Aspects of holographic axion dynamics Yuta Hamada (Harvard) - - PowerPoint PPT Presentation

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Aspects of holographic axion dynamics Yuta Hamada (Harvard) - - PowerPoint PPT Presentation

Aspects of holographic axion dynamics Yuta Hamada (Harvard) 1905.03663, 2001.05510 and 2007.13535, with Elias Kiritsis (APC&Crete), Francesco Nitti (APC), and Lukas T. Witkowski (IAP) 1 2020/11/18 Strings and Fields 2020 2 Axion


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Aspects of holographic axion dynamics

Yuta Hamada (Harvard)

1905.03663, 2001.05510 and 2007.13535, with Elias Kiritsis (APC&Crete), Francesco Nitti (APC), and Lukas T. Witkowski (IAP)

2020/11/18 Strings and Fields 2020

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Axion

Ubiquitous in field theory and string theory. In the context of particle physics, roles of axion are


  • Inflaton candidate

  • Solution of strong CP problem.
  • Dark Matter candidate

2

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Axion

Ubiquitous in field theory and string theory. In the context of particle physics, roles of axion are


  • Inflaton candidate

  • Solution of strong CP problem.
  • Dark Matter candidate

2

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SLIDE 4

Axion Monodromy

String theory setup (flux, brane) for axion monodromy inflation.

[(McAllister-)Silverstein-Westphal ’08, Kaloper-Sorbo ‘08]

Field theory [Witten ’80], Holography [Witten ’98]

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There are many branches 
 parametrized by integer .

k

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SLIDE 5

Axion Backreaction

In the context of axion monodromy inflation, 
 large field excursion is typically needed. Is there effect of axion backreacion? Result: 
 We find that there exists a significant backreaction 
 when the field excursion is order of the Planck scale.

4

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SLIDE 6

Axion

Ubiquitous in field theory and string theory.

5

In the context of particle physics, roles of axion are


  • Inflaton candidate

  • Solution of strong CP problem.
  • Dark Matter candidate
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SLIDE 7

Axion

Ubiquitous in field theory and string theory.

5

In the context of particle physics, roles of axion are


  • Inflaton candidate

  • Solution of strong CP problem.
  • Dark Matter candidate
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SLIDE 8

Strong CP problem

ℒ ∼ − FμνFμν + θ Fμν ˜ Fμν

Experimental constraint is .

θ ≲ 10−9

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An explanation is given by QCD axion , whose Lagrangian is

a ℒ ∼ (∂μa)2 − FμνFμν + a fa Fμν ˜ Fμν

EOM for axion requires .

δaZ ∼ ⟨Fμν ˜ Fμν⟩ = 0 θ = 0

QCD Lagrangian is

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Strong CP problem?

Dynamical solution to Strong CP? It is possible that term receives finite renormalization. A speculation: -angle flows to zero in the IR, and strong CP- problem is alleviated.

θ θ

[Knizhnik-Morozov ’84, Levine-Libbt ’85, Latorre-Luken ’97, Nakamura-Schierholz, ’19]

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Holography

Similar observation is obtained in holography. Bulk axion becomes zero in the IR. → The -angle flows to zero.

θ

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Since the IR theta angle itself is not observable, the physical meaning is not clear. We compute CP-violating interaction among glueballs, and see if these couplings are

  • suppressed. 


Result: We do not see the suppression, which implies strong CP problem remains.

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SLIDE 11

Talk Plan

  • 1. Introduction and results
  • 2. Setup: Axion-Dilaton-Einstein theory
  • 3. Axion backreaction
  • 4. Strong CP-violation

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SLIDE 12

Talk Plan

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  • 1. Introduction and results
  • 2. Setup: Axion-Dilaton-Einstein theory
  • 3. Axion backreaction
  • 4. Strong CP-violation
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SLIDE 13

Setup

Ansatz

Sbulk = M3

5 ∫ d5x

−g [R − 1 2 gab∂aφ∂bφ − 1 2Y(φ)gab∂aa∂ba − V(φ)] + SGHY

Axion kinetic term

11

Boundary term 5d Ricci scalar 5d Planck mass

We use a bottom up holography model. 5d Axion-Dilaton-Einstein theory, 
 ( and RG coordinate ).

xμ r

ds2 = e2A(r) (dr2 + ημνdxμdxν), φ = φ(r), a = a(r)

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SLIDE 14

UV and IR

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IR: , , is either finite or infinity. IR is singular, but is expected to be resolved, e.g. by adding KK modes. (Good singularity)

eA → 0 φ → ∞ r → rIR rIR

UV: Asymptotically , , .

