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201. The Japanese space gravitational wave antenna: DECIGO

Author

Kawamura, Seiji, primary, Ando, Masaki, additional, Seto, Naoki, additional, Sato, Shuichi, additional, Nakamura, Takashi, additional, Tsubono, Kimio, additional, Kanda, Nobuyuki, additional, Tanaka, Takahiro, additional, Yokoyama, Jun'ichi, additional, Funaki, Ikkoh, additional, Numata, Kenji, additional, Ioka, Kunihito, additional, Takashima, Takeshi, additional, Agatsuma, Kazuhiro, additional, Akutsu, Tomotada, additional, Aoyanagi, Koh-suke, additional, Arai, Koji, additional, Araya, Akito, additional, Asada, Hideki, additional, Aso, Yoichi, additional, Chen, Dan, additional, Chiba, Takeshi, additional, Ebisuzaki, Toshikazu, additional, Ejiri, Yumiko, additional, Enoki, Motohiro, additional, Eriguchi, Yoshiharu, additional, Fujimoto, Masa-Katsu, additional, Fujita, Ryuichi, additional, Fukushima, Mitsuhiro, additional, Futamase, Toshifumi, additional, Harada, Tomohiro, additional, Hashimoto, Tatsuaki, additional, Hayama, Kazuhiro, additional, Hikida, Wataru, additional, Himemoto, Yoshiaki, additional, Hirabayashi, Hisashi, additional, Hiramatsu, Takashi, additional, Hong, Feng-Lei, additional, Horisawa, Hideyuki, additional, Hosokawa, Mizuhiko, additional, Ichiki, Kiyotomo, additional, Ikegami, Takeshi, additional, Inoue, Kaiki T, additional, Ishidoshiro, Koji, additional, Ishihara, Hideki, additional, Ishikawa, Takehiko, additional, Ishizaki, Hideharu, additional, Ito, Hiroyuki, additional, Itoh, Yousuke, additional, Izumi, Kiwamu, additional, Kawano, Isao, additional, Kawashima, Nobuki, additional, Kawazoe, Fumiko, additional, Kishimoto, Naoko, additional, Kiuchi, Kenta, additional, Kobayashi, Shiho, additional, Kohri, Kazunori, additional, Koizumi, Hiroyuki, additional, Kojima, Yasufumi, additional, Kokeyama, Keiko, additional, Kokuyama, Wataru, additional, Kotake, Kei, additional, Kozai, Yoshihide, additional, Kunimori, Hiroo, additional, Kuninaka, Hitoshi, additional, Kuroda, Kazuaki, additional, Kuroyanagi, Sachiko, additional, Maeda, Kei-ichi, additional, Matsuhara, Hideo, additional, Matsumoto, Nobuyuki, additional, Michimura, Yuta, additional, Miyakawa, Osamu, additional, Miyamoto, Umpei, additional, Miyoki, Shinji, additional, Morimoto, Mutsuko Y, additional, Morisawa, Toshiyuki, additional, Moriwaki, Shigenori, additional, Mukohyama, Shinji, additional, Musha, Mitsuru, additional, Nagano, Shigeo, additional, Naito, Isao, additional, Nakamura, Kouji, additional, Nakano, Hiroyuki, additional, Nakao, Kenichi, additional, Nakasuka, Shinichi, additional, Nakayama, Yoshinori, additional, Nakazawa, Kazuhiro, additional, Nishida, Erina, additional, Nishiyama, Kazutaka, additional, Nishizawa, Atsushi, additional, Niwa, Yoshito, additional, Noumi, Taiga, additional, Obuchi, Yoshiyuki, additional, Ohashi, Masatake, additional, Ohishi, Naoko, additional, Ohkawa, Masashi, additional, Okada, Kenshi, additional, Okada, Norio, additional, Oohara, Kenichi, additional, Sago, Norichika, additional, Saijo, Motoyuki, additional, Saito, Ryo, additional, Sakagami, Masaaki, additional, Sakai, Shin-ichiro, additional, Sakata, Shihori, additional, Sasaki, Misao, additional, Sato, Takashi, additional, Shibata, Masaru, additional, Shinkai, Hisaaki, additional, Shoda, Ayaka, additional, Somiya, Kentaro, additional, Sotani, Hajime, additional, Sugiyama, Naoshi, additional, Suwa, Yudai, additional, Suzuki, Rieko, additional, Tagoshi, Hideyuki, additional, Takahashi, Fuminobu, additional, Takahashi, Kakeru, additional, Takahashi, Keitaro, additional, Takahashi, Ryutaro, additional, Takahashi, Ryuichi, additional, Takahashi, Tadayuki, additional, Takahashi, Hirotaka, additional, Akiteru, Takamori, additional, Takano, Tadashi, additional, Tanaka, Nobuyuki, additional, Taniguchi, Keisuke, additional, Taruya, Atsushi, additional, Tashiro, Hiroyuki, additional, Torii, Yasuo, additional, Toyoshima, Morio, additional, Tsujikawa, Shinji, additional, Tsunesada, Yoshiki, additional, Ueda, Akitoshi, additional, Ueda, Ken-ichi, additional, Utashima, Masayoshi, additional, Wakabayashi, Yaka, additional, Yagi, Kent, additional, Yamakawa, Hiroshi, additional, Yamamoto, Kazuhiro, additional, Yamazaki, Toshitaka, additional, Yoo, Chul-Moon, additional, Yoshida, Shijun, additional, Yoshino, Taizoh, additional, and Sun, Ke-Xun, additional

Published
2011
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207. Merger of binary neutron stars of unequal mass in full general relativity

Author

Shibata, Masaru, Taniguchi, Keisuke, Uryu, Koji, Shibata, Masaru, Taniguchi, Keisuke, and Uryu, Koji

Abstract

We present results of three dimensional numerical simulations of the merger of unequal-mass binary neutron stars in full general relativity. A $\Gamma$-law equation of state $P=(\Gamma-1)\rho\epsilon$ is adopted, where $P$, $\rho$, $\varep$, and $\Gamma$ are the pressure, rest mass density, specific internal energy, and the adiabatic constant, respectively. We take $\Gamma=2$ and the baryon rest-mass ratio $Q_M$ to be in the range 0.85--1. The typical grid size is $(633,633,317)$ for $(x,y,z)$ . We improve several implementations since the latest work. In the present code, the radiation reaction of gravitational waves is taken into account with a good accuracy. This fact enables us to follow the coalescence all the way from the late inspiral phase through the merger phase for which the transition is triggered by the radiation reaction. It is found that if the total rest-mass of the system is more than $\sim 1.7$ times of the maximum allowed rest-mass of spherical neutron stars, a black hole is formed after the merger irrespective of the mass ratios. The gravitational waveforms and outcomes in the merger of unequal-mass binaries are compared with those in equal-mass binaries. It is found that the disk mass around the so formed black holes increases with decreasing rest-mass ratios and decreases with increasing compactness of neutron stars. The merger process and the gravitational waveforms also depend strongly on the rest-mass ratios even for the range $Q_M= 0.85$--1., Comment: 32 pages, PRD68 to be published

