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Minimal theory of quasidilaton massive gravity GC2018, 18.02.06 - PowerPoint PPT Presentation

1 /17 Minimal theory of quasidilaton massive gravity GC2018, 18.02.06 M. Oliosi (YITP) Based on 2 /17 Minimal theory of quasidilaton massive gravity arXiv 1701.01581, with A. De Felice and S. Mukohyama Horndeski extension of the minimal


  1. 1 /17 Minimal theory of quasidilaton massive gravity GC2018, 18.02.06 M. Oliosi (YITP)

  2. Based on 2 /17 Minimal theory of quasidilaton massive gravity arXiv 1701.01581, with A. De Felice and S. Mukohyama Horndeski extension of the minimal theory of quasidilaton massive gravity arXiv 1709.03108, with A. De Felice and S. Mukohyama

  3. Outline 3 /17 Overview, motivations 1. Construction 2. From dRGT… i. …via the precursor theory… ii. …to the minimal quasidilaton iii. Solutions and some cosmology 3. Future prospects 4.

  4. Minimal quasidilaton – overview 4 /17  2 massive tensor modes + 1 scalar  Free of Boulware-Deser ghost  Quasidilatation global symmetry  Breaks Lorentz invariance (LI) to propagate 3 instead of 6 expected d.o.f.  Modifies gravity at cosmological scales Graviton mass:

  5. Motivations 5 /17  IR modification of gravity  Explore viable massive gravity theories Why the minimal quasidilaton? see e.g. Gümrükçüoglu Some advantages: et al. arXiv:1707.02004 From the point of view of quasidilaton theories , this has the I. least number of degrees of freedom , and thus is more tractable. In contrast to the MTMG , the minimal quasidilaton theory II. allows to use a Minkowski fiducial metric MTMG in De Felice et Passes the LIGO/Virgo tests III. al. arXiv:1506.01594

  6. Construction 6 /17 i. Start from dRGT massive gravity ii. Break LI and add the quasidilaton. iii. Switch to Hamiltonian and analyse “ à la Dirac” iv. Add constraints so that the final number of degrees of freedom is 3 “ à la MTMG ”. v. This defines the minimal theory.

  7. dRGT theory (arXiv:1011.1232) 7 /17 de Rham, Gabadadze, Contract the physical metric 𝑕 𝜈𝜉 Tolley with a new fiducial metric 𝑔 𝜈𝜉 Thanks to the special form of the potential, no Boulware-Deser ghost . Propagates 5 d.o.f.

  8. Quasidilaton (D’ Amico et al. arXiv 1206.4253) 8 /17 The Stückelberg scalar fields 𝜚 𝑏 can be introduced to recover covariance e.g. for Minkowski fiduciual metric Choose: Stückelberg sector is shift- and SO(3) symmetric. Add an additional global symmetry in the action. It acts on the Stückelberg fields as quasidilaton scalar! LI breaking

  9. LI breaking potential 9 /17 (De Felice & Mukohyama, arXiv 1506.01594) Use ADM decomposition And ADM Vierbein … as in MTMG ! The resulting potential:

  10. Precursor action 10 /17 Defining a precursor action is the first step in constructing the minimal theory. Auxiliary fields 𝑌 , 𝑇 , 𝜓 , 𝜄 We can include a cubic Horndeski 𝐺 𝑌, 𝑇 = 𝑄 𝑌 − 𝐻 𝑌 𝑇 structure ! 𝔜 = − 1 2 𝑕 𝜈𝜉 𝜖 𝜈 𝜏𝜖 𝜉 𝜏

  11. Degrees of freedom in the precursor theory 11 /17 Linear in 𝑂 , 𝑂 𝑗 , and 𝑁 11 d.o.f. 𝜓 𝛿 𝑗𝑘 𝑌 𝜏 𝜄 𝑇 (22 phase space d.o.f.) 1 first-class and 12 second-class constraints (8 phase space d.o.f.) 4 d.o.f.

  12. Minimal theory: new constraints 12 /17 We replace 2 Careful about precursor constraints keeping SO(3) by 4 new constraints (8 phase space d.o.f.) 4 d.o.f. 2 second-class constraints (6 phase space d.o.f.) 3 d.o.f. [In practice, 2 tensor modes and the quasidilaton 𝜏 ]

  13. Minimal theory, action 13 /17 There are still some Lagrange multipliers 𝜇 , 𝜇 𝑈 Luckily there is a unique mini-superspace solution: 𝜇 = 𝜇 𝑈 = 0

  14. Mini-superspace solutions 14 /17 de Sitter attractor The equation from 𝜇 is rewritten in a nice form. where 𝑏 is the scale factor. This implies that there exists a de Sitter attractor where either 𝒴 is constant ( α = −4 ) or 𝐾 𝒴 = 0 ( α ≠ −4 ). Stability of de Sitter solution Study the quadratic action for linear perturbations, and obtain the no-ghost conditions. It is nice and stable ! ☺

  15. Gravitational modes in the 15 /17 minimal quasidilaton Constraints GW 150914 GW170817/GRB170817A The minimal theory of quasidilaton massive gravity successfully passes the tests of both GW and multimessenger detections. - The sound speed of the tensor modes in the subhorizon limit coincides with the speed of light . - Small graviton mass of order 𝐼 0 ~10 −33 𝑓𝑊 .

  16. Future prospects 16 /17 i. Cosmology with matter and general FLRW. ii. Small scale behaviour – Vainshtein screening and astrophysics iii. Minimal… other theories iv. Theoretical consistency checks …keep in touch! ☺

  17. 17 /17 Thank you for your attention !

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