The Japanese space gravitational wave antenna: DECIGO

@article{Kawamura2011TheJS,
  title={The Japanese space gravitational wave antenna: DECIGO},
  author={Seiji Kawamura and Masaki Ando and Naoki Seto and Shuichi Sato and Takashi Nakamura and Kimio Tsubono and N Kanda and Takahiro Tanaka and Jun’ichi Yokoyama and Ikkoh Funaki and Kenji Numata and Kunihito Ioka and Takeshi Takashima and Kazuhiro Agatsuma and Tomotada Akutsu and Koh-suke Aoyanagi and Koji Arai and Akito Araya and Hideki Asada and Yoichi Aso and Dan Chen and Takeshi Chiba and Toshikazu Ebisuzaki and Yumiko Ejiri and Motohiro Enoki and Yoshiharu Eriguchi and Masataka Fujimoto and Ryuichi Fujita and Mitsuhiro Fukushima and Toshifumi Futamase and Tomohiro Harada and Tatsuaki Hashimoto and Kazuhiro Hayama and Wataru Hikida and Yoshiaki Himemoto and Hisashi Hirabayashi and Takashi Hiramatsu and Feng-Lei Hong and Hideyuki Horisawa and Mizuhiko Hosokawa and Kiyotomo Ichiki and Takeshi Ikegami and Kaiki Taro Inoue and Koji Ishidoshiro and Hideki Ishihara and Takehiko Ishikawa and Hideharu Ishizaki and Hiroyuki Ito and Yousuke Itoh and Kiwamu Izumi and Isao Kawano and Nobuki Kawashima and Fumiko Kawazoe and Naoko Kishimoto and Kenta Kiuchi and Shiho Kobayashi and Kazunori Kohri and Hiroyuki Koizumi and Yasufumi Kojima and Keiko Kokeyama and Wataru Kokuyama and Kei Kotake and Yoshihide Kozai and Hiroo Kunimori and Hitoshi Kuninaka and Kazuaki Kuroda and Sachiko Kuroyanagi and Kei-ichi Maeda and Hideo Matsuhara and Nobuyuki Matsumoto and Yuta Michimura and Osamu Miyakawa and Umpei Miyamoto and Shinji Miyoki and Mutsuko Y. Morimoto and Toshiyuki Morisawa and Shigenori Moriwaki and Shinji Mukohyama and Mitsuru Musha and Shigeo Nagano and Isao Naito and Kouji Nakamura and Hiroyuki Nakano and Ken-ichi Nakao and Shinichi Nakasuka and Yoshinori Nakayama and Kazuhiro Nakazawa and Erina Nishida and Kazutaka Nishiyama and Atsushi J. Nishizawa and Yoshito Niwa and Taiga Noumi and Yoshiyuki Obuchi and Masatake Ohashi and Naoko Ohishi and Masashi Ohkawa and Kenshi Okada and Norio Okada and Ken-ichi Oohara and Norichika Sago and Motoyuki Saijo and Ry{\^o} Sait{\^o} and Masaaki Sakagami and Shin-ichiro Sakai and Shihori Sakata and Misao Sasaki and Takashi Sato and Masaru Shibata and Hisa-aki Shinkai and Ayaka Shoda and Kentaro Somiya and Hajime Sotani and Naoshi Sugiyama and Yudai Suwa and Rieko Suzuki and Hideyuki Tagoshi and Fuminobu Takahashi and Kakeru Takahashi and Keitaro Takahashi and Ryutaro Takahashi and Ryuichi Takahashi and Tadayuki Takahashi and Hirotaka Takahashi and Takamori Akiteru and Tadashi Takano and Nobuyuki Tanaka and K eisuke Taniguchi and Atsushi Taruya and Hiroyuki Tashiro and Yasuo Torii and Morio Toyoshima and Shinji Tsujikawa and Y. Tsunesada and Akitoshi Ueda and Ken‐ichi Ueda and Masayoshi Utashima and Yaka Wakabayashi and Kent Yagi and Hiroshi Yamakawa and Kazuhiro Yamamoto and Toshitaka Yamazaki and Chul-Moon Yoo and Shijun Yoshida and Taizoh Yoshino and K-X Sun},
  journal={Classical and Quantum Gravity},
  year={2011},
  volume={28},
  pages={094011}
}
The objectives of the DECi-hertz Interferometer Gravitational Wave Observatory (DECIGO) are to open a new window of observation for gravitational wave astronomy and to obtain insight into significant areas of science, such as verifying and characterizing inflation, determining the thermal history of the universe, characterizing dark energy, describing the formation mechanism of supermassive black holes in the center of galaxies, testing alternative theories of gravity, seeking black hole dark… 

