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The CMB anomalies with a bouncing inflation. 朴云松( Y.S. Piao ). I. The motivation: CMB anomalies II. Our viewpoint: CMB anomalies is a hint of preinflationary physics III. Our model Based on collaboration with Guo and Liu - PowerPoint PPT Presentation
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The CMB anomaliesThe CMB anomalies
with a bouncing inflation with a bouncing inflation
朴云松(朴云松( Y.S. PiaoY.S. Piao ))
I. The motivation: CMB anomalies
II. Our viewpoint: CMB anomalies is a hint of preinflationary physics
III. Our model
Based on collaboration with Guo and Liu
arXiv:1304.6527
I. The motivation
Inflation is the current paradigm of early universe.
I. The motivation
The Planck’s results No Non-GaussiangityNo running
The Planck’s results
I. The motivation
I. The motivation
The Planck confirmed1. deficit of power on large angular scales
I. The motivation
The Planck confirmed2. power asymmetry on large angular scales
ˆ ˆ ˆ ˆ T n =s n 1+A n p
Dipole modulation
0.07 0.02 A
II. Our viewpoint
Why both the deficit of power and the power asymmetry appeared simultaneously on large angular scales ?
We think this is not accidental.
/lsx l
Dipole modulation
The CMB power asymmetry may be modeled as a dipole modulation of power.
kA
Erickcek et.alLyth,fluctuation mode
Dipole modulation
The modulation can be explained in light of
kA
Lyth, Liu, Guo, Piao
/lsx l
Dipole modulation
is determined by the observation on corresponding scales
The result is < 0.1
Erickcek et.alLyth,Thus for single inflation model
310kA
which is not consistent with Planck data.
II. Our viewpoint
We think: both the large modulation and the deficit of power implies on large angular scales
the anomalies on large angular scales is a hint of the preinflationary physics.
1 1 Rn k
III. Our model
Ten years ago
Ten years ago
III. Our model
III. The bounce model
Before 03, modified gravity Pre-big bang, ekpyrotic universe After 03, GR and field breaking null energy condition Ghostfree models ghost condensation (new ekpyrotic universe), G-bounce
a
t
Any of these mechanisms may apply to our model, the result is not affected, since the bounce does not alter the spectrum of primordial perturbation.
III. Our model
before the bounce, the field will climb up along its potential.
after the bounce, It rolls down.
The scenario: initially the universe is in a contracting phase, then it bounces into a slowroll inflationary phase.
III. Our model
The evolution of background (numerical)
III. Our model
The evolution of background is approximately
is the comoving Hubble scale at matching surface
III. Our model
The equation of is
where is defined,
III. Our model
In the contracting phase
In the inflationary phase
III. Our model
all physical quantities should continuously pass through the bounce.
Liu, Piao, Phys.Rev.D86, 083510 (2012)
III. Our model
Thus the continuity of brings
III. Our model
III. Our model
III. Our model
Planck used cutoff model Our model
III. Our model
III. Our model
The implication to the eternal inflation scenario in landscape
the bouncing inflation is a favored channel to implement the slow roll inflation.
IV. Conclusion
The anomalies appeared simultaneously is not accidental, which is a significant hint of
Pre-inflationary physics.
the string theory ?
Thank You!