AdS5 eA → ∞ φ → 0 r → 0

: 4d energy scale

eA(r)

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SLIDE 15

Correspondence

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dilaton

φ

axion

a

metric

gμν

energy momentum tensor

Tμν

, is field strength

Tr[FμνFμν] Fμν

: instanton density

Tr[Fμν ˜ Fμν]

dual 4d operator Bulk field

Near-boundary ( ) solution: 
 ,

r → 0 a(r) = aUV + Q r4 + . . . aUV = θ + 2πk Nc Q ∼ ⟨Fμν ˜ Fμν⟩

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SLIDE 16

IR axion boundary

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In the IR, we put .

aIR = 0

Support: The axion is a form field component along an internal cycle, 
 which shrinks to zero-size in the IR. Single-valuedness then demands that the axion field vanishes at such points.

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SLIDE 17

Talk Plan

  • 1. Introduction and results
  • 2. Setup: Axion-Dilaton-Einstein theory
  • 3. Axion backreaction
  • 4. Strong CP-violation

15

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SLIDE 18

Numerical Analysis

Sbulk = M3

5 ∫ d5x

−g [R − 1 2 gab∂aφ∂bφ − 1 2Y(φ)gab∂aa∂ba − V(φ)] + SGHY

Choose and (next slide).

V(φ) Y(φ)

Compute RG flow solutions with given ansatz and IR b.c, scanning over for all possible values for axion source .

aUV

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Parametrizing IR

Take model such that in the IR:

φ → ∞, V(φ) ≃ − V∞ebφφP, Y(φ) ≃ Y∞e

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Two classes of potentials: 1: Steep


  • r

, 


  • finite. Glueball spectra

2: Soft

, . . Glueball spectra

b > 2/3, arbitrary P b = 2/3 1 < P rIR m2

n ∼ n2

b = 2/3 0 < P < 1 rIR = + ∞ m2

n ∼ n2P

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SLIDE 20

is bounded aUV

In the probe approximation, any value of is possible. Backreaction → range of becomes bounded.

aUV aUV

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UV IR UV IR

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Analytical Results

There are no regular RG flow solutions satisfying the boundary conditions with .

|aUV| > amax

UV

This can be understood analytically:
 Using the EOMs, one can show that . is the function which appears in axion kinetic term.

|aUV| ≤ ∫

IR UV

dφ Y Y

String-inspired choice is , which leads


Y = e

|aUV| ≤ 2/ 6 ∼ 𝒫(1)

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SLIDE 22

Implication

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SLIDE 23

Implication

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Implication

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Implication

Constraints on large field excursion. This is reminiscent of swampland distance conjecture [Ooguri-Vafa ’06].

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SLIDE 26

Implication

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Implication

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Swampland distance conjecture When field excursion is large, the tower of particle becomes light. Original EFT breaks down. We may need to go another EFT.

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SLIDE 28

Connection to WGC?

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Similar story for axion? In this case, charged object is instanton rather than particle. 
 Axion version of WGC? [work in progress] [Horowitz-Santos ’19] observes similar bound on large gauge field source in Maxwell theory. 
 However, they found if there exists scalar field which satisfies (charge) > (mass), then the singularity disappears by condensation. This is nothing but Weak Gravity Conjecture (WGC).

[ArkaniHamed-Motl-Nicolis-Vafa ‘06]

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SLIDE 29

Talk Plan

  • 1. Introduction and results
  • 2. Setup: Axion-Dilaton-Einstein theory
  • 3. Axion backreaction
  • 4. Strong CP-violation

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SLIDE 30

Flow of -angle θ

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  • angle becomes zero in the IR, as we required. 


What does this mean in physics?

θ

UV IR UV IR

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Glueballs spectra

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We compute wavefunctions and spectra of glueballs. Masses are decreasing functions of . Qualitatively consistent with lattice result. [Del-Debbio et. al. ’10]

θ

(glueball) = Normalizable linearized fluctuations. 
 Roughly speaking, 
 (Dilaton fluctuation) = glueball, (Axion fluctuation) = glueball, (Metric fluctuation) = glueball.
 Solutions of eigenvalue problem give spectra.

0++ 0−+ 2++

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SLIDE 32

Glueballs interaction

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Glueball cubic couplings are obtained by looking terms third order in gauge- invariant fluctuations. Expand the fluctuation by using wavefucntion of glueball. 
 Cubic interactions among glueballs are

  • btained by overlap integration.

CP conserving: (even)-(even)-(even) interaction, … CP violating: (even)-(even)-(odd), (odd)-(odd)-(odd) interaction

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SLIDE 33

CP-violating interaction

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CP-violating couplings are not suppressed. Blue: (odd-odd-odd)/(even-even-even) Red: (odd-even-even)/(even-even-even)

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SLIDE 34

Summary

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We investigated the dynamics of axion 
 by using bottom up holography model. We find


  • significant backreaction for trans-

Planckian field excursion.


  • although -angle flows to 0 in IR,

the suppression of CP-violating effect is not seen in physical observable.

θ