Space gravitational wave antenna DECIGO and B-DECIGO

Since the direct detection of gravitational wave will give us a fruitful insight about the early universe or life of stars, laser interferometric gravitational wave detectors with the strain

DECi-hertz Interferometer Gravitational-wave Observatory: Forecast Constraints on the Cosmic Curvature with LSST Strong Lenses

In this paper, we aim to use the DECi-hertz Interferometer Gravitational-wave Observatory (DECIGO), a future Japanese space gravitational-wave antenna sensitive to the frequency range between LISA

Detection Landscape in the deci-Hertz Gravitational-Wave Spectrum

Direct observations of gravitational waves at frequencies around deci-Hertz will play a crucial role in fully exploiting the potential of multi-messenger astronomy. In this chapter, we discuss the

Gravitational wave astronomy

We are entering a new era of gravitational-wave astronomy. The ground-based interferometers have reached their initial design sensitivity in the audio band. Several upper limits have been set for

Multiple Measurements of Gravitational Waves Acting as Standard Probes: Model-independent Constraints on the Cosmic Curvature with DECIGO

Although the spatial curvature has been precisely determined via observations of the cosmic microwave background by the Planck satellite, it still suffers from the well-known cosmic curvature

LION: laser interferometer on the moon

Gravitational wave astronomy has now left its infancy and has become an important tool for probing the most violent phenomena in our Universe. The LIGO/Virgo-KAGRA collaboration operates ground based

Orbit optimization and time delay interferometry for inclined ASTROD-GW formation with half-year precession-period

ASTROD-GW (ASTROD [Astrodynamical Space Test of Relativity using Optical Devices] optimized for Gravitational Wave detection) is a gravitational-wave mission with the aim of detecting gravitational

Prospects for gravitational-wave polarization tests from compact binary mergers with future ground-based detectors

There exist six possible polarization modes of gravitational waves in general metric theory of gravity, while two tensor polarization modes are allowed in general relativity. The properties and

Observational results from the LIGO and Virgo detectors

The first generation of ground-based interferometric gravitational wave detectors, LIGO, GEO and Virgo, have operated and taken data at their design sensitivities over the last few years. The data
...

References

SHOWING 1-10 OF 43 REFERENCES

DECIGO: the Japanese space gravitational wave antenna

DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) is the planned Japanese space gravitational wave antenna, aiming to detect gravitational waves from astrophysically and

The Japanese space gravitational wave antenna—DECIGO

DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) is the future Japanese space gravitational wave antenna. It aims at detecting various kinds of gravitational waves between 1 mHz and

DECIGO and DECIGO pathfinder

A space gravitational-wave antenna, DECIGO (DECI-hertz interferometer Gravitational wave Observatory), will provide fruitful insights into the universe, particularly on the formation mechanism of

Determining the Hubble constant from gravitational wave observations

I report here how gravitational wave observations can be used to determine the Hubble constant, H0. The nearly monochromatic gravitational waves emitted by the decaying orbit of an ultra–compact,

Detecting Planets around Compact Binaries with Gravitational Wave Detectors in Space

I propose a method to detect planets around compact binaries that are strong sources of gravitational radiation. This approach is to measure gravitational wave phase modulations induced by the

Possibility of direct measurement of the acceleration of the universe using 0.1 Hz band laser interferometer gravitational wave antenna in space.

TLDR
It may be possible to construct a laser interferometer gravitational wave antenna in space with h(rms) approximately 10(-27) at f approximately 0.1 Hz and the formula for phase shift due to accelerating motion might be applied for binary sources of LISA.

The gravitational wave background from cosmological compact binaries

We use a population synthesis approach to characterize, as a function of cosmic time, the extragalactic close binary population descended from stars of low to intermediate initial mass. The

Ultrahigh precision cosmology from gravitational waves

We show that the Big Bang Observer (BBO), a proposed space-based gravitational-wave (GW) detector, would provide ultraprecise measurements of cosmological parameters. By detecting ∼3×10^5

Cosmological test of gravity with polarizations of stochastic gravitational waves around 0.1-1 Hz

In general relativity, a gravitational wave has two polarization modes (tensor mode), but it could have additional polarizations (scalar and vector modes) in the early stage of the Universe, where

Ground-based interferometers and their science reach

The existence of gravitational waves was predicted by Einstein more than 90 years ago, but they have not yet been directly detected. A Michelson laser interferometer is one of the most promising