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American Physical SocietyApril Meeting 2013 April 13 - April 16 Denver, CO, USACopyright 2013 Thomas J. Buckholtz1

1Dark MatterBosons and FermionsThomas J. Buckholtz Thomas.J.Buckholtz@gmail.com Abstract: J8.000082Copyright 2013 Thomas J. Buckholtz

2List aspects of this talkNote scope of researchSummarize some findingsProvide some detailsDiscuss possible objectionsNote some implicationsDark-matter beings would consider us to be part of [their] dark matter.3Copyright 2013 Thomas J. Buckholtz

3Note scope of researchScope of research4Copyright 2013 Thomas J. BuckholtzTSMHereHereList known elementary particlesyesyesExplain gravitationnoyesExplain dark matternoyesExplain dark energynoyesExplain rate-of-expansion changesnoyesCompute neutrino massnoyesCompute Higgs-like boson massno ?yesExplain matter/anti-matter 1no ?yes ?Explain size of CP violationnoyes ?Provide other predictions?yes

4Summarize some findingsThe universe includes 24 ensembles of somewhat similar stuff.Baryonic matter (including its photons) is one ensemble.Each ensemble has its own traditional elementary particles, except gravitons.Beings in each ensemble could Measure the ensembles elementary particles as being somewhat similar baryonic-matters measurements of traditional elementary particles.Consider that there are 5 ensembles of dark matter and 18 ensembles of dark energy.Know that their ensemble shares gravity with the 5 ensembles they consider to be dark matter.

5Copyright 2013 Thomas J. Buckholtz

5Summarize some findings(4/3)(6)2 = {(qe)2/(40)} / {GN(me)2} m tauon / me e3e - 3m neutrino me -1 3/2 0.09161 eV/c2 m Higgs-like boson (17/9)1/2 m Z boson 125.325 GeV/c2m Z boson me . 6 . (1.1062)2 . 1/3 . -3/2 6Copyright 2013 Thomas J. Buckholtz

6Provide some details10 e-family bosons (eC)4321CSpan(ensembles)44e4photon134e3graviton3e3624e23e22e21214e13e12e11e124Forcer-2r-4r-6r-87Copyright 2013 Thomas J. Buckholtz

7Provide some details4 axes nx , ny , nz , and nt .4 p-space axes p1 , p2 , p3 , and p4 .For p4 matched with nt , 6 permutations exist.6 = 1 + 5For example, baryonic matter + dark matterMore generally, 24 permutations exist.24 = 1 + 5 + 18Baryonic matter + dark matter + dark energy8Copyright 2013 Thomas J. Buckholtz

8Provide some details< , n6 , n5 , nx , ny , nz , nt >Photon ground state - < # , 0 , -1 , -1 >Photon excited state - < # , 1 , -1 , -2 >Graviton ground state - < # , 0 , #, #, -1 , -2 >Graviton excited state - < # , 1 , #, #, -1 , -3 > 9Copyright 2013 Thomas J. Buckholtz

9Discuss possible objectionsInterpretations of cosmic microwave background (CMB) dataTimeless ratios of 1:5:18It takes time for dark-energy clumping to impact baryonic-matter photonsNegative quantum numbers for harmonic oscillatorsIn 3 dimensions, ~ r-1 . exp(-(r/)2) normalizes24 ensemblesCould be 48, but can people detect the other 24?10Copyright 2013 Thomas J. Buckholtz

10Note scope of researchScope of researchTSMHereHereList known elementary particlesyesyesExplain gravitationnoyes< # , 1 , #, #, -1 , -3 > Explain dark matternoyes5 ensemblesExplain dark energynoyes18 ensemblesExplain rate-of-expansion changesnoyes3e3 (0.5 z), 2e2 (2.3 z 0.7)Compute neutrino massnoyes 0.09161 eV/c2 Compute Higgs-like boson massno ?yes 125.325 GeV/c2Explain matter/anti-matter 1no ?yes ?Explain size of CP violationnoyes ?Provide other predictions?yes11Copyright 2013 Thomas J. Buckholtz

11Note some implicationsDark-matter beings would consider us to be part of [their] dark matter.Dark-energy beings would consider us to be part of [their] dark energy.Copyright 2013 Thomas J. Buckholtz12

12Dark MatterBosons and FermionsThomas J. Buckholtz Thomas.J.Buckholtz@gmail.com Abstract: J8.0000813Copyright 2013 Thomas J. Buckholtz

13ReferencePhysics Small and Vast: Complementing the Standard ModelCopyright 2013 Thomas J. Buckholtz14

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