Published
2003
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208. Various features of quasiequilibrium sequences of binary neutron stars in general relativity

Author

Taniguchi, Keisuke, Gourgoulhon, Eric, Taniguchi, Keisuke, and Gourgoulhon, Eric

Abstract

Quasiequilibrium sequences of binary neutron stars are numerically calculated in the framework of the Isenberg-Wilson-Mathews (IWM) approximation of general relativity. The results are presented for both rotation states of synchronized spins and irrotational motion, the latter being considered as the realistic one for binary neutron stars just prior to the merger. We assume a polytropic equation of state and compute several evolutionary sequences of binary systems composed of different-mass stars as well as identical-mass stars with adiabatic indices gamma=2.5, 2.25, 2, and 1.8. From our results, we propose as a conjecture that if the turning point of binding energy (and total angular momentum) locating the innermost stable circular orbit (ISCO) is found in Newtonian gravity for some value of the adiabatic index gamma_0, that of the ADM mass (and total angular momentum) should exist in the IWM approximation of general relativity for the same value of the adiabatic index., Comment: Text improved, some figures changed or deleted, new table, 38 pages, 31 figures, accepted for publication in Phys. Rev. D

Published
2003
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212. DECIGO and DECIGO pathfinder

Author

Ando, Masaki, primary, Kawamura, Seiji, additional, Seto, Naoki, additional, Sato, Shuichi, additional, Nakamura, Takashi, additional, Tsubono, Kimio, additional, Takashima, Takeshi, additional, Funaki, Ikkoh, additional, Numata, Kenji, additional, Kanda, Nobuyuki, additional, Tanaka, Takahiro, additional, Ioka, Kunihito, additional, Agatsuma, Kazuhiro, additional, Aoyanagi, Koh-suke, additional, Arai, Koji, additional, Araya, Akito, additional, Asada, Hideki, additional, Aso, Yoichi, additional, Chiba, Takeshi, additional, Ebisuzaki, Toshikazu, additional, Ejiri, Yumiko, additional, Enoki, Motohiro, additional, Eriguchi, Yoshiharu, additional, Fujimoto, Masa-Katsu, additional, Fujita, Ryuichi, additional, Fukushima, Mitsuhiro, additional, Futamase, Toshifumi, additional, Harada, Tomohiro, additional, Hashimoto, Tatsuaki, additional, Hayama, Kazuhiro, additional, Hikida, Wataru, additional, Himemoto, Yoshiaki, additional, Hirabayashi, Hisashi, additional, Hiramatsu, Takashi, additional, Hong, Feng-Lei, additional, Horisawa, Hideyuki, additional, Hosokawa, Mizuhiko, additional, Ichiki, Kiyotomo, additional, Ikegami, Takeshi, additional, Inoue, Kaiki T, additional, Ishidoshiro, Koji, additional, Ishihara, Hideki, additional, Ishikawa, Takehiko, additional, Ishizaki, Hideharu, additional, Ito, Hiroyuki, additional, Itoh, Yousuke, additional, Izumi, Kiwamu, additional, Kawano, Isao, additional, Kawashima, Nobuki, additional, Kawazoe, Fumiko, additional, Kishimoto, Naoko, additional, Kiuchi, Kenta, additional, Kobayashi, Shiho, additional, Kohri, Kazunori, additional, Koizumi, Hiroyuki, additional, Kojima, Yasufumi, additional, Kokeyama, Keiko, additional, Kokuyama, Wataru, additional, Kotake, Kei, additional, Kozai, Yoshihide, additional, Kunimori, Hiroo, additional, Kuninaka, Hitoshi, additional, Kuroda, Kazuaki, additional, Maeda, Kei-ichi, additional, Matsuhara, Hideo, additional, Mino, Yasushi, additional, Miyakawa, Osamu, additional, Miyamoto, Umpei, additional, Miyoki, Shinji, additional, Morimoto, Mutsuko Y, additional, Morisawa, Toshiyuki, additional, Moriwaki, Shigenori, additional, Mukohyama, Shinji, additional, Musha, Mitsuru, additional, Nagano, Shigeo, additional, Naito, Isao, additional, Nakamura, Kouji, additional, Nakamura, Masahiro, additional, Nakano, Hiroyuki, additional, Nakao, Kenichi, additional, Nakasuka, Shinichi, additional, Nakayama, Yoshinori, additional, Nakazawa, Kazuhiro, additional, Nishida, Erina, additional, Nishiyama, Kazutaka, additional, Nishizawa, Atsushi, additional, Niwa, Yoshito, additional, Noumi, Taiga, additional, Obuchi, Yoshiyuki, additional, Ohashi, Masatake, additional, Ohishi, Naoko, additional, Ohkawa, Masashi, additional, Okada, Kenshi, additional, Okada, Norio, additional, Oohara, Kenichi, additional, Sago, Norichika, additional, Saijo, Motoyuki, additional, Saito, Ryo, additional, Sakagami, Masaaki, additional, Sakai, Shin-ichiro, additional, Sakata, Shihori, additional, Sasaki, Misao, additional, Sato, Takashi, additional, Shibata, Masaru, additional, Shinkai, Hisaaki, additional, Somiya, Kentaro, additional, Sotani, Hajime, additional, Sugiyama, Naoshi, additional, Suwa, Yudai, additional, Suzuki, Rieko, additional, Tagoshi, Hideyuki, additional, Takahashi, Fuminobu, additional, Takahashi, Kakeru, additional, Takahashi, Keitaro, additional, Takahashi, Ryutaro, additional, Takahashi, Ryuichi, additional, Takahashi, Tadayuki, additional, Takahashi, Hirotaka, additional, Akiteru, Takamori, additional, Takano, Tadashi, additional, Taniguchi, Keisuke, additional, Taruya, Atsushi, additional, Tashiro, Hiroyuki, additional, Torii, Yasuo, additional, Toyoshima, Morio, additional, Tsujikawa, Shinji, additional, Tsunesada, Yoshiki, additional, Ueda, Akitoshi, additional, Ueda, Ken-ichi, additional, Utashima, Masayoshi, additional, Wakabayashi, Yaka, additional, Yagi, Kent, additional, Yamakawa, Hiroshi, additional, Yamamoto, Kazuhiro, additional, Yamazaki, Toshitaka, additional, Yokoyama, Jun'ichi, additional, Yoo, Chul-Moon, additional, Yoshida, Shijun, additional, Yoshino, Taizoh, additional, and Sun, Ke-Xun, additional

Published
2010
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214. Quasiequilibrium sequences of synchronized and irrotational binary neutron stars in general relativity. III. Identical and different mass stars with gamma=2

