application for joining data analysis group in kagra

16
Application for joining Data Analysis Group in KAGRA Dongfeng Gao Wuhan Institute of Physics and Mathematics (WIPM) Chinese Academy of Sciences (CAS) August 23, 2018

Upload: others

Post on 02-Feb-2022

2 views

Category:

Documents


0 download

TRANSCRIPT

Page 1: Application for joining Data Analysis Group in KAGRA

Application for joining Data Analysis Group in KAGRA

Dongfeng GaoWuhan Institute of Physics and Mathematics (WIPM)

Chinese Academy of Sciences (CAS)

August 23, 2018

Page 2: Application for joining Data Analysis Group in KAGRA

Overall description of Research Unit

2

• Unit leader (Full name, current position, email address)

Dongfeng Gao, Associate professor, [email protected]

• Affiliation of unit leader(If the unit leader is not a faculty member (a tenure track assistant professor or above ), please write down the reason to submit as a unit leader) Wuhan Institute of Physics and Mathematics, Chinese Academy of SciencesWest No. 30 Xiao Hong Shan, Wuhan 430071, China

• Members (Full Name, current position, email address, roles)

1. Dongfeng GaoAssociate professor, [email protected], unit leader

2. Gang WangPostdoc fellow, [email protected], working on the gravitational-wave parameter estimation

3. Wei ZhaoPhD student, [email protected], working on the gravitational effects in atomic physics

Page 3: Application for joining Data Analysis Group in KAGRA

3

• Working groups CBC

• Research plan: Working group: CBCProject: Test of General Relativity

Description of research: In WIPM, many efforts are put on testing the weak equivalenceprinciple (WEP), which is the foundation of General Relativity. The basic idea is to launchtwo atomic species in a 10-meter-high atom interferometer, and compare their accelerationsdue to the Earth’s gravity. We are working on to improve the WEP test to the 10-10 level.

To push the “Test of General Relativity” in full aspects, it is also important to test theequivalence principle (EP) with other massless microscopic particles, such as photons andgravitons. One of our future research plans at WIPM is to use two atomic clocks at differentheight, compare the gravitational redshifts of lights, and test the EP.

Then, it is of great value to use data from KAGRA for EP test. Especially, in the era ofmulti-messenger astronomy, people have done initial test of the EP by comparing thevelocities of the light wave and gravitational-wave.

It can be expected that when combining the data from atom interferometer, atomicclock, and KAGRA, a lot of important work on “Test of General Relativity” can be done.

Members: Dongfeng Gao, Gang Wang, Wei ZhaoCollaborators: Mingsheng Zhan, Wei-tou Ni

Page 4: Application for joining Data Analysis Group in KAGRA

Clifford M. Will, "The Confrontation between General Relativity and Experiment",Living Rev. Relativity 17, (2014), 3.

The statement of WEP is that the trajectory of a freely falling “test”body (one not acted upon by such forces as electromagnetism andtoo small to be affected by tidal gravitational forces) is independentof its internal structure and composition. In the simplest case ofdropping two different bodies in a gravitational field, WEP states thatthe bodies fall with the same acceleration (this is often termed theUniversality of Free Fall, or UFF).

The weak equivalence principle (WEP)

WEP test with Atom Interferometers (AI) @ WIPM

4

Page 5: Application for joining Data Analysis Group in KAGRA

The Einstein equivalence principle (EEP)

1. WEP is valid.

2. The outcome of any local non-gravitational experiment is independent of the velocity of the freely-falling reference frame in which it is performed. (The local Lorentz invariance (LLI))

3. The outcome of any local non-gravitational experiment is independent of where and when in the universe it is performed. (The local position invariance (LPI))

5

Page 6: Application for joining Data Analysis Group in KAGRA

The strong equivalence principle (SEP)

1. WEP is valid for self-gravitating bodies as well as for test bodies.

2. The outcome of any local test experiment is independent of the velocity of the (freely falling) apparatus.

3. The outcome of any local test experiment is independent of where and when in the universe it is performed.

SEP EEP WEP

6

Page 7: Application for joining Data Analysis Group in KAGRA

Experimental tests of WEP

A direct test of WEP is the comparison of the acceleration of twolaboratory-sized bodies of different composition in an externalgravitational field. If the principle were violated, then the accelerationsof different bodies would differ.

