Search

23 Oct 2012: which could be readily detectable around other stars by Spitzer 24 μm surveys for 25 Myr after. ... SiO h (24). which occurs with a rate coefficient m3 s-1 (Andreazza et al.

23 Feb 2012: Gyr), and its excess emission at 24 μm lieswell outside the range defined by most stars of its age (Figure 1;Wyatt 2008). ... The median S/N of the SL data is 24 and of theSH/LH data is 37.

12 Jan 2012: 8 arcminaway to the SE (PA = 120) that is visible at 24, 70, and100µm.

19 Jan 2012: 0 2 4 6 8 10 12 14 16 18 20 22 24 26 28 300.0.

24 Nov 2012: Finally, we used the SPIRE 3σ upper limits as a constraint toreject any model with a flux density of the dust emission largerthan 24 mJy at 250µm. ... The upper inset zooms on the IRS wavelengths and displays spectra asSν(λ/24)2 on a linear scale

12 Mar 2012: Apply local SU(5) gauge symmetry - get 24 gauge bosons: γ, W+, W-, Z, 8 gluons and 12 X,Y bosons mediating quark-lepton transitions!These violate baryon and lepton number! ... and sgn(µ) as in SUGRA!Cgrav! Coupling for decays into gravitinos! 3/2/12

13 Mar 2012: 3/12/12 Astroparticle 24. Exploit fact that gravity couples to all particle types! ... Assume system created in disk - get minimum lifetime for black hole, 24 Myr, and hence max curvature of ADS bulk - 80 microns!

24 Jan 2012: CURRICULUM VITAE. FULL NAME: George Petros EFSTATHIOUNATIONALITY: BritishDATE OF BIRTH: 2nd Sept 1955. QUALIFICATIONS. Dates Academic Institution Degree. 10/73 to 7/76 Keble College, Oxford. B.A. in Physics10/76 to 9/79 Department of Physics, Ph.D.

27 Feb 2012: 2/20/12 Astroparticle 24.  Bulk region.  Co-annihilation region.  Focus point region.

10 Dec 2012: There isboth cool dust (observable to Herschel) and warm dust(evident from IRS and MIPS 24 excesses). ... In the context of the wide belt imaging model, the IRSand MIPS 24 excesses are attributed to a warm innerring.