Author

Taniguchi, Keisuke, Gourgoulhon, Eric, Taniguchi, Keisuke, and Gourgoulhon, Eric

Abstract

We present the first computations of quasiequilibrium binary neutron stars with different mass components in general relativity, within the Isenberg-Wilson-Mathews approximation. We consider both cases of synchronized rotation and irrotational motion. A polytropic equation of state is used with the adiabatic index gamma=2. The computations have been performed for the following combinations of stars: (M/R)_{star 1} vs. (M/R)_{star 2} = 0.12 vs. (0.12, 0.13, 0.14), 0.14 vs. (0.14, 0.15, 0.16), 0.16 vs. (0.16, 0.17, 0.18), and 0.18 vs. 0.18, where (M/R) denotes the compactness parameter of infinitely separated stars of the same baryon number. It is found that for identical mass binary systems there is no turning point of the binding energy (ADM mass) before the end point of the sequence (mass shedding point) in the irrotational case, while there is one before the end point of the sequence (contact point) in the synchronized case. On the other hand, in the different mass case, the sequence ends by the tidal disruption of the less massive star (mass shedding point). It is then more difficult to find a turning point in the ADM mass. Furthermore, we find that the deformation of each star depends mainly on the orbital separation and the mass ratio and very weakly on its compactness. On the other side, the decrease of the central energy density depends on the compactness of the star and not on that of the companion., Comment: 17 pages, revtex file with 14 figures and 4 tables, accepted for publication in Phys. Rev. D

Published
2002
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215. Measuring Neutron Star Radii with Gravitational Wave Detectors

Author

Faber, Joshua A., Grandclement, Philippe, Rasio, Frederic A., Taniguchi, Keisuke, Faber, Joshua A., Grandclement, Philippe, Rasio, Frederic A., and Taniguchi, Keisuke

Abstract

Coalescing binary neutron stars (NS) are expected to be an important source of gravitational waves (GW) detectable by laser interferometers. We present here a simple method for determining the compactness ratio M/R of NS based on the observed deviation of the GW energy spectrum from point-mass behavior at the end of an inspiral event. Our method is based on the properties of quasi-equilibrium binary NS sequences and does not require the computation of the full GW signal h(t). Combined with the measurement of the NS masses from the GW signal during inspiral, the determination of M/R will allow very strong constraints to be placed on the equation of state of nuclear matter at high densities., Comment: Minor revisions and ref. updates, RevTeX4, 6 pages, 2 figures, accepted by Phys. Rev. Lett

Published
2002
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216. The Japanese space gravitational wave antenna: DECIGO

Author

Chen, Dan, Hong, Feng-Lei, Ichiki, Kiyotomo, Ikegami, Takeshi, Inoue, Kaiki T., Ishidoshiro, Koji, Ishihara, Hideki, Ishizaki, Hideharu, Ito, Hiroyuki, Itoh, Yousuke, Izumi, Kiwamu, Kawashima, Nobuki, Kawazoe, Fumiko, Kishimoto, Naoko, Kiuchi, Kenta, Kobayashi, Shiho, Kohri, Kazunori, Kojima, Yasufumi, Kokeyama, Keiko, Kokuyama, Wataru, Kotake, Kei, Kozai, Yoshihide, Kunimori, Hiroo, Kuroda, Kazuaki, Kuroyanagi, Sachiko, Maeda, Kei-ichi, Matsumoto, Nobuyuki, Michimura, Yuta, Miyakawa, Osamu, Miyamoto, Umpei, Miyoki, Shinji, Morisawa, Toshiyuki, Moriwaki, Shigenori, Mukohyama, Shinji, Musha, Mitsuru, Nagano, Shigeo, Naito, Isao, Nakamura, Kouji, Nakano, Hiroyuki, Nakao, Kenichi, Nakasuka, Shinichi, Nakayama, Yoshinori, Nakazawa, Kazuhiro, Nishida, Erina, Nishizawa, Atsushi, Niwa, Yoshito, Noumi, Taiga, Obuchi, Yoshiyuki, Ohashi, Masatake, Ohishi, Naoko, Ohkawa, Masashi, Okada, Kenshi, Okada, Norio, Oohara, Kenichi, Sago, Norichika, Saijo, Motoyuki, Saito, Ryo, Sakagami, Masaaki, Sakata, Shihori, Sasaki, Misao, Sato, Takashi, Shibata, Masaru, Shinkai, Hisaaki, Shoda, Ayaka, Somiya, Kentaro, Sotani, Hajime, Sugiyama, Naoshi, Suwa, Yudai, Suzuki, Rieko, Tagoshi, Hideyuki, Takahashi, Fuminobu, Takahashi, Kakeru, Takahashi, Keitaro, Takahashi, Ryutaro, Takahashi, Ryuichi, Takahashi, Hirotaka, Akiteru, Takamori, Takano, Tadashi, Tanaka, Nobuyuki, Taniguchi, Keisuke, Taruya, Atsushi, Tashiro, Hiroyuki, Torii, Yasuo, Toyoshima, Morio, Tsujikawa, Shinji, Tsunesada, Yoshiki, Ueda, Akitoshi, Ueda, Ken-ichi, Wakabayashi, Yaka, Yagi, Kent, Yamakawa, Hiroshi, Yamamoto, Kazuhiro, Yamazaki, Toshitaka, Yoo, Chul-Moon, Yoshida, Shijun, Yoshino, Taizoh, Sun, Ke-Xun, Kawamura, Seiji, Ando, Masaki, Seto, Naoki, Sato, Shuichi, Nakamura, Takashi, Tsubono, Kimio, Kanda, Nobuyuki, Tanaka, Takahiro, Yokoyama, Jun'ichi, Funaki, Ikkoh, Numata, Kenji, Ioka, Kunihito, Takashima, Takeshi, Agatsuma, Kazuhiro, Akutsu, Tomotada, Aoyanagi, Koh-suke, Arai, Koji, Araya, Akito, Asada, Hideki, Aso, Yoichi, Chiba, Takeshi, Ebisuzaki, Toshikazu, Ejiri, Yumiko, Enoki, Motohiro, Eriguchi, Yoshiharu, Fujimoto, Masa-Katsu, Fujita, Ryuichi, Fukushima, Mitsuhiro, Futamase, Toshifumi, Harada, Tomohiro, Hashimoto, Tatsuaki, Hayama, Kazuhiro, Hikida, Wataru, Himemoto, Yoshiaki, Hirabayashi, Hisashi, Hiramatsu, Takashi, Horisawa, Hideyuki, Hosokawa, Mizuhiko, Ishikawa, Takehiko, Kawano, Isao, Koizumi, Hiroyuki, Kuninaka, Hitoshi, Matsuhara, Hideo, Morimoto, Mutsuko Y., Nishiyama, Kazutaka, Sakai, Shin-ichiro, Takahashi, Tadayuki, and Utashima, Masayoshi

Subjects
Physics, Optics, Physics and Astronomy (miscellaneous), Gravitational wave, business.industry, Big Bang Observer, Antenna (radio), Space (mathematics), business
Abstract

