Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen....

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Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L. Baker, Jr. GRAWAVE® LLC, 8123 Tuscany Avenue, Playa del Rey, California 90293, USA

Transcript of Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen....

Page 1: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

Selection and Detection of High-Frequency Relic Gravitational

Waves

Fangyu Li, Zhenya Chen.Chongqing University, Chongqing 400044,.

ChinaRobert M. L. Baker, Jr.

GRAWAVE® LLC, 8123 Tuscany Avenue, Playa del Rey, California 90293, USA

Page 2: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

1.1. Motivation and Background.Motivation and Background.

2.2. Outline.Outline.

3.3. Electromagnetic Detection to High-Electromagnetic Detection to High-Frequency Gravitational Waves.Frequency Gravitational Waves.

4.4. Challenges and opportunity.Challenges and opportunity.

Page 3: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

Background

Classification of gravitational wave frequency bands.(1) ν~1Hz-104Hz, the detecting region by ground laser interferometer

gravitational wave observatory, such as VIRGO, LIGO, etc.

(2) ν~100Hz-103Hz, the detecting region by the resonant mass detectors, such as Weber Bar.

(3) ν~10-4Hz-1Hz, the detecting region by Laser Interferometer Space Antenna, such as LISA.

(4) ν~10-6Hz-10-3Hz, the detecting region by ASTROD.

(5) ν~107Hz-109Hz, the detecting region by electromagnetic microwave cavity or circular waveguide.

(6) ν~109Hz-1011Hz, the detecting region by coupling system of the microwave beams and static EM fields.

Page 4: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

S. W. Hawking: (1979) High-frequency gravitational waves in excess of 100kHz and may have the most promise for terrestrial generation and practical, scientific, and commercial application (Cambridge university press, Cambridge,

98, 1979)

L. D. Landau and E. M. Lifishitz: Since it has definite energy, the gravitational

waves is itself the source of some additional gravitational field… its field is a second-order effect… but in the case of high-frequency gravitational waves the effect is significantly strengthened….

(the Classical Theory of Fields, on page 372, 1975)

Page 5: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.
Page 6: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

Why would we like to study this project?

(1) According to the theory of general relativity, Gravitational waves (GWs) and Electromagnetic (EM) waves have a same propagating velocity in vacuum:

Optimum coherence effect of the two fields may be generated(2) The GHz (~109Hz-1010Hz) are just typical microwave

frequency band, one can use well-considered microwave technology in the frequency region.

( )

( )

g

g e

e

GWs V cV V c

EM waves V c

Page 7: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

(3) (under the resonant condition) (3) (under the resonant condition)

Characteristic dimensions of the EM Characteristic dimensions of the EM

detecting system would be L~1-10m, detecting system would be L~1-10m,

they are the typical laboratory they are the typical laboratory

dimensions, and it is easy to construct array.dimensions, and it is easy to construct array.

(4)The microwave beam (e.g., Gaussian (4)The microwave beam (e.g., Gaussian

beam) propagating a static field is an beam) propagating a static field is an

open system in free space.open system in free space.

the EM response has more direct the EM response has more direct

displaying effect.displaying effect.

