Decigo.jp

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Host name	www3829.sakura.ne.jp
IP address	163.43.102.39
Location	Osaka Japan
Latitude	34.6848
Longitude	135.5142
Timezone	Asia/Tokyo
Postal	543-0062

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Decigo

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DECIGO and DECIGO Pathfinder

DECIGO 1000km DPF 30cm DECIGO 1000km Local Sensor Actuator Thruster Laser DPF 30cm . DPF satellite Amaldi9 (July 15, 2011, Cardiff, U.K.) Stabilized. Laser source Interferometer 950x950x1100mm module Satellite Bus system Solar Paddle Mission Thruster head On-board Computer Bus thruster Satellite Bus (‘Standard bus’ system) DPF Payload …

Decigo.jp

DA: 9 PA: 45 MOZ Rank: 54

Gravitational-wave observatories: LCGT and DECIGO - 東京大学

DECIGO The 20th workshop on General Relativity and Gravitation (JGRG20, Sept. 23, 2010, YITP, Kyoto) DECIGO Space GW antenna (~2027) Obs. band around 0.1 Hz 10–4 10–2 100 102 104 10–26 10–24 10–22 10–20 10–18 10–16 Frequency [Hz] Strain [1/Hz 1/2] Terrestrial Detectors (Ad. LIGO, LCGT, etc) DECIGO LISA

Granite.phys.s.u-tokyo.ac.jp

DA: 28 PA: 34 MOZ Rank: 63

Primordial gravitational wave and DECIGO

E-mail: [email protected] DECIGO working group Gravitational waves were detected in 2015 for the first time in the history of humankind. Since then, around ten gravitational wave signals coming from black hole/neutron star binary coalescences have been detected. Among various expected gravitational wave sources, the beginning of the universe is one of …

Inspirehep.net

DA: 14 PA: 39 MOZ Rank: 55

DECIGO - granite.phys.s.u-tokyo.ac.jp

DECIGO (LISA type, 5x104km) DECIGO (FP type, 1000km) Laser: 10W, 532nm Mass: 100kg Mirror: 1m dia. WD-WD conf usion noise Decisive factor: Binary confusion noise . 11th Marcel Grossmann Meeting on General Relativity (July 23 - 29, 2006, Freie Universität Berlin) 7 Pre-conceptual Design (4) Arm length Cavity arm length : Limited by diffraction loss Calculate …

Granite.phys.s.u-tokyo.ac.jp

DA: 28 PA: 21 MOZ Rank: 52

ISAS/JAXA Funaki Laboratory | Next Generation Deep Space Mission

DECIGO will have a chance to observe gravitational wave in an orbit around the sun, unveiling the physics at the beginning of the universe. DECIGO consists of three formation flying spacecraft using an interferometry. DECIGO pathfinder will verify required technologies for DECIGO, and DPF is a strong candidate for small scientific satellite of ISAS that will fly around 2017. Our …

Stage.tksc.jaxa.jp

DA: 18 PA: 27 MOZ Rank: 49

DECIGO and DECIGO Pathfinder

DECIGO-PF GW2010 (October 16, 2010, University of Minnesota, Minneapolis) DECIGO Pathfinder (DPF) Single satellite (Payload ~1m3, 350kg) Low-earth orbit (Altitude 500km, sun synchronous) 30cm FP cavity with 2 test masses Stabilized laser source Drag-free control First milestone mission for DECIGO Shrink arm cavity DECIGO 1000km DPF 30cm DECIGO ...

Conservancy.umn.edu

DA: 19 PA: 49 MOZ Rank: 73

Proc. International Conference on Space Optical Systems and

For DECIGO and DPF Mitsuru Musha, Ken'ichi Nakagawa, Ken-ichi Ueda Institute for Laser Science University of electro-communications 1-5-1 Chofugaoka, Chofu-shi, Tokyo, Japan [email protected] Abstract—As a light source for the space gravitational wave detector DECIGO/DPF, we have developed space-borne frequency-stabilized lasers. The light source …

Icsos2012.nict.go.jp

DA: 20 PA: 19 MOZ Rank: 45

Prospects of determination of reheating temperature after …

Abstract. If the tensor-to-scalar ratio $r$ of cosmological perturbations takes a large value $r\\sim 0.1$, which may be inferred from the recent BICEP2 result,

Academic.oup.com

DA: 16 PA: 35 MOZ Rank: 58

7KH-DSDQHVHVSDFHJUDYLWDWLRQDOZDYHDQWHQQD

DECIGO pathfinder Masaki Ando, Seiji Kawamura, Shuichi Sato et al.-Recent citations Gravitational Waves Induced by Non-Gaussian Scalar Perturbations Rong-Gen Cai et al-Detecting nonclassical primordial gravitational waves with Hanbury-Brown Twiss interferometry Sugumi Kanno and Jiro Soda-How post-Newtonian dynamics shape the distribution of …

Www-o.oit.ac.jp

DA: 15 PA: 50 MOZ Rank: 88

DECIGO PATHFINDER | International Journal of Modern Physics D

Abstract. DECIGO Pathfinder (DPF) is a small (~350 kg) satellite orbiting the Earth. DPF was originally proposed as the first milestone mission for a future space gravitational-wave (GW) antenna, DECi-hertz Interferometer Gravitational wave Observatory (DECIGO). In addition to the purpose of space demonstrations for DECIGO, DPF has scientific ...

Worldscientific.com

DA: 23 PA: 34 MOZ Rank: 66

Developments of high frequency and intensity stabilized lasers for ...

In Japan, not only the ground-based gravitational wave (GW) detector mission KAGRA but also the space GW detector mission DECIGO (DECi-hertz Interferometer Gravitational wave Observatory) and its milestone mission B-DECIGO have been promoted. The designed strain sensitivity of DECIGO and B-DECIGO are δL / L < 10 −23.

Link.springer.com

DA: 17 PA: 34 MOZ Rank: 61

(PDF) DECIGO pathfinder - ResearchGate

DECIGO, a DECi-hertz Interferometer Gravitational wave Observatory, is a space gravitational wave. antenna planned to be launched in 2024 [1] [2]. The purpose of …

Researchgate.net

DA: 20 PA: 39 MOZ Rank: 70

หอดูดาวคลื่นความโน้มถ่วงเดซิเฮิรตซ์

Deci เฮิรตซ์ Interferometer ความโน้มถ่วงคลื่นหอดูดาว (หรือDECIGO ) เป็นเสนอญี่ปุ่นพื้นที่ตามหอคลื่นความโน้มถ่วง [1] [2]เลเซอร์อินเทอร์ตรวจจับคลื่นความโน้มถ่วง ...

Sawadee.wiki

DA: 12 PA: 12 MOZ Rank: 36

Space gravitational wave antenna DECIGO and B-DECIGO

Since B-DECIGO is a downsized mission of DECIGO, the designed strain sensitivity is l/l = 2 × 10 −23 /√Hz which is one order of magnitude worse than that of DECIGO (blue trace in Fig. 3b). B-DECIGO has initially started as a pathfinder of DECIGO, and its main purpose is the feasibility tests of the key technologies such as formation flight with the separation of 100 km, …

Link.springer.com

DA: 17 PA: 34 MOZ Rank: 64

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