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The CMB anomalies The CMB anomalies with with a bouncing inflation a bouncing inflation 朴朴朴朴朴朴Y.S. Pi Y.S. Pi ao ao

The CMB anomalies with a bouncing inflation

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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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Page 1: The CMB anomalies                        with a bouncing inflation

The CMB anomaliesThe CMB anomalies

with a bouncing inflation with a bouncing inflation

朴云松(朴云松( Y.S. PiaoY.S. Piao ))

Page 2: The CMB anomalies                        with a bouncing inflation

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

Page 3: The CMB anomalies                        with a bouncing inflation

I. The motivation

Inflation is the current paradigm of early universe.

Page 4: The CMB anomalies                        with a bouncing inflation

I. The motivation

The Planck’s results No Non-GaussiangityNo running

Page 5: The CMB anomalies                        with a bouncing inflation

The Planck’s results

I. The motivation

Page 6: The CMB anomalies                        with a bouncing inflation

I. The motivation

The Planck confirmed1. deficit of power on large angular scales

Page 7: The CMB anomalies                        with a bouncing inflation

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

Page 8: The CMB anomalies                        with a bouncing inflation

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.

Page 9: The CMB anomalies                        with a bouncing inflation

/lsx l

Dipole modulation

The CMB power asymmetry may be modeled as a dipole modulation of power.

kA

Erickcek et.alLyth,fluctuation mode

Page 10: The CMB anomalies                        with a bouncing inflation

Dipole modulation

The modulation can be explained in light of

kA

Lyth, Liu, Guo, Piao

/lsx l

Page 11: The CMB anomalies                        with a bouncing inflation

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.

Page 12: The CMB anomalies                        with a bouncing inflation

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

Page 13: The CMB anomalies                        with a bouncing inflation

III. Our model

Ten years ago

Page 14: The CMB anomalies                        with a bouncing inflation

Ten years ago

Page 15: The CMB anomalies                        with a bouncing inflation

III. Our model

Page 16: The CMB anomalies                        with a bouncing inflation

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.

Page 17: The CMB anomalies                        with a bouncing inflation

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.

Page 18: The CMB anomalies                        with a bouncing inflation

III. Our model

The evolution of background (numerical)

Page 19: The CMB anomalies                        with a bouncing inflation

III. Our model

The evolution of background is approximately

is the comoving Hubble scale at matching surface

Page 20: The CMB anomalies                        with a bouncing inflation

III. Our model

The equation of is

where is defined,

Page 21: The CMB anomalies                        with a bouncing inflation

III. Our model

In the contracting phase

In the inflationary phase

Page 22: The CMB anomalies                        with a bouncing inflation

III. Our model

all physical quantities should continuously pass through the bounce.

Liu, Piao, Phys.Rev.D86, 083510 (2012)

Page 23: The CMB anomalies                        with a bouncing inflation

III. Our model

Thus the continuity of brings

Page 24: The CMB anomalies                        with a bouncing inflation

III. Our model

Page 25: The CMB anomalies                        with a bouncing inflation

III. Our model

Page 26: The CMB anomalies                        with a bouncing inflation

III. Our model

Planck used cutoff model Our model

Page 27: The CMB anomalies                        with a bouncing inflation

III. Our model

Page 28: The CMB anomalies                        with a bouncing inflation

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.

Page 29: The CMB anomalies                        with a bouncing inflation

IV. Conclusion

The anomalies appeared simultaneously is not accidental, which is a significant hint of

Pre-inflationary physics.

the string theory ?

Page 30: The CMB anomalies                        with a bouncing inflation

Thank You!