapping the sky to determine the position and brightness of several hundred million galaxies and quasars.
By calculating the clustering of these galaxies, which stretch nearly one-third of the way to the edge of the universe, and analyzing their velocities and distortion from intervening material – due to weak lensing, primarily by dark matter – the researchers have shown that Einstein's theory explains the nearby universe better than alternative theories of gravity.

The Princeton scientists studied the effects of gravity on the SDSS galaxies and clusters of galaxies over long periods of time. They observed how this fundamental force drives galaxies to clump into larger collections of galaxies and how it shapes the expansion of the universe.
Critically, because relativity calls for the curvature of space to be equal to the curvature of time, the researchers could calculate whether light was influenced in equal amounts by both, as it should be if general relativity holds true.
"This is the first time this test was carried out at all, so it's a proof of concept," Mandelbaum said. "There are other astronomical surveys planned for the next few years. Now that we know this test works, we will be able to use it with better data that will be available soon to more tightly constrain the theory of gravity."
Firming up the predictive powers of GR can help scientists better understand whether current models of the universe make sense, the scientists said.
"Any test we can do in building our confidence in applying these very beautiful theoretical things but which have not been tested on these scales is very important," Gunn said. "It certainly helps when you are trying to do complicated things to understand fundamentals. And this is a very, very, very fundamental thing."
"The nice thing about going to the cosmological scale is that we can test any full, alternative theory of gravity, because it should predict the things we observe," said co-author Uros Seljak, a professor of physics and of astronomy at UC Berkeley and a faculty scientist at Lawrence Berkeley National Laboratory who is currently on leave at the Institute of Theoretical Physics at the University of Zurich. "Those alternative theories that do not require dark matter fail these tests."

gugoXX
18-03-2010, 22:17
La relativita' generale "funziona" bene per grandi masse e per grandi distanze.
Pero' ad una certa scala abbiamo problemi, e abbiamo "inventato" una presunta materia oscura finora non effettivamente riscontrata.

E' una situazione abbastanza imbarazzante ammettere che manca all'appello il 90% della massa dell'universo (cit.)

Magari non esiste, ed e' una inesattezza della relativita' generale.
Puzza sempre di piu' di etere.

Jarni
19-03-2010, 00:07
c'è qualche mio collega che sta seguendo il corso di relatività generale e sta violentemente battendo la testa contro tensori a n-mila indici :D

non sembrano nemmeno formule, sono proprio geroglifici :sofico:

Se vedi i simboli di Christoffel di prima e seconda specie ti metti a piangere...:D
Li mortacci a chi l'ha inventati, 'sti tensori!:muro:

:dissident:
19-03-2010, 00:30
La relativita' generale "funziona" bene per grandi masse e per grandi distanze.
Pero' ad una certa scala abbiamo problemi, e abbiamo "inventato" una presunta materia oscura finora non effettivamente riscontrata.

E' una situazione abbastanza imbarazzante ammettere che manca all'appello il 90% della massa dell'universo (cit.)

Magari non esiste, ed e' una inesattezza della relativita' generale.
Puzza sempre di piu' di etere.

A dire il vero ci sono parecchie evidenze osservative della reale esistenza della Materia Oscura..

gugoXX
19-03-2010, 00:36
A dire il vero ci sono parecchie evidenze osservative della reale esistenza della Materia Oscura..

Ad esempio?

Jarni
19-03-2010, 00:48
Ad esempio?

Effetti gravitazionali nel moto delle galassie.

:dissident:
19-03-2010, 00:48
Ad esempio:

NASA Finds Direct Proof of Dark Matter (http://www.nasa.gov/home/hqnews/2006/aug/HQ_06297_CHANDRA_Dark_Matter.html)

Ma anche le dinamiche dei superammassi e i fenomeni di lente gravitazionale sembrano indicare che esista questa forma di massa oscura..

gugoXX
19-03-2010, 00:55
Effetti gravitazionali nel moto delle galassie.

Ecco. Dicevo proprio il contrario.
Per giustificare il moto delle galassie e continuare a farle ruotare in un universo guidato dalla relativita' generale e' stata ipotizzata la materia oscura che sarebbe la causa dell'altrimenti anomalia
Oppure la materia oscura non esiste, e la teoria che abbiamo non sarebbe quella definitiva, e le galassie si starebbero muovendo secondo una legge diversa, senza bisogno di materia oscura.

Nella rotazione delle galassie non stiamo parlando di pochi punti percentuali, cosi' come per l'anomalia della precessione di mercurio se studiato secondo la gravitazione di Newton.
La differenza rispetto alla teoria e' enorme. Tanto da rendere necessaria la "creazione" di un 90% di massa mancante.
Cosa propone Occam? Lo tiriamo fuori solo quando si parla di complottismo?