7

Page 8: Application for joining Data Analysis Group in KAGRA

8

Atom Interferometer

Page 9: Application for joining Data Analysis Group in KAGRA

9

Theory of Atom Interferometers (AI)

Page 10: Application for joining Data Analysis Group in KAGRA

12-meter AI @ WIPM

1000 1500 2000 2500 3000

0.00

0.25

0.50

0.75

1.00

1.25

1.50

1.75

2.00

12 m

11 m

10 m9 m8 m7 m6 m5 m

4 m

3 m

2 m

TO

F S

ign

al (a

. u

.)

Time (ms)

1 m

2800 2900 3000 3100 3200 33000.01

0.02

0.03

0.04

0.05

0.06

12 m

11 m

10 m

TO

F S

ign

al (a

. u

.)

Time (ms)

10

Page 11: Application for joining Data Analysis Group in KAGRA

WEP test to the 10-8 –level @ WIPM

=(2.8±3.0)×10-8

L. Zhou, et al., Phys. Rev. Lett. 115, 013004 (2015)

10-10 -level in the near future 11

Page 12: Application for joining Data Analysis Group in KAGRA

Redshift measurement: test the local Lorentz invariance (LLI)

In a gravitational potential field:

1 2

20

- u=c

1 2

20

- u=(1+ )

c

Generality Relativity: β =0

Year Methods Parameters References

1976 Smithsonianh10000 km

Gravity Probe A 7×10-5 Phys. Rev. Lett. 45,

2081(1980)

2008JILA , LNE-SYRTE,The Uni

versity of TokyoSr-clock, H maser, 199Hg+ 3.5×10−6 Phys. Rev. Lett. 100,

140801 (2008)

2010 UC Berkeley Müller Atom Interferometer 7×10-9 ?Nature, 467, E2(2010)

Nature, 463, 926(2010)

2010 JILA Wineland Al+-clock h30 cm =0.5×10-16

?Science 329,1630(2010)

2011 UC Berkeley Müller Atom Interferometer 10-6 Phys. Rev. Lett. 106, 151102(2011)

Planned EP test with Atomic Clocks (AC) @ WIPM

12

Page 13: Application for joining Data Analysis Group in KAGRA

AI + AC to measure Redshift of photons

Atomic clocks

Atom Interferometers13

Page 14: Application for joining Data Analysis Group in KAGRA

AI4 L ~ 1 kmH

~ 3

00 m

AI1

AI2

AI3

AC1

AC2

AI1,2:10m atom interferometerAI3,4: 1 m atom interferometerAC1,2: atomic clock

Vacuum tube for laser lights

Planned underground lab at Mountain Zhao

14

Page 15: Application for joining Data Analysis Group in KAGRA

15

EP test with gravitational-wave detection

LIGO Scientific Collaboration and Virgo Collaboration, Fermi Gamma-ray Burst Monitor, and INTEGRAL, Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A, Astrophys. J. Lett. 848, L13 (2017).

Page 16: Application for joining Data Analysis Group in KAGRA

16

In WIPM, many efforts are put on testing the weak equivalence principle(WEP), which is the foundation of General Relativity. The basic idea is to launchtwo atomic species in a 10-meter-high atom interferometer, and compare theiraccelerations due to the Earth’s gravity. We are working on to improve the WEPtest to the 10-10 level.

To push the “Test of General Relativity” in full aspects, it is also important totest the equivalence principle (EP) with other massless microscopic particles, suchas photons and gravitons. One of our future research plans at WIPM is to use twoatomic clocks at different height, compare the gravitational redshifts of lights, andtest the EP.

Then, it is of great value to use data from KAGRA for EP test. Especially, in theera of multi-messenger astronomy, people have done initial test of the EP bycomparing the velocities of the light wave and gravitational-wave.

It can be expected that when combining the data from atom interferometer,atomic clock, and KAGRA, a lot of important work on “Test of General Relativity”can be done.

Summary