• Weak lensing from space I: instrumentation and survey strategy

    Updated: 2010-04-30 09:28:15
    : Home About Publishing Technology IngentaConnect Blog Help Check our FAQs Or contact us to report problems : with Subscription access Article delivery Registration Library administrator tasks Other problems For Publishers Why go online Why choose IngentaConnect Beyond Print : enhancing your service Access and authentication Article purchasing Managing your publications Usage statistics Reference linking services Branding opportunities Keeping in touch Contact us For Researchers For Authors About IngentaConnect Search and browse Publications available Accessing articles Managing your account Creating marked lists Creating Saved searches Receiving email alerts Subscribing to RSS feeds Software compatibility Ingenta Labs Register For Librarians Resource Zone Why choose IngentaConnect Why

  • Signatures of ultra-high energy cosmic ray composition from propagation of nuclei in intergalactic photon fields

    Updated: 2010-04-30 09:28:15
    . Home About Publishing Technology IngentaConnect Blog Help Check our FAQs Or contact us to report problems : with Subscription access Article delivery Registration Library administrator tasks Other problems For Publishers Why go online Why choose IngentaConnect Beyond Print : enhancing your service Access and authentication Article purchasing Managing your publications Usage statistics Reference linking services Branding opportunities Keeping in touch Contact us For Researchers For Authors About IngentaConnect Search and browse Publications available Accessing articles Managing your account Creating marked lists Creating Saved searches Receiving email alerts Subscribing to RSS feeds Software compatibility Ingenta Labs Register For Librarians Resource Zone Why choose IngentaConnect Why

  • Supersymmetric dark matter in M31: can one see neutralino annihilation with CELESTE?

    Updated: 2010-04-30 09:28:15
    : . Home About Publishing Technology IngentaConnect Blog Help Check our FAQs Or contact us to report problems : with Subscription access Article delivery Registration Library administrator tasks Other problems For Publishers Why go online Why choose IngentaConnect Beyond Print : enhancing your service Access and authentication Article purchasing Managing your publications Usage statistics Reference linking services Branding opportunities Keeping in touch Contact us For Researchers For Authors About IngentaConnect Search and browse Publications available Accessing articles Managing your account Creating marked lists Creating Saved searches Receiving email alerts Subscribing to RSS feeds Software compatibility Ingenta Labs Register For Librarians Resource Zone Why choose IngentaConnect Why

  • Dark Iron, and Mirror Matter

    Updated: 2010-04-11 16:14:11
    : , 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 Monday , 22 March 2010 Dark Iron , and Mirror Matter Dark Iron it sounds like something drawf's mine in a fantasy game , not from something out of astrophysics but Mirror Matter Iron Nuclei is what Robert Foot claims the CDMS II detector has discovered . Combined with his sighting of mirror electrons in the CDMS detector , and candidate of mirror oxygen atoms in the solid DAMA results . Thing are looking up for mirror matter as a theory of dark . matter The Theory of Mirror Matter , is just like in Alice in the looking glass , another physic

  • The Demise of the LSP

    Updated: 2010-04-11 16:14:09
    : 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 , 23 December 2009 The Demise of the LSP Astronomers have known there was something missing from universe for years , Zwicky first calculated how stars should move under gravity in a galaxy back in 1933, and found there was far more matter in a galaxy than could be accounted for by stars . But it wasn't until the 1990s that astronomers really begin to believe in dark matter . But now finally experiments are starting to get close to discovering what it all the mysterious missing matter really is . And looking more and more like it isn't

  • A possible detection of heavy-photons

    Updated: 2010-04-08 09:01:29
    : 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 Friday , 29 January 2010 A possible detection of heavy-photons Always on the lookout for strange physics , I was fascinated by a Paper by Boer and Fields at ArXiv . They analysised 7 previous experiment all which should something bizarre , A new Light Neutral Boson . There particle has a mass range of 1.5MeV to 20MeV , a lifespan of about 10^-15 to 10^-16 seconds . And strangely shows up only in experiment using photograph Emulsion . There X boson appears to be made in the decay on the neutral pion , one decay out of every thousand , and itself decays into an electron positron pair . They don't even have bad statistics ranging for 2.8 sigma to 8 sigma in the different experiments the . review A boson is a force carrying particle , given a mass of 1 MeV , Boer's and Field's particle would mediate a short range force novel to the standard model . Looking at previous limits to a fifth force this particle is in a range previously thought to

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