Page 8: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

[1] W. J. Kim et al., Phys. Rev. Lett[1] W. J. Kim et al., Phys. Rev. Lett 96 96 (2006), 2000402(2006), 2000402[2] M. Giovannini, [2] M. Giovannini, Phys. Rev. D 60 (1999), 123511Phys. Rev. D 60 (1999), 123511 M. Giovannini, M. Giovannini, Class. Quantum Grav. 16 (1999), 2905Class. Quantum Grav. 16 (1999), 2905[3] A. Riazuelo and J. P. Uzan.[3] A. Riazuelo and J. P. Uzan. Phys. Rev. D 62 (2000), Phys. Rev. D 62 (2000), 083506083506[4] J. P. Qstriker and P. J. Sternhardt, [4] J. P. Qstriker and P. J. Sternhardt, Sci. Am. (Int. Ed.)Sci. Am. (Int. Ed.) 284(2001), 46.284(2001), 46.[5] L. P. Grishchuk, [5] L. P. Grishchuk, (2003), gr-qc/0305051(2003), gr-qc/0305051[6] R. R. Caldwell et al., [6] R. R. Caldwell et al., Sci. Am. (In. Ed.) 272 (2001), 20.Sci. Am. (In. Ed.) 272 (2001), 20.[7] B. A. Remington et al., [7] B. A. Remington et al., Science 284 (1999), 1488Science 284 (1999), 1488[8] P. Chen, [8] P. Chen, (2003) astro-Ph/0303350.(2003) astro-Ph/0303350.[9] C. Joshi and P. Corkum, [9] C. Joshi and P. Corkum, Physics Today (1995), (1) 36.Physics Today (1995), (1) 36.[10] G. Mourou et al.,[10] G. Mourou et al., Physic Today (1998), (1) 22 Physic Today (1998), (1) 22[11] J. M. Hopking and W. Sibbett, [11] J. M. Hopking and W. Sibbett, Sci. Am. (In. Ed.) 268 Sci. Am. (In. Ed.) 268 (2000), 1.(2000), 1.[12] M. Portilla et al., [12] M. Portilla et al., Phys. Rev. D 63 (2001), 044014-1-7Phys. Rev. D 63 (2001), 044014-1-7

Page 9: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

[13] R. M. L. Baker, Jr., [13] R. M. L. Baker, Jr., First International High-Frequency GWFirst International High-Frequency GW

Conference, edited by P. Murad, The MITRE Corporation,Conference, edited by P. Murad, The MITRE Corporation,

Mclean, VA, USA (2003), Paper HFGW-03-101, Paper HFGW-Mclean, VA, USA (2003), Paper HFGW-03-101, Paper HFGW-

03-117.03-117.

H. D. Froning et al., H. D. Froning et al., (2003), Paper HFGW-03-122.(2003), Paper HFGW-03-122.

H. Dehnen et al.,H. Dehnen et al., (2003), Paper-HFGW-03-102. (2003), Paper-HFGW-03-102.

D. G. Fontana et al., D. G. Fontana et al., (2003), Paper-HFGW-03-107.(2003), Paper-HFGW-03-107.

G. V. Stephenson, G. V. Stephenson, (2003), Paper-HFGW-03-104.(2003), Paper-HFGW-03-104.

[14] R. C. Woods et al., [14] R. C. Woods et al., (STAIF 2005), Americal Institute of Physics(STAIF 2005), Americal Institute of Physics

Conference Proceeding, Melville, NY 746 (2005), 1298.Conference Proceeding, Melville, NY 746 (2005), 1298.

R. M. L. Baker, Jr., et al.,R. M. L. Baker, Jr., et al., ibid (STAIF 2005), (2005), 1315 ibid (STAIF 2005), (2005), 1315

[15] D. G. Fontana et al.,[15] D. G. Fontana et al., (STAIF 2004), Americal Institute of Physics, (STAIF 2004), Americal Institute of Physics,

Melville, NY 699 (2004), 1114Melville, NY 699 (2004), 1114

[16] Hansheng Peng et al[16] Hansheng Peng et al., “286-TW Ti: Sapphire Laser at CAEP”., “286-TW Ti: Sapphire Laser at CAEP”

SPIE Prodeedings (2004) 5627.SPIE Prodeedings (2004) 5627.

