Generalized solution for RS metric and LHC phenomenology Alexander Kisselev IHEP, NRC “Kurchatov Institute”, Protvino, Russia The Third Annual Conference.

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Presentation transcript:

Generalized solution for RS metric and LHC phenomenology Alexander Kisselev IHEP, NRC “Kurchatov Institute”, Protvino, Russia The Third Annual Conference on Large Hadron Collider Physics (LHCP2015) St. Petersburg, Russia, September 2, 2015

Plan of the talk  Randall-Sundrum scenario with two branes. Original RS solution  Generalization of RS solution  Solution with explicit orbifold symmetries  Role of constant term. Different physical schemes  Dilepton production at LHC in RS-like scenario  Conclusions 2 LHCP2015, St. Petersburg, Russia, September 2, 2015

Randall-Sundrum scenario Randall-Sundrum scenario Periodicity: (x, y ± 2πr c ) = (x, y) Z 2 -symmetry: (x, y) = (x, –y) Background metric (y is extra coordinate) orbifold S 1 /Z 2 0 ≤ y ≤ πr c Two fixed points: y=0 and y= πr c two (1+3)-dimensional branes 3 LHCP2015, St. Petersburg, Russia, September 2, 2015 warp factor

5-dimensional action Einstein-Hilbert’s equations: 4 LHCP2015, St. Petersburg, Russia, September 2, 2015 (brane terms) (gravity term)

(Randall & Sundrum, 1999) The RS solution: -does not explicitly reproduce the jump of derivative on TeV brane (at y=πr c ) - is not symmetric with respect to both branes (located at y=0 and y=πr c ) - does not include a constant term Original Randall-Sundrum solution Original Randall-Sundrum solution 5 LHCP2015, St. Petersburg, Russia, September 2, 2015

σ(y)+ C y 2πr c -πr c 0 πr c κπr c Two equivalent solutions related to different branes 6 LHCP2015, St. Petersburg, Russia, September 2, 2015 Generalization of RS solution

7 LHCP2015, St. Petersburg, Russia, September 2, 2015 with fine tuning (0 ≤ C ≤ κπr c ) 1-st derivative of σ(y) Generalized solution 2-nd derivative of σ(y) factor of 2 different than that of RS

8 LHCP2015, St. Petersburg, Russia, September 2, 2015 Explicit account of periodicity and Z 2 -symmetry Solution for the warp function in variable Arccos(z) is principal value of inverse cosine Arccos(cos x) = { x - 2nπ, 2nπ ≤ x ≤ (2n+1)π -x + 2(n+1)π, (2n+1)π ≤ x ≤ 2(n+1)π In particular, σ(y) = κy for 0 ≤ y ≤ πr c (see, for instance, Gradshteyn &Ryzhik ) (A.K., 2015)

(y ≠ πnr c, n = 0, ±1, ±2, …) 9 LHCP2015, St. Petersburg, Russia, September 2, st derivative of σ(y): 2-nd derivative of σ(y): (periodicity) (Z 2 symmetry) Orbifold symmetries:

Hierarchy relation Interaction Lagrangian (massive gravitons only) 10 LHCP2015, St. Petersburg, Russia, September 2, 2015 Different values of C result in quite diverse physical models Masses of KK gravitons m n and coupling Λ π depend on C via M 5 and κ Masses of KK gravitons (x n are zeros of J 1 (x))

I. C = 0 that requires Masses of KK resonances RS1 model Graviton spectrum - heavy resonances, with the lightest one above 1 TeV ( Randall & Sundrum, 1999) Different physical scenarios Different physical scenarios 11 LHCP2015, St. Petersburg, Russia, September 2, 2015

II. C = κπr c Masses of KK resonances RSSC model: scenario with small curvature of 5-dimensional space-time For small κ, graviton spectrum is similar to that of the ADD model (Giudice, 2005 Petrov & A.K., 2005) 12 LHCP2015, St. Petersburg, Russia, September 2, 2015

III. C = κπr c /2 13 LHCP2015, St. Petersburg, Russia, September 2, 2015 Masses of gravitons Let Almost continuous spectrum of KK gravitons ( A.K., 2015) “symmetric” scheme

Virtual Gravitons at the LHC pp-collisions at LHC mediated by KK graviton exchange in s-channel Processes: Sub-processes: h (n) Σ n≥1 14 LHCP2015, St. Petersburg, Russia, September 2, 2015 KK gravitons

where Tensor part of graviton propagator Energy-momentum tensors Matrix element of sub-process and Graviton widths (process independent) 15 LHCP2015, St. Petersburg, Russia, September 2, 2015

16 LHCP2015, St. Petersburg, Russia, September 2, 2015 Dilepton production at LHC in scenario with small curvature Dilepton production at LHC in scenario with small curvature Number of events with p t > p t cut Interference (SM-gravity) contribution is negligible Statistical significance Scenario II (C = κπr c )

