• Why We Need the Higgs, or Something Like It

    Updated: 2011-06-14 22:25:10
    In the comments to the previous post, Monty asks a perfectly good question, which can be shortened to: “Is the Higgs boson really necessary?” The answer is a qualified “yes” — we need the Higgs boson, or something like it. That is, we can’t simply take the Standard Model as we know it and extend [...]

  • 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 An 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

  • Weak lensing from space I: instrumentation and survey strategy

    Updated: 2011-03-22 06:26:14
    : 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 1 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 .

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

    Updated: 2011-03-22 06:26:12
    . 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 1 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

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

    Updated: 2011-03-22 06:26:09
    : . 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 1 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

  • Further Solar Neutrino Mysteries

    Updated: 2010-07-14 08:52:00
    : 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 , 14 July 2010 Further Solar Neutrino Mysteries Scientists have known how the Sun shines for quite a while , thermonuclear fusion was well established as was the so called proton proton chain in which four protons , from hydrogen atoms are converted into Helium nuclei,2 neutrinos and two positrons . Since neutrinos react rarely enough to mostly pass through all the sun , it would be possible to measure the rate of thermonuclear fusion in the sun , by how many neutrino where captured in a lab on earth . Yet when the homestake experiment

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