Page 10: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

[17] X. Yang, et al., [17] X. Yang, et al., Optics Letters 27 (2002), 1135Optics Letters 27 (2002), 1135[18] Yuelin Li et al., [18] Yuelin Li et al., Opt. Soc. Am. B17 (6) (2000), 1098Opt. Soc. Am. B17 (6) (2000), 1098[19] R. M. L. Baker, Jr., Fangyu Li and Ruxin Li, (2005), AIAA(N.USA),[19] R. M. L. Baker, Jr., Fangyu Li and Ruxin Li, (2005), AIAA(N.USA), (2005).1076.(2005).1076.[20] L. P. Grishchuk,[20] L. P. Grishchuk, First International High-Frequency GW First International High-Frequency GW Conference, edited by P. Murad, The MITRE Corporation,Conference, edited by P. Murad, The MITRE Corporation, Mclean, VA, USA (2003), Paper HFGW-03-119Mclean, VA, USA (2003), Paper HFGW-03-119[21] A. M. Cruise,[21] A. M. Cruise, Class. Quantum Grav. 17 (2000), 2525 Class. Quantum Grav. 17 (2000), 2525 A.M. Cruise et al., Submitted toA.M. Cruise et al., Submitted to Class. Quantum,Grav. (2005) Class. Quantum,Grav. (2005) (personal communication)(personal communication)[22] P. Bernard et al., [22] P. Bernard et al., (2002), gr-qc/0203024(2002), gr-qc/0203024 P. Bernard et al., P. Bernard et al., Review of Scientific Instruments 72 (2001),Review of Scientific Instruments 72 (2001), 24282428[23] A. Chincarini and G. Gemme, First International High-Frequency[23] A. Chincarini and G. Gemme, First International High-Frequency GW ConferenceGW Conference, edited by P. Mural, The MITRE Corporation, , edited by P. Mural, The MITRE Corporation, Mclean, VA, USA (2003), Paper-03-103Mclean, VA, USA (2003), Paper-03-103 [24] U. H. Gerlach, [24] U. H. Gerlach, Phys. Rev. D 46 (1992), 1239Phys. Rev. D 46 (1992), 1239[25] L. P. Grishchuk and M. V. Sazhin, [25] L. P. Grishchuk and M. V. Sazhin, Sov. Phys. JETP 53 (1983),Sov. Phys. JETP 53 (1983), 11281128

Page 11: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

[26] Ning Li and D. G. Torr, [26] Ning Li and D. G. Torr, Phys. Rev. D 43 (1991), 457. Phys. Rev.Phys. Rev. D 43 (1991), 457. Phys. Rev. B 46 (1992), 5491 B 46 (1992), 5491 [27] N. V. Mitskievich and A. I. Nesterov[27] N. V. Mitskievich and A. I. Nesterov, Gen. Relativ. Gravit. 27, Gen. Relativ. Gravit. 27 (1995), 361(1995), 361[28] R. M. L. Baker, Jr.,Fangyu Li,[28] R. M. L. Baker, Jr.,Fangyu Li, AIAA/AIP STAIF edited by AIAA/AIP STAIF edited by M. S. El-Genr, (Melville, N. Y. USA) (2006) Feb. 18M. S. El-Genr, (Melville, N. Y. USA) (2006) Feb. 18[29] Fangyu Li, Mengxi Tang and Dongping Shi,[29] Fangyu Li, Mengxi Tang and Dongping Shi, Phys. Rev. D 67 Phys. Rev. D 67 (2003), 104008-1-17.(2003), 104008-1-17.[30] Fangyu Li,Mengxi Tang and Jun Luo, [30] Fangyu Li,Mengxi Tang and Jun Luo, Phys. Rev. D 62Phys. Rev. D 62 (2000), 044018-1-9.(2000), 044018-1-9.[31] Fangyu Li et al.,[31] Fangyu Li et al., First Intenational High-Frequency GW First Intenational High-Frequency GW Conference, edited by P. Murad, The MITRE Corporation,Conference, edited by P. Murad, The MITRE Corporation, Mclean, VA, USA (2003), Pape-HFGW-03-108Mclean, VA, USA (2003), Pape-HFGW-03-108[32] Fangyu Li and Mengxi Tang, International Journal of Mordern [32] Fangyu Li and Mengxi Tang, International Journal of Mordern Physics D 11(7) (2002),1049.Physics D 11(7) (2002),1049.[33] Mengxi Tang and Fangyu Li,Classical and Quantum Gravity 17(2000),[33] Mengxi Tang and Fangyu Li,Classical and Quantum Gravity 17(2000), 1049.1049.[34] W. K. Logi and A. R. Mickdson,[34] W. K. Logi and A. R. Mickdson, Phys. Rev. D 16 (1977), 2915 Phys. Rev. D 16 (1977), 2915

