Publication List
(except for collaboration papers of LIGO and KAGRA and conference proceedings)

SAO/NASA Astrophysics Data System (ADS)

Refereed Journal Papars

[32]"Measurement of cosmic expansion rate with stellar-mass binary black hole",
Atsushi Nishizawa,
Physical Review D 96, 101303(R) (2017).

[31]"Testing Gravity with Pulsar Scintillation Measurements",
Huan Yang, Atsushi Nishizawa, and Ue-Li Pen,
Physical Review D 95, 084049 (2017).

[30] "Constraining stellar binary black hole formation scenarios with eLISA eccentricity measurements",
Atsushi Nishizawa, Alberto Sesana, Emanuele Berti, and Antoine Klein,
Monthly Notices of the Royal Astronomical Society 465, 4375 (2017).

[29] "Gravitational wave memory: A new approach to study modified gravity",
Song Ming Du, Atsushi Nishizawa,
Physical Review D 94, 104063 (2016).

[28] "eLISA eccentricity measurements as tracers of binary black hole formation",
Atsushi Nishizawa, Emanuele Berti, Antoine Klein, and Alberto Sesana,
Physical Review D 94, 064020 (2016).

[27] "Detecting Black-Hole Binary Clustering via the Second-Generation Gravitational-Wave Detectors",
Toshiya Namikawa, Atsushi Nishizawa, and Atsushi Taruya,
Physical Review D 94, 024013 (2016).

[26] "Constraining the propagation speed of gravitational waves with compact binaries at cosmological distances",
Atsushi Nishizawa,
Physical Review D 93, 124036 (2016).

[25] "Anisotropies of gravitational-wave standard sirens as a new cosmological probe without redshift information",
Toshiya Namikawa, Atsushi Nishizawa, and Atsushi Taruya,
Physical Review Letters 116, 121302 (2016).

[24] "Weak value amplification and beyond the standard quantum limit in position measurements",
Atsushi Nishizawa,
Physical Review A, 92, 032123 (2015).

[23] "Search for an emission line of a gravitational wave background",
Atsushi Nishizawa and Naoki Seto,
Physical Review D, 91, 122001 (2015).

[22] "Measuring Speed of Gravitational Waves by Observations of Photons and Neutrinos from Compact Binary Mergers and Supernovae",
Atsushi Nishizawa and Takashi Nakamura,
Physical Review D, 90, 044048 (2014).

[21] "Constraint on reheating after f(R) inflation from gravitational waves",
Atsushi Nishizawa and Hayato Motohashi,
Physical Review D, 89, 063541 (2014).

[20] "Probing for massive stochastic gravitational-wave background with a detector network",
Atsushi Nishizawa and Kazuhiro Hayama,
Physical Review D 88, 064005 (2013).

[19] "Beyond Concordance Cosmology with Magnification of Gravitational-Wave Standard Sirens",
Stefano Camera and Atsushi Nishizawa,
Physical Review Letters 110, 151103 (2013).

[18] "Model-independent test of gravity with a network of ground-based gravitational-wave detectors",
Kazuhiro Hayama and Atsushi Nishizawa,
Physical Review D 87, 062003 (2013).

[17] "Reheating after f(R) inflation",
Hayato Motohashi and Atsushi Nishizawa,
Physical Review D, 86, 083514 (2012).

[16] "Weak-value amplification in a shot-noise limited interferometer",
Atsushi Nishizawa, Kouji Nakamura, and Masa-Katsu Fujimoto,
Physical Review A, 85, 062108 (2012).

[15] "Direct Measurement of the Positive Acceleration of the Universe and Testing Inhomogeneous Models under Gravitational Wave Cosmology",
Kent Yagi, Atsushi Nishizawa, and Chul-Moon Yoo,
Journal of Cosmology and Astroparticle Physics, 04, 031 (2012).

[14] "Evaluation of weak measurements to all orders",
Kouji Nakamura, Atsushi Nishizawa, and Masa-Katsu Fujimoto,
Physical Review A, 85, 012113 (2012).

[13] "Cosmology with space-based gravitational-wave detectors: Dark energy and primordial gravitational waves",
Atsushi Nishizawa, Kent Yagi, Atsushi Taruya, and Takahiro Tanaka,
Physical Review D, 85, 044047 (2012).

