Updated: 2012-09-06 03:12:04
: Contact us Help Shopping cart Home About us Article title , keywords or abstract Article title Publication title Author Advanced search Subject Publisher Publication Browse : by Home Astroparticle Physics Volume 20, Number 4 Weak lensing from space I : instrumentation and survey strategy Authors : Rhodes J . Refregier A . Massey R . Albert J . Bacon D . Bernstein G . Ellis R . Jain B . Kim A . Lampton M . McKay T . Akerlof C . Aldering G . Amanullah R . Astier P . Baltay C . Barrelet E . Bebek C . Bergstrom L . Bercovitz J . Bester M . Bigelow B . Bohlin R . Bonissent A . Bower C . Brown M . Campbell M . Carithers W . Commins E . Day C . Deustua S . DiGennaro R . Ealet A . Emmet W . Eriksson M . Fouchez D . Fruchter A . Genat J . F . Gerdes D . Gladney L . Goldhaber G . Goobar A . Groom
Updated: 2012-09-06 03:12:03
. Contact us Help Shopping cart Home About us Article title , keywords or abstract Article title Publication title Author Advanced search Subject Publisher Publication Browse : by Home Astroparticle Physics Volume 20, Number 4 Signatures of ultra-high energy cosmic ray composition from propagation of nuclei in intergalactic photon fields Authors : Yamamoto T . Mase K . Takeda M . Sakaki N . Teshima . M : Source Astroparticle Physics Volume 20, Number 4, January 2004 pp . 405-412(8 Publisher : Elsevier view table of contents next article Buy download fulltext : article This article is hosted on another website . You may be required to register , activate a subscription or purchase the article before you can obtain the full . text Proceed : Keywords Ultra-high energy cosmic rays Propagation
Updated: 2012-09-06 03:12:01
: . Contact us Help Shopping cart Home About us Article title , keywords or abstract Article title Publication title Author Advanced search Subject Publisher Publication Browse : by Home Astroparticle Physics Volume 20, Number 4 Supersymmetric dark matter in M31 : can one see neutralino annihilation with CELESTE Authors : Falvard A . Giraud E . Jacholkowska A . Lavalle J . Nuss E . Piron F . Sapinski M . Salati P . Taillet R . Jedamzik K . Moultaka . G : Source Astroparticle Physics Volume 20, Number 4, January 2004 pp . 467-484(18 Publisher : Elsevier view table of contents next article Buy download fulltext : article This article is hosted on another website . You may be required to register , activate a subscription or purchase the article before you can obtain the full . text Proceed :
Updated: 2012-01-10 23:53:00
: skip to main skip to sidebar Axitronics Dark energy solved By giving neutrino there own type of electric and magnetic forces . The force is known as the axial force , thus the title , axitronics , as the equivalent of electronics for . neutrinos Tuesday , 10 January 2012 Dark Energy and Expansion 101 BDOA wrote this over at Science 2.0 in reply to an articles on the Einstein plus Higgs expansions paradox . How can space expanded when there's an Aether except relatisticly invarent like field of Higgs particle in it . I'll need to dumb this done to the level of the . readership Space doesn't expand next you'll be telling me that Hubble was a bungling . detective Its a good paradox though . Is there an energy cost of free space , as your expand the universe . Especially if that free space
Updated: 2012-01-04 11:48:00
: skip to main skip to sidebar Axitronics Dark energy solved By giving neutrino there own type of electric and magnetic forces . The force is known as the axial force , thus the title , axitronics , as the equivalent of electronics for . neutrinos Wednesday , 4 January 2012 Hiding a Z' Just five days ago I posted about results on how the Higgs Boson decayed , and suggested extra pairs of vector like quarks to make the photon signal match . Since then a pape r by Radovan Dermisek , Sung-Gi Kim , Aditi Raval has come out showing that a Z' hiding very near in mass to the standard models Z the neutral particle of the weak force solves the problem of the forward backward asymmetry in bottom quark creation . The Z' is around 92.5 GeV just 1GeV more missing than the ordinary Z interacts with