No deviations from the CM were seen at the LHC M 5 > 6.4 TeV for TeV, L = 5 fb fb -1 M 5 > 9.0 TeV for 13 TeV, L = 30 fb LHCP2015, St. Petersburg, Russia, September 2, 2015 Week dependence of limits on parameter κ (p t cut = 200 GeV) LHC search limits on M 5

with For chosen values of parameters TeV physics at LHC energies Scenario III (C = κπr c /2) (relation of m n with x n was used) 18 LHCP2015, St. Petersburg, Russia, September 2, 2015

 Generalized solution for metric in RS-like scenario is derived  This solution σ(y): - is symmetric with respect to the branes - has the jumps of its derivative on both branes - is consistent with the orbifold symmetries - depends on constant C (0 ≤ C ≤ κπr c )  Different values of C result in quite diverse physical scenarios: RS1, RSSC, “symmetric” models 19 LHCP2015, St. Petersburg, Russia, September 2, 2015 ConclusionsConclusions

20 LHCP2015, St. Petersburg, Russia, September 2, 2015  All these schemes lead to TeV physics at LHC, but with different experimental signatures  LHC limits on gravity scale M 5 are obtained in RS-like scheme with small curvature Conclusions (continued)

21 LHCP2015, St. Petersburg, Russia, September 2, 2015 Thank you for your attention

Back-up slides 22 LHCP2015, St. Petersburg, Russia, September 2, 2015

23 LHCP2015, St. Petersburg, Russia, September 2, 2015 ADD model : M D > 4 TeV (for n ED = 4)real graviton production M S > 7 TeV (for n ED = 4) (HLZ convention) virtual graviton exchange (CMS, PLB 746 (2015) 79) (CMS, EPJC 75 (2015) 235) RS model : m G* > 2.7 TeV (for κ/M Pl = 0.1 ) (ATLAS, PRD 90 (2014) ) Extra dimensions: LHC limits

24 LHCP2015, St. Petersburg, Russia, September 2, 2015 Pseudorapidity cuts: |η| ≤ 2.4 (muons) |η| ≤ 1.44, 1.57 ≤ |η| ≤ 2.4 (electrons) Efficiency: 85 % K-factor: 1.5 for SM background 1.0 for signal Dilepton production

Uncertainties in search limit (L = 30 fb -1 ) Uncertainties in search limit (L = 30 fb -1 ) PDF set (2.7%) ΔL (3%) μ/2 →μ→2μ

Statistical significance in RSSC for pp → e + e - + X as a function of 5-dimensional reduced Planck scale M 5 and cut on electron transverse momentum p t cut for 7 TeV (L=5 fb -1 ) and 8 TeV (L=20 fb -1 ) 26 LHCP2015, St. Petersburg, Russia, September 2, 2015

27 LHCP2015, St. Petersburg, Russia, September 2, 2015 Statistical significance for the process pp → e + e - + X as a function of 5-dimensional reduced Planck scale M 5 and cut on electron transverse momentum p t cut for 13 TeV (L=30 fb -1 )

Graviton contributions in RSSC to the process pp → μ+μ- + X (solid lines) vs. SM contribution (dashed line) for 7 TeV 28 LHCP2015, St. Petersburg, Russia, September 2, 2015

Graviton contributions in RSSC to the process pp → μ+μ- + X (solid lines) vs. SM contribution (dashed line) for 14 TeV 29 LHCP2015, St. Petersburg, Russia, September 2, 2015

30 LHCP2015, St. Petersburg, Russia, September 2, Weak logarithmic dependence on energy comes from PDFs dσ(grav): week dependence on curvature κ (for fixed x ┴ )

31 LHCP2015, St. Petersburg, Russia, September 2, 2015 dσ(pp →h (n) →γγ ) = 2 ∙ dσ(pp →h (n) →l + l - ) universal for all subprocesses while in SM:

Effective gravity action Shift is equivalent to the change Invariance of the action rescaling of fields and masses: Massive theory is not scale-invariant From the point of view of 4- dimensional observer these two theories are not physically equivalent 32 LHCP2015, St. Petersburg, Russia, September 2, 2015

Randall-Sundrum solution Does it mean that σ RS (y) is a linear function for all y? The answer is negative: one must use the periodicity condition first, and only then estimate absolute value |y| In other words, extra coordinate y must be reduced to the interval -πr c ≤ y ≤ πr c (by using periodicity condition) before evaluating functions |x|, ε(x), … 33 LHCP2015, St. Petersburg, Russia, September 2, 2015

Examples: definition of σ(y) outside interval |y| ≤ πr c Let y = πr c + y 0, where 0 < y 0 < πr c (that is, πr c < y < 2πr c ) σ(y)+ C 2πr c 0πr c κπr c y κ(πr c - y 0 ) πr c + y 0 34 LHCP2015, St. Petersburg, Russia, September 2, 2015

RSSC model is not equivalent to the ADD model with one ED of size R=(πκ) -1 up to κ ≈ eV Hierarchy relation for small κ But the inequality means that RSSC model vs.ADD model 35 LHCP2015, St. Petersburg, Russia, September 2, 2015

36 LHCP2015, St. Petersburg, Russia, September 2, 2015 where (A.K, 2006) 36

37 LHCP2015, St. Petersburg, Russia, September 2,