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Jong-Phil Lee Yonsei Univ. 16 Nov 2010, Yonsei Univ. Based on JPL, 1009.1730; 0911.5382;0901.1020
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2 Unparticles Brief Flat higher dim’l deconstruction Ungravity Fractional eXtra Dimension (FXD) Unparticle and Bs-anti Bs Conclusions
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4 H. Georgi, PRL98; PLB650 SM Sector Scale Inv. Sector Weakly interacting Particles with definite masses NO particles With definite nonzero masses Unparticle!
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5 energy MUMU UU BZ SM Dimensional transmutation Scale inv. emerges. MWMW ; EWSB ; scale inv. breaking Banks-Zaks( BZ ) Theory Massless fermionic gauge theory With an infrared-stable fixed point. matching
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6 Production Cross Section Phase Space
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7 Two-point function Spectral density function Fixed by scale inv. Normalization factor Unparticles with d U look like a Non-integral number of massless particles.
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8 Grinstein, Intriligator, Rothstein, PLB662 Cheung, Keung, Yuan, PRD76 Scalar Unparticle Propagator Vector Unparticle Propagator
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9 Fox, Rajaraman, Shirman,, PRD76 scale invariance breaking “Good Correspondence” 0 : U reduces to the usual Unparticle spectral function d U 1 : the corresponding propagator is a free particle propagator of mass m.
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10 Interaction Lagrangian Phase spaces
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13 Stephanov, PRD76 Philosophy lim S 0 Unparticle s particles with mass gap continuous sum for unparticles
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14 Assume that the scale invariance is slightly broken; continuous ldiscrete l In general, Matching in the limit D-->0 Spectral function Propagator
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15 Massless field Lagrangian in 4+d dim Kk mode expansion
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16 JPL, PRD 79 Massive Lagrangian Massive propagator
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19 Goldberg & Nath, PRL 100 Newtonian gravity modified Tensor unparticle interaction
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20 Basic Idea lim S 0 Unparticle particle s with mass gap KK sum over Extra dim. 2d U - 1 N+1
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21 Ungravity Lagrangian Spectral Function Two-Point Function
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22 Ungravity Propagator Tensor Structure Grinstein, Intriligator, Rothstein, PLB662
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23 for massive graviton Tensor Operator Decomposed Matching Tensor Structure for Deconstructed states Deconstructed Ungravity (polarization tensor) JPL, 0911.5382
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24 Arkani-Hamed et al., PRL 84 AdS(4+N) metric KK Decomposition Reparametrizaion for which
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25 Newtonian Potential
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27 (4+N)-dim’l Gravity Proposition JPL, 0911.5382
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28 Intermediate States Have Vanishing Mass? Does Fn Satisfy the Matching Condition? Newtonian Potential Modification For large L>>r
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30 Schwarzschild radius Schwarzschild metric Newtonian gravity modified Geometric BH cross section ~10 -5 fm for typical parameters Mureika, PLB660
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31 Mureika, Spallucci arXiv:1006.4556 (Bm : baryon current) Vector Unparticle Interaction “repulsive contribution”
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32 Extremal Condition (1)M>Me : Massive object. Two-horizon BH. (2)M=Me : Critical object. Single horizon. Extremal BH. (3)M<Me : “naked-singularity” Horizons As M goes down, the two horizons approach to each other. Inner & outer Horizons exist.
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33 cf) Hawking temp. for Schwarzschild BH in D-dim Weak coupling phase Strong coupling phase
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34 Ask, EPJC(2009)60 Invariant mass spectrum of U Dense KK tower of large XD
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37 Scalar and vector unparticle couplings s- and t-channel contribution at tree level
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40 Unitarity constraint In the literature, people usually put d S =d V But this is NOT true. f S is suppressed by a factor of f V is suppressed by
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41 suppressed positive definite cf) Unparticles cannot explain the positive f s D
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42 JPL, 1009.1730
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43 degree
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44 Unparticles of spin 2 produce ungravity. Ungravity modifies the Newtonian gravitational potential. Ungravity physics is realized in AdS(4+N)-dim’l gravity. Ungravity can be understood in the context of fractional extra dimensions. Scalar unparticles contribute predominantly to the Bs-(anti Bs) mixing, and can naturally explain its negative phase. The LHC might see evidences of unparticles.
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2010 LHC Workshop @ Korea (Konkuk Univ) Jong-Phil Lee(Yonsei Univ.) 46 1234567890-= qwertyuiop[]\ asdfghjkl;’ zxcvbnm,./` !@#$%^&*()_+ QWERTYUIOP{}| ASDFGHJKL:” ZXCVBNM<>?~
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2010 LHC Workshop @ Korea (Konkuk Univ) Jong-Phil Lee(Yonsei Univ.) 47 D 0000 and D 00 have opposite sign: D 0000 ~(-h 00 ) 2 ; D 00 ~-h 00
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