String Regge trajectory on de Sitter space and implications to - - PowerPoint PPT Presentation
String Regge trajectory on de Sitter space and implications to - - PowerPoint PPT Presentation
Strings and Fields 2019 String Regge trajectory on de Sitter space and implications to inflation Siyi Zhou HKUST Stockholm U Based on arXiv: 1907.02535 [hep-th] w/Toshifumi Noumi, Toshiaki Takeuchi Outline Nave Expectation from Flat
SLIDE 1
SLIDE 2
Outline
- NaΓ―ve Expectation from Flat Space
- Regge Trajectory in dS
- High Energy Scattering
- Summary
SLIDE 3
dS in String Theory
- Maldacena-Nunez no-go theorem
- KKLT evades the no-go theorem
- Non-perturbative effects
SLIDE 4
Can we have a consistent world-sheet theory on de Sitter space?
- Higuchi bound in de Sitter space
- Modification of Regge trajectories
SLIDE 5
Higuchi Bound
- A unitarity bound on the mass of higher-spin
particles in de Sitter space
- π2 β₯ π‘ π‘ β 1 πΌ2 for bosons
- π2 β₯ π‘2 πΌ2 for fermions
- Particles with masses violating the Higuchi
bound contain helicity modes with a negative norm β Prohibited by unitarity
SLIDE 6
Linear Regge Trajectory Violates the Bound
Prohibited by Higuchi Bound Linear Regge Trajectory Violates the Bound
ππ β ππ‘
2
πΌ π‘π β ππ‘
2
πΌ2 π2 β π‘ ππ‘
2
A typical length of the string at the critical value is near the Hubble horizon scale
π βΌ ππ ππ‘ ππ‘ βΌ πΌβ1 ππ‘ βΌ 1/ππ‘
See also Lust, Palti 19
SLIDE 7
How the Regge Trajectory is modified in dS?
SLIDE 8
Rotating Folded String in Flat Space
- Centrifugal Force
- String Tension
- Balance of the two
forces requires the boundary have the speed of light
SLIDE 9
Regge Trajectory on de Sitter
- Static coordinate of de Sitter space
ππ‘2 = π2 β 1 β π 2 ππ’2 + ππ 2 1 β π 2 + π 2πΞ©2
2
- Change the variable π = sin π
ππ‘2 = π2 β cos2 πππ’2 + ππ2 + sin2ππΞ©2
2
- Wick Rotation π β βππ π’ β ππ’ π2 β βπ2
- In this way we obtain the global coordinate on
anti-de Sitter space
See also de Vega-Egusquiza '96 Gubser-Klevanov-Polyakov '02 for AdS
SLIDE 10
Rotating Folded String in dS Space
- Centrifugal Force
- String Tension
- Hubble Expansion
- Boundaries have
the speed of light
SLIDE 11
Semiclassical Rotating String
- π = ππ’
- The string Lagrangian (Nambu-Goto)
π = β4 π2 2ππ½β² ΰΆ±
π0
ππ cos2π β π2 sin2 π
- String Energy
πΉ = β4 π2 2ππ½β² ΰΆ±
π0
ππ cos2 π cos2π β π2 sin2 π
- String Spin
π = β4 π2 2ππ½β² ΰΆ±
π0
ππ π sin2 π cos2π β π2 sin2 π
See also de Vega-Egusquiza '96
SLIDE 12
Leading Regge trajectory vs Higuchi bound
π2/π½β² π2/π½β²2
SLIDE 13
Leading Regge trajectory vs Higuchi bound
- Curved space effects modify the Regge
Trajectory to make it consistent with Higuchi bound
- Existence of maximal spin on the trajectory
- The longest string touching the horizon has a
speed of light even if π = 0
- The spectrum of long strings on de Sitter is
qualitatively different from the flat space and
- AdS. The longest string has a vanishing spin and
a finite mass due to the accelerated expansion
SLIDE 14
Energy Spin Relation
π2/π½β²2 π2/π½β²
SLIDE 15
Short Strings
- The energy and spin are the same as the flat
space ones
- Linear Regge trajectory
SLIDE 16
Long Strings
- Spacetime curvature is not negligible
- Touching the horizon π0 β
π 2
- π β 0
SLIDE 17
High Energy Scattering
- In string theory, existence of an infinite higher
spin tower (the Regge tower) is crucial to make mild the high-energy behavior of scattering amplitudes and to UV complete gravity in a weakly coupled regime
- Existence of a maximum spin in the Regge
trajectory makes it nontrivial to maintain the mildness of high-energy scattering
SLIDE 18
Two Possibilities
- UV completion by the leading Regge trajectory
- UV completion by multiple Regge trajectories
SLIDE 19
UV completion: leading Regge trajectory
- In order to UV complete gravity in a weakly
coupled regime, we would need sufficiently many higher-spin states from the string scale up to near the Planck scale.
- The mass πΉβ~π/π½β²~ππ‘
2/πΌ of the maximum
spin state in the leading Regge trajectory has to be bigger than the Planck scale πΉβ > πππ
SLIDE 20
UV completion: leading Regge trajectory
- This condition implies an upper bound on the
vacuum energy of inflation π = 3πππ
2 πΌ2 < ππ‘ 4
- An upper bound on the tensor-to-scalar ratio
π = 0.01 Γ
π 1016π»ππ 4 < 0.01 ππ‘ 1016π»ππ 4
- πππ can be the Planck scale in higher
dimension, which makes the bound weaker
SLIDE 21
UV completion: multiple Regge trajectories
π2/π½β²2 π2/π½β²
N-folded closed string πΆ =1 πΆ = π πΆ = π πΆ = π ππΆ = πΆπ π»πΆ = πΆπ» ππΆ
π = πΆ Γ ππ»πΆ
π·β²
We donβt know yet if scattering amplitudes are Reggeized.
(ππΆβ
π , π»πΆβ) = (πΆπππΆβ π , πΆπ»πΆβ)
SLIDE 22
Summary
- String Regge trajectory is modified in de Sitter
space
- There exists a maximum spin for each trajectory
- Semiclassical string spectrum on de Sitter space is
consistent with the Higuchi bound
- There may exist an upper bound on tensor to
scalar ratio under some assumptions π = 0.01 Γ
π 1016π»ππ 4 < 0.01 ππ‘ 1016π»ππ 4
SLIDE 23
Next Step
SLIDE 24