著者人数: 145名, 資料番号: SA1002921000

Published
2011

219. DECIGO: The Japanese space gravitational wave antenna

Author

Sato, Shuichi, primary, Kawamura, Seiji, additional, Ando, Masaki, additional, Nakamura, Takashi, additional, Tsubono, Kimio, additional, Araya, Akito, additional, Funaki, Ikkoh, additional, Ioka, Kunihito, additional, Kanda, Nobuyuki, additional, Moriwaki, Shigenori, additional, Musha, Mitsuru, additional, Nakazawa, Kazuhiro, additional, Numata, Kenji, additional, Sakai, Shin-ichiro, additional, Seto, Naoki, additional, Takashima, Takeshi, additional, Tanaka, Takahiro, additional, Agatsuma, Kazuhiro, additional, Aoyanagi, Koh-suke, additional, Arai, Koji, additional, Asada, Hideki, additional, Aso, Yoichi, additional, Chiba, Takeshi, additional, Ebisuzaki, Toshikazu, additional, Ejiri, Yumiko, additional, Enoki, Motohiro, additional, Eriguchi, Yoshiharu, additional, Fujimoto, Masa-Katsu, additional, Fujita, Ryuichi, additional, Fukushima, Mitsuhiro, additional, Futamase, Toshifumi, additional, Ganzu, Katsuhiko, additional, Harada, Tomohiro, additional, Hashimoto, Tatsuaki, additional, Hayama, Kazuhiro, additional, Hikida, Wataru, additional, Himemoto, Yoshiaki, additional, Hirabayashi, Hisashi, additional, Hiramatsu, Takashi, additional, Hong, Feng-Lei, additional, Horisawa, Hideyuki, additional, Hosokawa, Mizuhiko, additional, Ichiki, Kiyotomo, additional, Ikegami, Takeshi, additional, Inoue, Kaiki T, additional, Ishidoshiro, Koji, additional, Ishihara, Hideki, additional, Ishikawa, Takehiko, additional, Ishizaki, Hideharu, additional, Ito, Hiroyuki, additional, Itoh, Yousuke, additional, Kawashima, Nobuki, additional, Kawazoe, Fumiko, additional, Kishimoto, Naoko, additional, Kiuchi, Kenta, additional, Kobayashi, Shiho, additional, Kohri, Kazunori, additional, Koizumi, Hiroyuki, additional, Kojima, Yasufumi, additional, Kokeyama, Keiko, additional, Kokuyama, Wataru, additional, Kotake, Kei, additional, Kozai, Yoshihide, additional, Kudoh, Hideaki, additional, Kunimori, Hiroo, additional, Kuninaka, Hitoshi, additional, Kuroda, Kazuaki, additional, Maeda, Kei-ichi, additional, Matsuhara, Hideo, additional, Mino, Yasushi, additional, Miyakawa, Osamu, additional, Miyoki, Shinji, additional, Morimoto, Mutsuko Y, additional, Morioka, Tomoko, additional, Morisawa, Toshiyuki, additional, Mukohyama, Shinji, additional, Nagano, Shigeo, additional, Naito, Isao, additional, Nakamura, Kouji, additional, Nakano, Hiroyuki, additional, Nakao, Kenichi, additional, Nakasuka, Shinichi, additional, Nakayama, Yoshinori, additional, Nishida, Erina, additional, Nishiyama, Kazutaka, additional, Nishizawa, Atsushi, additional, Niwa, Yoshito, additional, Noumi, Taiga, additional, Obuchi, Yoshiyuki, additional, Ohashi, Masatake, additional, Ohishi, Naoko, additional, Ohkawa, Masashi, additional, Okada, Norio, additional, Onozato, Kouji, additional, Oohara, Kenichi, additional, Sago, Norichika, additional, Saijo, Motoyuki, additional, Sakagami, Masaaki, additional, Sakata, Shihori, additional, Sasaki, Misao, additional, Sato, Takashi, additional, Shibata, Masaru, additional, Shinkai, Hisaaki, additional, Somiya, Kentaro, additional, Sotani, Hajime, additional, Sugiyama, Naoshi, additional, Suwa, Yudai, additional, Suzuki, Rieko, additional, Tagoshi, Hideyuki, additional, Takahashi, Fuminobu, additional, Takahashi, Kakeru, additional, Takahashi, Keitaro, additional, Takahashi, Ryutaro, additional, Takahashi, Ryuichi, additional, Takahashi, Tadayuki, additional, Takahashi, Hirotaka, additional, Akiteru, Takamori, additional, Takano, Tadashi, additional, Taniguchi, Keisuke, additional, Taruya, Atsushi, additional, Tashiro, Hiroyuki, additional, Torii, Yasuo, additional, Toyoshima, Morio, additional, Tsujikawa, Shinji, additional, Tsunesada, Yoshiki, additional, Ueda, Akitoshi, additional, Ueda, Ken-ichi, additional, Utashima, Masayoshi, additional, Wakabayashi, Yaka, additional, Yamakawa, Hiroshi, additional, Yamamoto, Kazuhiro, additional, Yamazaki, Toshitaka, additional, Yokoyama, Jun'ichi, additional, Yoo, Chul-Moon, additional, Yoshida, Shijun, additional, and Yoshino, Taizoh, additional

Published
2009
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222. Quasiequilibrium sequences of synchronized and irrotational binary neutron stars in general relativity. II. Newtonian limits

Author

Taniguchi, Keisuke, Gourgoulhon, Eric, Bonazzola, Silvano, Taniguchi, Keisuke, Gourgoulhon, Eric, and Bonazzola, Silvano

Abstract

We study equilibrium sequences of close binary systems composed of identical polytropic stars in Newtonian gravity. The solving method is a multi-domain spectral method which we have recently developed. An improvement is introduced here for accurate computations of binary systems with stiff equation of state ($\gamma > 2$). The computations are performed for both cases of synchronized and irrotational binary systems with adiabatic indices $\gamma=3,~2.5,~2.25,~2$ and 1.8. It is found that the turning points of total energy along a constant-mass sequence appear only for $\gamma \ge 1.8$ for synchronized binary systems and $\gamma \ge 2.3$ for irrotational ones. In the synchronized case, the equilibrium sequences terminate by the contact between the two stars. On the other hand, for irrotational binaries, it is found that the sequences terminate at a mass shedding limit which corresponds to a detached configuration., Comment: 27 pages, 2 tables, 34 figures, revtex, added one more figure and its explanation, accepted to Phys. Rev. D

Published
2001
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223. Equilibrium sequences of synchronized and irrotational binary systems composed of different mass stars in Newtonian gravity

Author

Taniguchi, Keisuke, Gourgoulhon, Eric, Taniguchi, Keisuke, and Gourgoulhon, Eric

Abstract

We study equilibrium sequences of close binary systems on circular orbits and composed of different mass stars with polytropic equation of state in Newtonian gravity. The solving method is a multidomain spectral method which we have recently developed. The computations are performed for both cases of synchronized and irrotational binary systems with adiabatic indices $\gamma = 3, 2.5, 2.25, 2$ and 1.8, and for three mass ratios: $M_1/M_2 =0.5, 0.2$ and 0.1. It is found that the equilibrium sequences always terminate at a mass shedding limit (appearance of a cusp on the surface of the less massive star). For synchronized binaries, this contrasts with the equal mass case, where the sequences terminate instead by a contact configuration. Regarding the turning point of the total angular momentum (or total energy) along a sequence, we find that it is difficult to get it for small mass ratios. Indeed, we do not find any turning points for $M_1/M_2 \le 0.5$ in the irrotational case. However, in the synchronized case, it becomes easier again to find one for mass ratios much smaller than $M_1/M_2 \sim 0.2$., Comment: 22 pages, 6 tables, 24 figures, revtex, Suppressed much of Sec.II, added some explanations and modified some figures, accepted for publication in Phys. Rev. D