Page 12: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

Some expected and possible HFGW sources

ν (Hz) h ΩRelic GWs  ~109-1011 ~ 10-30-10-32

(r. m. s)

~10-5-10-6

Solar Plasma  ~1015 ~ 10-39

(on the earth)

Strong EM Systems (e.g. ,see First High-

frequency GW Conference

Proceedings,Mclean,Virginia,USA,2003 )

  ~107-108 ~ 10-29-10-35

(on the focal region)

High Energy Particles

(e.g., Fermi Ring)

 

~104 - 105

~ 10-39-10-40

(on the center)

Page 13: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.
Page 14: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.
Page 15: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.
Page 16: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.
Page 17: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

According to According to Randall-SuRandall-Sundrumndrum models, the HFG models, the HFGWs would be more capaWs would be more capable of carrying energy froble of carrying energy from our m our

3-brane world than lowe3-brane world than lower-frequency GWs by their-frequency GWs by their propagation in the extrr propagation in the extra dimensions,do inverse a dimensions,do inverse effects of the effects of the

R-S models exist for our R-S models exist for our brane world?brane world?

Page 18: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.
Page 19: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

Birmingham University, Birmingham, England

Page 20: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

R. Ballantini et.al.,Institute of National Nuclear Physics, Genova, Italy

Page 21: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.
Page 22: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.
Page 23: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.
Page 24: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

Unlike the cavity EM response to the HFGWs, a Gaussian beam (GB) passing through a static magnetic field is an open system in the free space, the perturbation photon flux and the background photon flux have very different physical behaviour in the local regions, and the perturbation has more direct observable effect.

Page 25: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

Coupling system of fractal membranes and Gaussian beam passing through a static magnetic field

Page 26: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

High-frequency relic GWs and their asymptotic behavior in the high-frequency band:

1 3 2 2 3 2( ) [ ( ) ( ) ( ) ( )]. 2

A k J k A k J k

General form of high-frequency constant amplitude GWs is

Asymptotic form in the high-frequency region and in the laboratory frame of reference will be

.(1), (2)Eqs ( , ) ( ) ( ) exp[ ( )]

( ) ( ) exp[ ( )]

g g g

g g g

h x t A k a t i k x t

B k a t i k x t

(3)

(1)

(2)

exp ( )

exp ( )

g g

g g

h A i k x t

h A i k x t

(4)

( )[exp( ) exp( )] , ij ijh ik x ik x e

a

Page 27: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

The Gaussian beam with the double transverse polarized electric modes (DTPEM)

2210

22exp exp tan

21

ee e

k rr zi k z t

W f Rz

f

(5)

2(0) (0)

20

2(0) (0)

20

(0)

0

1 2Re exp ,

2

1 2Re exp ,

2

1Re

2

yxx y x

e e

y xy x y

e e

y xz x y

e e e

i rn f

y x W

i rn f

x y W

i in

z

2(0)

2

2exp .z

rf

z W

(6)

Page 28: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

0

(0) (1)

1

0

g g g F Jg

F F F

F F F

(7)

Page 29: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

High-frequency relic GW:

the tensor perturbation

Gaussian beam +static magnetic field:

background real photons +virtual photons

Synchro-coherent

resonanceωe=ωg

It is possible to produce the perturpative photon flux

(PPF),and the PPF and BPF have very different physical behaviour in some special local

regions

(0) (1) (2)

T T T Tmn mn mn mn= + +

(0) (1) (2)

T T Tmn mn mn? ?

Page 30: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

zo

B0

x

y y

x

GW

GW

EMW

Gaussian beam

PPF

PPF

Page 31: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

The PPF and the BPF propagate along opposite directions in the regions of 1st, 3rd,6th,and 8th octants,while they have the same propagating directions in the regions of 2nd, 4th , 5th and 7th octants.