[12] "Tracing the redshift evolution of Hubble parameter with gravitational-wave standard sirens",
Atsushi Nishizawa, Atsushi Taruya, and Shun Saito,
Physical Review D, 83, 084045 (2011).

[11] "Cosmological test of gravity with polarizations of stochastic gravitational waves around 0.1-1 Hz",
Atsushi Nishizawa, Atsushi Taruya, and Seiji Kawamura,
Physical Review D, 81, 104043 (2010).

[10] "Measurement of angular antispring effect in optical cavity by radiation pressure",
Shihori Sakata, Osamu Miyakawa, Atsushi Nishizawa, Hideharu Ishizaki, and Seiji Kawamura,
Physical Review D, 81, 064023 (2010).

[9] "Development of displacement- and frequency-noise-free interferometer in 3-D configuration for gravitational wave detection",
Keiko Kokeyama, Shuichi Sato, Atsushi Nishizawa, Seiji Kawamura, Yanbei Chen, Akio Sugamoto,
Physical Review Letters, 103, 171101 (2009).

[8] "Probing nontensorial polarizations of stochastic gravitational-wave backgrounds with ground-based laser interferometers",
Atsushi Nishizawa, Atsushi Taruya, Kazuhiro Hayama, Seiji Kawamura, Masa-aki Sakagami,
Physical Review D, 79, 082002 (2009).

[7] "Experimental investigation of a control scheme for a zero-detuning resonant sideband extraction interferometer for next-generation gravitational-wave detectors",
Fumiko Kawazoe, Akio Sugamoto, Volker Leonhardt, Shuichi Sato, Toshitaka Yamazaki, Mitsuhito Fukushima, Seiji Kawamura, Osamu Miyakawa, Kentaro Somiya, Tomoko Morioka, Atsushi Nishizawa,
Classical and Quantum Gravity, 25, 195008 (2008).

[6] "Resonant speed meter for gravitational wave detection",
Atsushi Nishizawa, Seiji Kawamura, Masa-aki Sakagami,
Physical Review Letters, 101, 081101 (2008).

[5] "Search for a stochastic backgrounds of 100-MHz gravitational waves with laser interferometers",
Tomotada Akutsu, Seiji Kawamura, Atsushi Nishizawa, Koji Arai, Kazuhiro Yamamoto, Daisuke Tatsumi, Shigeo Nagano, Erina Nishida, Takeshi Chiba, Ryuichi Takahashi, Naoshi Sugiyama, Mitsuhiro Fukushima, Toshitaka Yamazaki, Masa-katsu Fujimoto,
Physical Review Letters, 101, 101101 (2008).

[4] "Demonstration of displacement-noise-free interferometry using bi-directional Mach-Zehnder interferometers",
Shuichi Sato, Keiko Kokeyama, Seiji Kawamura, Robert L. Ward, Atsushi Nishizawa, Yanbei Chen, Archana Pai, Kentaro Somiya,
Classical and Quantum Gravity, 25, 114031 (2008).

[3] "Optimal Location of Two Laser-interferometric Detectors for Gravitational Wave Backgrounds at 100 MHz",
Atsushi Nishizawa, Seiji Kawamura, Tomotada Akutsu, Koji Arai, Kazuhiro Yamamoto, Daisuke Tatsumi, Erina Nishida, Masa-aki Sakagami, Takeshi Chiba, Ryuichi Takahashi, Naoshi Sugiyama,
Classical and Quantum Gravity, 25, 225011 (2008).

[2] "Laser-interferometric detectors for gravitational wave backgrounds at 100 MHz: Detector design and sensitivity",
Atsushi Nishizawa, Seiji Kawamura, Tomotada Akutsu, Koji Arai, Kazuhiro Yamamoto, Daisuke Tatsumi, Erina Nishida, Masa-aki Sakagami, Takeshi Chiba, Ryuichi Takahashi, Naoshi Sugiyama,
Physical Review D, 77, 022002 (2008).

[1] "Quantum noise in differential-type gravitational-wave interferometer and signal recycling",
Atsushi Nishizawa, Masa-aki Sakagami, Seiji Kawamura,
Physical Review D, 76, 042002 (2007).


Non-refereed Papars
Thesis