marcus
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turbo-1 said:Interesting - their model has built-in inflation from a bounce (perhaps one of many), no particle horizon, and a universe that has always existed. A temporally infinite universe moots the "something from nothing" question, since the "something" has always existed anyway.
The first notice of inflation as an automatic feature of Loop gravity was in 2002.
Martin Bojowald
Inflation from Quantum Geometry
http://arxiv.org/gr-qc/0206054
Bojowald is known for having removed the big bang singularity---resulting in a bounce---in 2001. That was expected result----there'v been other cases where quantizing a classical has eliminated singularities or other glitches in behavior.
But getting inflation "for free" was an unexpected bonus from the theory.
So a couple of string proponents---Roy Maartens and Shinji Tsujikawa---investigated to see if it was kosher. And it was! They quibbled with Bojowald on some non-essential points but confirmed the main result.
they worked with a Loop postdoc named Parampreet Singh who is now at Ashtekar's institute, Penn State. that was last year
Tsujikawa, Singh, Maartens
Loop Quantum Gravity Effects on Inflation and the CMB
http://arxiv.org/astro-ph/0311015
they also confirmed that some imprint of LQG on the CMB might ultimately be observable, something to look for, as a test of the theory.
This fall Singh gave a series of 3 talks about further work along those lines (LQC phenomenology, predicting things to look for, as tests)
You can tell that the story, for me, has drama. It is a big part of it. Bojowald inflation result came as a surprise, it could have been wrong,
string guys checked it, apparently it's right, half a dozen others checked it, Ganashyam Date found that it was generic or robust.
And now in Fall 2004 Singh has laid out some faint traces of imprint of the theory to look for, in his seminar talks. this is all since mid-2002, less than a year and a half. Kind of action that's fun to watch, if someone's into it .
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