fuzzy euclidean wormholes in de sitter space
TRANSCRIPT
![Page 1: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/1.jpg)
Dong-han Yeom
Fuzzy Euclidean wormholes in
de Sitter space
Leung Center for Cosmology and Particle Astrophysics, National Taiwan University
![Page 2: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/2.jpg)
Quantum cosmology
We want to understand the initial singularity
![Page 3: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/3.jpg)
Two approaches
1. The resolved initial singularity induces an effective classical
geometry, e.g., a big-bounce.
2. The resolved initial singularity becomes a wave function and
the initial condition is a superposition of various initial
conditions.
![Page 4: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/4.jpg)
Question
1. Typical interpretation of LQC corresponds a big bounce model.
2. Typical interpretation of WDW wave function, e.g., Hartle-
Hawking wave function, corresponds a superposition model.
Is there any correspondence between both pictures?
![Page 5: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/5.jpg)
In case of HH wave function
Usually interpreted by superposition
Hartle and Hertog, 2015
![Page 6: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/6.jpg)
In case of HH wave function
However, what if there is a conspiracy?
![Page 7: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/7.jpg)
Euclidean wormhole as a clue
Euclidean wormhole can give a conspiracy between a
contracting phase and a specific expanding phase
Chen, Hu and Yeom, 2016
![Page 8: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/8.jpg)
Euclidean quantum cosmology
The Hartle-Hawking wave function
minisuperspace:
eqns of motion:
![Page 9: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/9.jpg)
Classicality
Due to the analyticity, all functions can be complexified.
However, after a sufficient Lorentzian time, every
functions should be realized: classicality.
Within this classicality, we are allowed to use complex-
valued functions.
![Page 10: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/10.jpg)
Euclidean wormhole
Initial conditions (2 x 2 x 2 conditions)
![Page 11: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/11.jpg)
Euclidean wormhole
An example of the wormhole solution
![Page 12: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/12.jpg)
Euclidean wormhole
An example of the wormhole solution
poles
classicalizeddirections
![Page 13: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/13.jpg)
Euclidean wormhole
Along a certain Euclidean and Lorentzian contour
![Page 14: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/14.jpg)
Interpretations
Duality between โtwo time arrowsโ and โone time arrowโ
![Page 15: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/15.jpg)
Probability
Sometimes, more probable than the Hawking-Moss instantons
![Page 16: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/16.jpg)
Bridge between two interpretations
If we interpret this as two arrows, then it corresponds the
superposition picture.
If we interpret this as one arrow, then it corresponds the quantum
big bounce.
![Page 17: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/17.jpg)
Question 1
Can this duality between the quantum big bounce and the
superposition picture be applied for LQC?
![Page 18: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/18.jpg)
Question 2
Can this big bounce or conspiracy between the contracting and
the bouncing phase be applied for black hole cases?
![Page 19: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/19.jpg)
Euclidean path-integral
๐ ๐ = ๐โ๐๐๐ซ๐๐ซ๐๐๐๐บ path integral as a propagator
|๐โฉ =
๐
๐๐|๐๐โฉ
![Page 20: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/20.jpg)
Euclidean path-integral
๐ ๐ = ๐โ๐๐๐ซ๐๐ซ๐๐โ๐บ๐ฌ Euclidean analytic continuation
|๐โฉ =
๐
๐๐|๐๐โฉ
![Page 21: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/21.jpg)
Euclidean path-integral
๐ ๐ = ๐โ๐๐๐ซ๐๐ซ๐๐โ๐บ๐ฌ
โ ๐โ๐๐ ๐โ๐บ๐ฌ๐จ๐งโ๐ฌ๐ก๐๐ฅ๐ฅ
steepest-descent approximation
need to find/sum instantons
|๐โฉ =
๐
๐๐|๐๐โฉ
![Page 22: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/22.jpg)
Understanding black hole evolution
|๐โฉ
๐ ๐ = ๐โ๐๐๐ซ๐๐ซ๐๐โ๐บ๐ฌ
![Page 23: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/23.jpg)
Understanding black hole evolution
|๐โฉ
|๐๐โฉ๐ ๐ = ๐โ๐๐๐ซ๐๐ซ๐๐
โ๐บ๐ฌ
![Page 24: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/24.jpg)
Understanding black hole evolution
|๐โฉ
|๐๐โฉโฆ
|๐โฉ =
๐
๐๐|๐๐โฉ
๐ ๐ = ๐โ๐๐๐ซ๐๐ซ๐๐โ๐บ๐ฌ
Hartle and Hertog, 2015
|๐๐โฉ
![Page 25: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/25.jpg)
Understanding black hole evolution
|๐โฉ
|๐๐โฉโฆ
|๐๐โฉ๐ ๐ = ๐โ๐๐๐ซ๐๐ซ๐๐
โ๐บ๐ฌ
|๐โฉ =
๐
๐๐|๐๐โฉ
![Page 26: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/26.jpg)
Understanding black hole evolution
๐ ๐ โ ๐โ๐๐ ๐โ๐บ๐ฌ๐จ๐งโ๐ฌ๐ก๐๐ฅ๐ฅ
|๐โฉ
|๐๐โฉโฆ
|๐๐โฉ
Euclidean
Lorentzian
Lorentzian
|๐โฉ =
๐
๐๐|๐๐โฉ
![Page 27: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/27.jpg)
Understanding black hole evolution
|๐โฉ =
๐
๐๐|๐๐โฉ
๐ ๐ โ ๐โ๐๐ ๐โ๐บ๐ฌ๐จ๐งโ๐ฌ๐ก๐๐ฅ๐ฅ |๐๐โฉ
โฆ|๐๐โฉ
Euclidean
Lorentzian
Lorentzian
If there is a trivial geometry,
then every correlations will be recovered by
the geometry.
Information exists in the wave function.
|๐โฉ
![Page 28: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/28.jpg)
Understanding black hole evolution
๐ ๐ โ ๐โ๐๐ ๐โ๐บ๐ฌ๐จ๐งโ๐ฌ๐ก๐๐ฅ๐ฅ
|๐โฉ
|๐๐โฉIf one follows only one dominant history,
then information cannot be recovered,
though GR and local QFT can be satisfied.
โEffective loss of informationโ
![Page 29: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/29.jpg)
Asymptotic picture of LQG?
|๐โฉ
|๐๐โฉโฆ
|๐โฉ =
๐
๐๐|๐๐โฉ
|๐๐โฉ
Christodoulou, Rovelli, Speziale and Vilensky, 2016
![Page 30: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/30.jpg)
Interior picture of instantons
Christodoulou, Rovelli, Speziale and Vilensky, 2016
![Page 31: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/31.jpg)
Interior picture of instantons
In the Euclidean picture, such an instanton is not well-behaved, and hence it is not easy to give a proper tunneling rate.
However, what if there is a conspiracy? Then it can explain the internal bounce picture!
![Page 32: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/32.jpg)
Question 3
Non-unitarity of the entire universe, if there are two arrows of time.
![Page 33: Fuzzy Euclidean wormholes in de Sitter space](https://reader031.vdocuments.site/reader031/viewer/2022012504/617f77820fd23d73100d3373/html5/thumbnails/33.jpg)
Conclusion
1. There are various kind of Euclidean wormhole solutions that
may be more important than the Hawking-Moss instantons.
2. Euclidean wormholes can be interpreted both ways, either
quantum big bounce (one arrow) or superposition (two
arrows).
3. If this โdualityโ of time arrows are very fundamental, then it will
have very profound implications.