Published
2001
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224. BI-1-7 Space gravitational wave detector : DECIGO & DPF

Author

Musha, Mitsuru, Kawamura, Seiji, Ando, Masaki, Seto, Naoki, Sato, Shuichi, Nakamura, Takashi, Tsubono, Kimio, Takashima, Takeshi, Funaki, Ikko, Numata, Kenji, Kanda, Nobuyuki, Tanaka, Takahiro, Ioka, Kunihito, Aoyagi, Kosuke, Wagatsuma, Kazuhiro, Asada, Hideki, Aso, Yoichi, Arai, Koji, Araya, Akito, Ikegami, Takeshi, Ishikawa, Takehiko, Ishizaki, Hideharu, Ishidoshiro, Koji, Ishihara, Hideki, Izumi, Kiwamu, Ichiki, Kiyotomo, Ito, Hiroyuki, Ito, Yosuke, Inoue, Kaiki, Ueda, Akitoshi, Ueda, Kenichi, Utashima, Masayoshi, Ejiri, Yumiko, Enoki, Motohiro, Ebisuzaki, Toshikazu, Eriguchi, Yoshiharu, Oishi, Naoko, Okawa, Masashi, Ohashi, Masatake, Ohara, Kenichi, Obuchi, Yoshiyuki, Okada, Kenshi, Kawashima, Nobuki, Kawazoe, Fumiko, Kono, Isao, Kiuchi, Kenta, Kishimoto, Naoko, Kuninaka, Hitoshi, Kunimori, Hiro, Kuroda, Kazuaki, Koizumi, Hiroyuki, [checking], Kori, Kazunori, Kokuyama, Wataru, Kokeyama, Keiko, Kozai, Yoshihide, Kojima, Yasufumi, Kotake, Kei, Kobayashi, Shiho, Saijo, Motoyuki, Saito, Ryo, Sakai, Shinichiro, Sakagami, Masaaki, Sakata, Shihori, Sago, Norichika, Sasaki, Takashi, Sato, Takashi, Shibata, Masaru, Shinkai, Hisaaki, Sugiyama, Naoshi, Suzuki, Rieko, Suwa, Yudai, Somiya, Kentaro, Sotani, Hajime, Takano, Tadashi, Takahashi, Kakeru, Takahashi, Keitaro, Takahashi, Tadayuki, Takahashi, Hirotaka, Takahashi, Fuminobu, Takahashi, Ryuichi, Takahashi, Ryutaro, Takamori, Akiteru, Tagoshi, Hideyuki, Tashiro, Hiroyuki, Taniguchi, Keisuke, Taruya, Atsushi, Chiba, Takeshi, Tsujikawa, Shinji, Tsunesada, Yoshiki, Toyoshima, Morio, Torii, Yasuo, Naito, Isao, Nakao, Kenichi, Nakazawa, Kazuhiro, Nakasuka, Shinichi, Nakano, Hiroyuki, Nagano, Shigeo, Nakamura, Koji, Nakamura, Masaharu, Nakayama, Yoshinori, Nishizawa, Atsushi, Nishida, Erina, Nishiyama, Kazutaka, Niwa, Yoshito, Nomi, Taiga, Hashimoto, Tatsuaki, Hayama, Kazuhiro, Harada, Tomohiro, Hikita, Wataru, Himemoto, Yoshiaki, Hirabayashi, Hisashi, Hiramatsu, Naoshi, Fukushima, Mitsuhiro, Fujita, Ryuichi, Fujimoto, Masakatsu, Futamase, Toshifumi, Hosokawa, Mizuhiko, Horisawa, Hideyuki, Maeda, Keiichi, Matsuhara, Hideo, Mino, Yasushi, Miyagawa, Osamu, Miyamoto, Umpei, Miyoki, Shinji, Mukoyama, Shinji, Morisawa, Yoshiyuki, Morimoto, Mutsuko, Moriwaki, Shigenori, Yagi, Kento, Yamakawa, Hiroshi, Yamazaki, Toshitaka, Yamamoto, Kazuhiro, Yokoyama, Junichi, Yoshida, Shijun, Yoshino, Taizo, Wakabayashi, Yaka, and Sun, Ke-Xun

