• Weak lensing from space I: instrumentation and survey strategy

    Updated: 2011-09-20 20:10:32
    : 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

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

    Updated: 2011-09-20 20:10:30
    . 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

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

    Updated: 2011-09-20 20:10:28
    : . 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 :

  • Evidence for dark radiation

    Updated: 2011-09-19 07:54:00
    : 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 Monday , 19 September 2011 Evidence for dark radiation I've just read this paper which looks deeply at the cosmic background radiation , and up dates our estimate for number of light low mass particles around the time of the big bang . The data clearly shows the equivalent of 4 neutrino species . This provides evidence for at least one unknown low mass particle , perhaps an additional low mass right handed neutrino , or any light scalar or vector super-symmetric neutrino as speculated about below . To be clear a axi-photon would not show up in

  • arXiv Find: New Sources of Gravitational Waves During Inflation

    Updated: 2011-09-06 19:55:43
    Here’s an interesting paper from yesterday’s hep-th batch of abstracts. One of the exciting prospects in observational cosmology over the next several years is finding signals of gravitational waves in the cosmic microwave background. These can be produced by inflation, and indeed simple models (one scalar field, no funny tricks) predict a “consistency relation” between [...]

  • More Hints of Dark Matter

    Updated: 2011-09-06 03:27:03
    Also known as, “scientific progress goes boink.” One of the benefits of being a Master of Time and Space is that I get to see the future. For example, cosmologically-inclined folks have been wondering for a few weeks about this press release from the TAUP conference in Munich, which includes the lines “Latest results from [...]

  • Symmetry Breaking, Groups E8 and E6

    Updated: 2011-06-12 22:57:00
    : , 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 Sunday , 12 June 2011 Symmetry Breaking , Groups E8 and E6 Reviewing articles at ArVix its come to my attention , that most popular super-symmetry and String phenomenologist aren't choosing the right models of symmetry breaking , ignoring classic papers , and proofs , just so they can use too easy but wrong models to fit Higgs bosons into a grand unified theory of the universe . In particle physics a phenomenologist is a physicist that tries to make the bridge between mathematical elegant models produced by theorists , and the experimental

  • Neutron Scattering and Fifth Forces

    Updated: 2011-06-07 14:43:00
    : 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 , 7 June 2011 Neutron Scattering and Fifth Forces I regularly read ArXiv for reports on the experimental limits on Fifth Forces . But this on I missed up to now . Neutron Scattering is regularly performed on every material under the sun , and in neutron scattering , scientist clearly see point like scattering from the strong force of a nucleus , giving very clear scattering from a collation of femtoscopic points . What scatterers don't see is any scattering from long range 1 r^2$ type columb forces . This clearly limits strongly any fifth

  • The Axial Force and the neutrino sea.

    Updated: 2011-05-18 20:02:00
    : . 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 , 18 May 2011 The Axial Force and the neutrino sea . Regularly readers will know that my blog is many about the possibility of a fifth force , which acts primary between neutrinos . The strength of the force is unknown , but can be comparatively large and still not noticeable by traditionally experimental because it doesn't interact with electrons at all . The simplest case a long force is a fully conversed charges with a massless force carrier , the axi-photon . I have not yet investigate the case of massive force carrier , but the

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