Page 32: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

X

12

3 4

O

PPF

PPF

PPF

PPF

BPF

BPF

BPF

BPF

Y

Fig 1, the region of z>0

O

Y

X

Page 33: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

X

56

7 8

O

PPF

PPF

PPF

PPF

BPF

BPF

BPF

BPF

Y

Fig 2, the region of z<0

O

Y

X

Page 34: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

The perturbative photon fluxesThe perturbative photon fluxes

νν(Hz)(Hz) ΩΩ(peak (peak

values)values)

hh(r.m.s)(r.m.s)

l l (m),the (m),the interacting interacting dimensionsdimensions

of static of static magnetic fieldmagnetic field

The PPFs (sThe PPFs (s-1-1))

10101010 1010-6-6 2.00×102.00×10-31-31

0.30.366

2020

2.02 ×102.02 ×104.04×104.04×1022

1.35×101.35×103 3

10101010 1010-5-5 6.32×106.32×10-31-31

0.30.366

2020

6.37×10 6.37×10 1.27×101.27×1033

4.25×104.25×1033

Page 35: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

Directional sensitivity of the system

Propagating directions of the resonant components

of the relic GW PPFs (s-1)

z-zxy

1.27×103

3.16×106.30×10-1

0

Page 36: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

The thermal noise and the EM noise

For the possible external EM noise sources,using a Faradaycage or shielding covers made from the fractal membranes,ora good “microwave darkroom” might provide an effective shielding environment.

Page 37: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

(1) (1) (0) (1)*

0 0

1 1 1Re ( )

2yx

x y z ye e e

in E B E

y x

yy

(0)0 1

2 1/ 2 20

ˆ ( )1

4 [1 ( / ) ] ( / )y g

e

A B k y z l

z f z f z

y 2 (0)

0 112 2 3/ 2

0 0

ˆ ( )sin tan

2 2 [1 ( / ) ]g yk r A B y z lz

R f W z f

y

2 (0) 22 20 11 1

12 2 2 1/ 20

ˆ ( )1 4cos tan exp 1 ( )sin tan

2 4 [1 ( / ) ] 2g y g g

e

k r A B k z l k xz r x zF y

R f W W R z f R f

y

2 2 (0) 20 11 2 1

2 12 2 4 2 1/ 20

ˆ ( )2 1( )cos tan ( )cos tan

2 4 [1 ( / ) ] 2g g y gk x k A B z l k xz z

F y x F yR f W R W z f R f

y

2 21

2 2( ) sin tan exp

2gk x z x

F yR f W

22

1 2( ) exp( )cos( ) ,

2gk yy

F y dyW R

= -ò ,)2

sin()exp()(2

2

2

2 dyR

yk

W

yyF g

where,

Page 38: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

The separation of the PPF(signal) from the background photon flux

The distance to the fractal membrane 3.16cm 12cm 42cm 70cm

The background photon flux 2.44×1024 s-1 2.16×1022 s-1 1.27×103 s-1 1.97×10-6 s-1

The PPF reflected or transmitted by the fractal membrane

1.27×103 s-1 1.24×103 s-1 1.21×103 s-1 1.01×103 s-1

Page 39: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

Opportunity

1. This scheme might provide a new window and in new way for detection of the HFRGWs in the GHz band.

2. Typical dimensions of the detecting system would be only 1-10m, and constructing cost may be only one percent of LIGO or less.

3. It contains new ideas, new developed results (including theoretical, experimental and technological results)

Page 40: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

Difficulties and challenge

1. How to keep a good vacuum environment to avoid the scattering of the photons and the dielectric dissipation.

2. How to reduce further temperature and maintain a good cryogenic environment to suppress relevant thermal noise.

Page 41: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

3. How to make a best combination to reduce

and overcome system noise, what is the concrete

form and influence of quantum noise in the system?

4. How to suppress distortion of the shape and the spot

radius of the Gaussian beam, what is concrete

correction and influence of the higher order modes

in the Gaussian beam?

Page 42: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

However, because of fast development of relative technology,such as superconductors, nanotechnology, high-quality factor microwave cavities, ultra-fast science,strong field physics, cryogenic technology,strong microwave beam technology, high-energy laboratory astrophysics,etc.

They offered technically possibilities

This subject might become a reality

Page 43: Selection and Detection of High-Frequency Relic Gravitational Waves Fangyu Li, Zhenya Chen. Chongqing University, Chongqing 400044,. China Robert M. L.

Thank you!谢谢!