Abstract

本文データは学協会の許諾に基づきCiNiiから複製したものである

Published
2010

226. DECIGO: THE JAPANESE SPACE GRAVITATIONAL WAVE ANTENNA

Author

ANDO, MASAKI, primary, KAWAMURA, SEIJI, additional, NAKAMURA, TAKASHI, additional, SETO, NAOKI, additional, TSUBONO, KIMIO, additional, NUMATA, KENJI, additional, TAKAHASHI, RYUICHI, additional, MUSHA, MITSURU, additional, UEDA, KEN-ICHI, additional, FUNAKI, IKKOH, additional, MORIWAKI, SHIGENORI, additional, TAKASHIMA, TAKESHI, additional, SAKAI, SHIN-ICHIRO, additional, SATO, TAKASHI, additional, KANDA, NOBUYUKI, additional, NAGANO, SHIGEO, additional, HOSOKAWA, MIZUHIKO, additional, ISHIKAWA, TAKEHIKO, additional, SATO, SHUICHI, additional, ASO, YOICHI, additional, MORIMOTO, MUTSUKO Y., additional, AGATSUMA, KAZUHIRO, additional, AKUTSU, TOMOMI, additional, AKUTSU, TOMOTADA, additional, AOYANAGI, KOH-SUKE, additional, ARAI, KOJI, additional, ARASE, YUTA, additional, ARAYA, AKITO, additional, ASADA, HIDEKI, additional, CHIBA, TAKESHI, additional, EBISUZAKI, TOSHIKAZU, additional, ENOKI, MOTOHIRO, additional, ERIGUCHI, YOSHIHARU, additional, HONG, FENG-LEI, additional, FUJIMOTO, MASA-KATSU, additional, FUKUSHIMA, MITSUHIRO, additional, FUTAMASE, TOSHIFUMI, additional, GANZU, KATSUHIKO, additional, HARADA, TOMOHIRO, additional, HASHIMOTO, TATSUAKI, additional, HAYAMA, KAZUHIRO, additional, HIKIDA, WATARU, additional, HIMEMOTO, YOSHIAKI, additional, HIRABAYASHI, HISASHI, additional, HIRAMATSU, TAKASHI, additional, HORISAWA, HIDEYUKI, additional, ICHIKI, KIYOTOMO, additional, IKEGAMI, TAKESHI, additional, INOUE, KAIKI T., additional, IOKA, KUNIHITO, additional, ISHIDOSHIRO, KOJI, additional, ITO, HIROYUKI, additional, ITOH, YOUSUKE, additional, KAMAGASAKO, SHOGO, additional, KAWASHIMA, NOBUKI, additional, KAWAZOE, FUMIKO, additional, KIRIHARA, HIROYUKI, additional, KISHIMOTO, NAOKO, additional, KIUCHI, KENTA, additional, KLAUS, WERNER, additional, KOBAYASHI, SHIHO, additional, KOHRI, KAZUNORI, additional, KOIZUMI, HIROYUKI, additional, KOJIMA, YASUFUMI, additional, KOKEYAMA, KEIKO, additional, KOKUYAMA, WATARU, additional, KOTAKE, KEI, additional, KOZAI, YOSHIHIDE, additional, KUDOH, HIDEAKI, additional, KUNIMORI, HIROO, additional, KUNINAKA, HITOSHI, additional, KURODA, KAZUAKI, additional, MAEDA, KEI-ICHI, additional, MATSUHARA, HIDEO, additional, MINO, YASUSHI, additional, MIURA, JUN-ICHI, additional, MIYAKAWA, OSAMU, additional, MIYOKI, SHINJI, additional, MORIOKA, TOMOKO, additional, MORISAWA, TOSHIYUKI, additional, MUKOHYAMA, SHINJI, additional, NAITO, ISAO, additional, NAKAGAWA, NORIYASU, additional, NAKAMURA, KOUJI, additional, NAKANO, HIROYUKI, additional, NAKAO, KENICHI, additional, NAKASUKA, SHINICHI, additional, NAKAYAMA, YOSHINORI, additional, NISHIDA, ERINA, additional, NISHIYAMA, KAZUTAKA, additional, NISHIZAWA, ATSUSHI, additional, NIWA, YOSHITO, additional, OHASHI, MASATAKE, additional, OHISHI, NAOKO, additional, OHKAWA, MASASHI, additional, OKUTOMI, AKIRA, additional, ONOZATO, KOUJI, additional, OOHARA, KENICHI, additional, SAGO, NORICHIKA, additional, SAIJO, MOTOYUKI, additional, SAKAGAMI, MASAAKI, additional, SAKATA, SHIHORI, additional, SASAKI, MISAO, additional, SHIBATA, MASARU, additional, SHINKAI, HISAAKI, additional, SOMIYA, KENTARO, additional, SOTANI, HAJIME, additional, SUGIYAMA, NAOSHI, additional, TAGOSHI, HIDEYUKI, additional, TAKAHASHI, TADAYUKI, additional, TAKAHASHI, RYUTARO, additional, TAKAHASHI, KAKERU, additional, TAKAHASHI, HIROTAKA, additional, AKITERU, TAKAMORI, additional, TAKANO, TADASHI, additional, TANAKA, TAKAHIRO, additional, TANIGUCHI, KEISUKE, additional, TARUYA, ATSUSHI, additional, TASHIRO, HIROYUKI, additional, TOKUDA, MITSURU, additional, TOKUNARI, MASAO, additional, TOYOSHIMA, MORIO, additional, TSUJIKAWA, SHINJI, additional, TSUNESADA, YOSHIKI, additional, UTASHIMA, MASAYOSHI, additional, YAMAKAWA, HIROSHI, additional, YAMAMOTO, KAZUHIRO, additional, YAMAZAKI, TOSHITAKA, additional, YOKOYAMA, JUN'ICHI, additional, YOO, CHUL-MOON, additional, YOSHIDA, SHIJUN, additional, and YOSHINO, TAIZOH, additional

Published
2008
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231. Equilibrium sequences of irrotational binary polytropic stars : The case of double polytropic stars

Author

Taniguchi, Keisuke, Nakamura, Takashi, Taniguchi, Keisuke, and Nakamura, Takashi

Abstract

Solutions to equilibrium sequences of irrotational binary polytropic stars in Newtonian gravity are expanded in a power of $\epsilon=a_0/R$, where R and $a_0$ are the orbital separation of the binary system and the radius of each star for $R=\infty$. For each order of $\epsilon$, we should solve ordinary differential equations for arbitrary polytropic indices n. We show solutions for polytropic indices n= 0.5, 1, 1.5 and 2 up to $\epsilon^6$ orders. Our semi-analytic solutions can be used to check the validity of numerical solutions., Comment: 59 pages including 15 tables and 13 figures, revtex, accepted to Phys. Rev. D

Published
2000
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232. Gravitational waves from inspiralling compact binaries with magnetic dipole moments

Author

Ioka, Kunihito, Taniguchi, Keisuke, Ioka, Kunihito, and Taniguchi, Keisuke

Abstract

We investigate the effects of the magnetic dipole-dipole coupling and the electromagnetic radiation on the frequency evolution of gravitational waves from inspiralling binary neutron stars with magnetic dipole moments. This study is motivated by the discovery of the superstrongly magnetized neutron stars, i.e., magnetar. We derive the contributions of the magnetic fields to the accumulated cycles in gravitational waves as $N_{mag} \sim 6 \times 10^{-3} (H/10^{16}{\rm G})^{2}$, where $H$ denotes the strength of the polar magnetic fields of each neutron star in the binary system. It is found that the effects of the magnetic fields will be negligible for the detection and the parameter estimation of gravitational waves, if the upper limit for magnetic fields of neutron stars are less than $\sim 10^{16}$G, which is the maximum magnetic field observed in the soft gamma repeaters and the anomalous X-ray pulsars up to date. We also discuss the implications of electromagnetic radiation from the inspiralling binary neutron stars for the precursory X-ray emission prior to the gamma ray burst observed by the Ginga satellite., Comment: 15 pages, no figures, accepted for publication in ApJ

Published
2000
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237. Irrotational and Incompressible Binary Systems in the First Post-Newtonian Approximation of General Relativity

Author

Taniguchi, Keisuke and Taniguchi, Keisuke

Abstract

The first post-Newtonian (PN) hydrostatic equations for an irrotational fluid are solved for an incompressible binary system. The equilibrium configuration of the binary system is given by a small deformation from the irrotational Darwin-Riemann ellipsoid which is the solution at Newtonian order. It is found that the orbital separation at the innermost stable circular orbit (ISCO) decreases when one increases the compactness parameter $M_{\ast}/c^2 a_{\ast}$, in which $M_{\ast}$ and $a_{\ast}$ denote the mass and the radius of a star, respectively. If we compare the 1PN angular velocity of the binary system at the ISCO in units of $\sqrt{M_{\ast}/a_{\ast}^3}$ with that of Newtonian order, the angular velocity at the ISCO is almost the same value as that at Newtonian order when one increases the compactness parameter. Also, we do not find the instability point driven by the deformation at 1PN order, where a new sequence bifurcates throughout the equilibrium sequence of the binary system until the ISCO. We also investigate the validity of an ellipsoidal approximation, in which a 1PN solution is obtained assuming an ellipsoidal figure and neglecting the deformation. It is found that the ellipsoidal approximation gives a fairly accurate result for the total energy, total angular momentum and angular velocity. However, if we neglect the velocity potential of 1PN order, we tend to overestimate the angular velocity at the ISCO regardless of the shape of the star (ellipsoidal figure or deformed figure)., Comment: 36 pages with 5 figures, revtex, Prog. Theor. Phys. in press

Published
1999
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238. Almost analytic solutions to equilibrium sequences of irrotational binary polytropic stars for n=1

Author

Taniguchi, Keisuke, Nakamura, Takashi, Taniguchi, Keisuke, and Nakamura, Takashi

Abstract

A solution to an equilibrium of irrotational binary polytropic stars in Newtonian gravity is expanded in a power of \epsilon=a_0/R, where R and a_0 are the separation of the binary system and the radius of each star for R=\infty. For the polytropic index n=1, the solutions are given almost analytically up to order \epsilon^6. We have found that in general an equilibrium solution should have the velocity component along the orbital axis and that the central density should decrease when R decreases. Our almost analytic solutions can be used to check the validity of numerical solutions., Comment: 4 pages, 2 figures, revtex, accepted to Phys. Rev. Lett

Published
1999
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239. Results of the search for inspiraling compact star binaries from TAMA300’s observation in 2000–2004

Author

Akutsu, Tomomi, primary, Akutsu, Tomotada, additional, Ando, Masaki, additional, Arai, Koji, additional, Araya, Akito, additional, Asada, Hideki, additional, Aso, Youichi, additional, Barton, Mark A., additional, Beyersdorf, Peter, additional, Fujiki, Youhei, additional, Fujimoto, Masa-Katsu, additional, Fujita, Ryuichi, additional, Fukushima, Mitsuhiro, additional, Futamase, Toshifumi, additional, Hamuro, Yusaku, additional, Haruyama, Tomiyoshi, additional, Hayakawa, Hideaki, additional, Hayama, Kazuhiro, additional, Heinzel, Gerhard, additional, Horikoshi, Gen’ichi, additional, Iguchi, Hideo, additional, Iida, Yukiyoshi, additional, Ioka, Kunihito, additional, Ishitsuka, Hideki, additional, Kamikubota, Norihiko, additional, Kanda, Nobuyuki, additional, Kaneyama, Takaharu, additional, Karasawa, Yoshikazu, additional, Kasahara, Kunihiko, additional, Kasai, Taketoshi, additional, Katsuki, Mayu, additional, Kawabe, Keita, additional, Kawamura, Mari, additional, Kawamura, Seiji, additional, Kawashima, Nobuki, additional, Kawazoe, Fumiko, additional, Kojima, Yasufumi, additional, Kokeyama, Keiko, additional, Kondo, Kazuhiro, additional, Kozai, Yoshihide, additional, Kudoh, Hideaki, additional, Kuroda, Kazuaki, additional, Kuwabara, Takashi, additional, Matsuda, Namio, additional, Mio, Norikatsu, additional, Miura, Kazuyuki, additional, Miyakawa, Osamu, additional, Miyama, Shoken, additional, Miyoki, Shinji, additional, Mizusawa, Hiromi, additional, Moriwaki, Shigenori, additional, Musha, Mitsuru, additional, Nagano, Shigeo, additional, Nagayama, Yoshitaka, additional, Nakagawa, Ken’ichi, additional, Nakamura, Takashi, additional, Nakano, Hiroyuki, additional, Nakao, Ken-ichi, additional, Nishi, Yuhiko, additional, Numata, Kenji, additional, Ogawa, Yujiro, additional, Ohashi, Masatake, additional, Ohishi, Naoko, additional, Okutomi, Akira, additional, Oohara, Ken-ichi, additional, Otsuka, Shigemi, additional, Sago, Norichika, additional, Saito, Yoshio, additional, Sakata, Shihori, additional, Sasaki, Misao, additional, Sato, Kouichi, additional, Sato, Nobuaki, additional, Sato, Shuichi, additional, Sato, Youhei, additional, Seki, Hidetsugu, additional, Sekido, Aya, additional, Seto, Naoki, additional, Shibata, Masaru, additional, Shinkai, Hisaaki, additional, Shintomi, Takakazu, additional, Soida, Kenji, additional, Somiya, Kentaro, additional, Suzuki, Toshikazu, additional, Tagoshi, Hideyuki, additional, Takahashi, Hirotaka, additional, Takahashi, Ryutaro, additional, Takamori, Akiteru, additional, Takemoto, Shuzo, additional, Takeno, Kohei, additional, Tanaka, Takahiro, additional, Taniguchi, Keisuke, additional, Taniguchi, Shinsuke, additional, Tanji, Toru, additional, Tatsumi, Daisuke, additional, Taylor, C. T., additional, Telada, Souichi, additional, Tochikubo, Kuniharu, additional, Tokunari, Masao, additional, Tomaru, Takayuki, additional, Tsubono, Kimio, additional, Tsuda, Nobuhiro, additional, Tsunesada, Yoshiki, additional, Uchiyama, Takashi, additional, Ueda, Akitoshi, additional, Ueda, Ken-ichi, additional, Usui, Fumihiko, additional, Waseda, Koichi, additional, Watanabe, Yuko, additional, Yakura, Hiromi, additional, Yamamoto, Akira, additional, Yamamoto, Kazuhiro, additional, Yamazaki, Toshitaka, additional, Yanagi, Yuriko, additional, Yoda, Tatsuo, additional, Yokoyama, Jun’ichi, additional, Yoshida, Tatsuru, additional, and Zhu, Zong-Hong, additional

Published
2006
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242. The Japanese space gravitational wave antenna—DECIGO

Author

Kawamura, Seiji, primary, Nakamura, Takashi, additional, Ando, Masaki, additional, Seto, Naoki, additional, Tsubono, Kimio, additional, Numata, Kenji, additional, Takahashi, Ryuichi, additional, Nagano, Shigeo, additional, Ishikawa, Takehiko, additional, Musha, Mitsuru, additional, Ueda, Ken-ichi, additional, Sato, Takashi, additional, Hosokawa, Mizuhiko, additional, Agatsuma, Kazuhiro, additional, Akutsu, Tomotada, additional, Aoyanagi, Koh-suke, additional, Arai, Koji, additional, Araya, Akito, additional, Asada, Hideki, additional, Aso, Yoichi, additional, Chiba, Takeshi, additional, Ebisuzaki, Toshikazu, additional, Eriguchi, Yoshiharu, additional, Fujimoto, Masa-Katsu, additional, Fukushima, Mitsuhiro, additional, Futamase, Toshifumi, additional, Ganzu, Katsuhiko, additional, Harada, Tomohiro, additional, Hashimoto, Tatsuaki, additional, Hayama, Kazuhiro, additional, Hikida, Wataru, additional, Himemoto, Yoshiaki, additional, Hirabayashi, Hisashi, additional, Hiramatsu, Takashi, additional, Ichiki, Kiyotomo, additional, Ikegami, Takeshi, additional, Inoue, Kaiki T, additional, Ioka, Kunihito, additional, Ishidoshiro, Koji, additional, Itoh, Yousuke, additional, Kamagasako, Shogo, additional, Kanda, Nobuyuki, additional, Kawashima, Nobuki, additional, Kirihara, Hiroyuki, additional, Kiuchi, Kenta, additional, Kobayashi, Shiho, additional, Kohri, Kazunori, additional, Kojima, Yasufumi, additional, Kokeyama, Keiko, additional, Kozai, Yoshihide, additional, Kudoh, Hideaki, additional, Kunimori, Hiroo, additional, Kuroda, Kazuaki, additional, Maeda, Kei-ichi, additional, Matsuhara, Hideo, additional, Mino, Yasushi, additional, Miyakawa, Osamu, additional, Miyoki, Shinji, additional, Mizusawa, Hiromi, additional, Morisawa, Toshiyuki, additional, Mukohyama, Shinji, additional, Naito, Isao, additional, Nakagawa, Noriyasu, additional, Nakamura, Kouji, additional, Nakano, Hiroyuki, additional, Nakao, Kenichi, additional, Nishizawa, Atsushi, additional, Niwa, Yoshito, additional, Nozawa, Choetsu, additional, Ohashi, Masatake, additional, Ohishi, Naoko, additional, Ohkawa, Masashi, additional, Okutomi, Akira, additional, Oohara, Kenichi, additional, Sago, Norichika, additional, Saijo, Motoyuki, additional, Sakagami, Masaaki, additional, Sakata, Shihori, additional, Sasaki, Misao, additional, Sato, Shuichi, additional, Shibata, Masaru, additional, Shinkai, Hisaaki, additional, Somiya, Kentaro, additional, Sotani, Hajime, additional, Sugiyama, Naoshi, additional, Tagoshi, Hideyuki, additional, Takahashi, Tadayuki, additional, Takahashi, Hirotaka, additional, Takahashi, Ryutaro, additional, Takano, Tadashi, additional, Tanaka, Takahiro, additional, Taniguchi, Keisuke, additional, Taruya, Atsushi, additional, Tashiro, Hiroyuki, additional, Tokunari, Masao, additional, Tsujikawa, Shinji, additional, Tsunesada, Yoshiki, additional, Yamamoto, Kazuhiro, additional, Yamazaki, Toshitaka, additional, Yokoyama, Jun'ichi, additional, Yoo, Chul-Moon, additional, Yoshida, Shijun, additional, and Yoshino, Taizoh, additional

Published
2006
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247. Observation results by the TAMA300 detector on gravitational wave bursts from stellar-core collapses

Author

Ando, Masaki, primary, Arai, Koji, additional, Aso, Youichi, additional, Beyersdorf, Peter, additional, Hayama, Kazuhiro, additional, Iida, Yukiyoshi, additional, Kanda, Nobuyuki, additional, Kawamura, Seiji, additional, Kondo, Kazuhiro, additional, Mio, Norikatsu, additional, Miyoki, Shinji, additional, Moriwaki, Shigenori, additional, Nagano, Shigeo, additional, Numata, Kenji, additional, Sato, Shuichi, additional, Somiya, Kentaro, additional, Tagoshi, Hideyuki, additional, Takahashi, Hirotaka, additional, Takahashi, Ryutaro, additional, Tatsumi, Daisuke, additional, Tsunesada, Yoshiki, additional, Zhu, Zong-Hong, additional, Akutsu, Tomomi, additional, Akutsu, Tomotada, additional, Araya, Akito, additional, Asada, Hideki, additional, Barton, Mark A., additional, Fujiki, Youhei, additional, Fujimoto, Masa-Katsu, additional, Fujita, Ryuichi, additional, Fukushima, Mitsuhiro, additional, Futamase, Toshifumi, additional, Hamuro, Yusaku, additional, Haruyama, Tomiyoshi, additional, Hayakawa, Hideaki, additional, Heinzel, Gerhard, additional, Horikoshi, Gen’ichi, additional, Iguchi, Hideo, additional, Ioka, Kunihito, additional, Ishitsuka, Hideki, additional, Kamikubota, Norihiko, additional, Kaneyama, Takaharu, additional, Karasawa, Yoshikazu, additional, Kasahara, Kunihiko, additional, Kasai, Taketoshi, additional, Katsuki, Mayu, additional, Kawabe, Keita, additional, Kawamura, Mari, additional, Kawashima, Nobuki, additional, Kawazoe, Fumiko, additional, Kojima, Yasufumi, additional, Kokeyama, Keiko, additional, Kozai, Yoshihide, additional, Kudoh, Hideaki, additional, Kuroda, Kazuaki, additional, Kuwabara, Takashi, additional, Matsuda, Namio, additional, Miura, Kazuyuki, additional, Miyakawa, Osamu, additional, Miyama, Shoken, additional, Mizusawa, Hiromi, additional, Musha, Mitsuru, additional, Nagayama, Yoshitaka, additional, Nakagawa, Ken’ichi, additional, Nakamura, Takashi, additional, Nakano, Hiroyuki, additional, Nakao, Ken-ichi, additional, Nishi, Yuhiko, additional, Ogawa, Yujiro, additional, Ohashi, Masatake, additional, Ohishi, Naoko, additional, Okutomi, Akira, additional, Oohara, Ken-ichi, additional, Otsuka, Shigemi, additional, Saito, Yoshio, additional, Sakata, Shihori, additional, Sasaki, Misao, additional, Sato, Kouichi, additional, Sato, Nobuaki, additional, Sato, Youhei, additional, Seki, Hidetsugu, additional, Sekido, Aya, additional, Seto, Naoki, additional, Shibata, Masaru, additional, Shinkai, Hisaaki, additional, Shintomi, Takakazu, additional, Soida, Kenji, additional, Suzuki, Toshikazu, additional, Takamori, Akiteru, additional, Takemoto, Shuzo, additional, Takeno, Kohei, additional, Tanaka, Takahiro, additional, Taniguchi, Keisuke, additional, Taniguchi, Shinsuke, additional, Tanji, Toru, additional, Taylor, C. T., additional, Telada, Souichi, additional, Tochikubo, Kuniharu, additional, Tokunari, Masao, additional, Tomaru, Takayuki, additional, Tsubono, Kimio, additional, Tsuda, Nobuhiro, additional, Uchiyama, Takashi, additional, Ueda, Akitoshi, additional, Ueda, Ken-ichi, additional, Usui, Fumihiko, additional, Waseda, Koichi, additional, Watanabe, Yuko, additional, Yakura, Hiromi, additional, Yamamoto, Akira, additional, Yamamoto, Kazuhiro, additional, Yamazaki, Toshitaka, additional, Yanagi, Yuriko, additional, Yoda, Tatsuo, additional, Yokoyama, Jun’ichi, additional, and Yoshida, Tatsuru, additional

Published
2005
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