Relevant bibliographies by topics / Gravitational wave

Academic literature on the topic 'Gravitational wave'

Author: Grafiati
Published: 4 June 2021
Last updated: 1 April 2023

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Journal articles on the topic "Gravitational wave"

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Cai, Rong-Gen, Zhoujian Cao, Zong-Kuan Guo, Shao-Jiang Wang, and Tao Yang. "The gravitational-wave physics." National Science Review 4, no. 5 (April 4, 2017): 687–706. http://dx.doi.org/10.1093/nsr/nwx029.

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Abstract The direct detection of gravitational wave by Laser Interferometer Gravitational-Wave Observatory indicates the coming of the era of gravitational-wave astronomy and gravitational-wave cosmology. It is expected that more and more gravitational-wave events will be detected by currently existing and planned gravitational-wave detectors. The gravitational waves open a new window to explore the Universe and various mysteries will be disclosed through the gravitational-wave detection, combined with other cosmological probes. The gravitational-wave physics is not only related to gravitation theory, but also is closely tied to fundamental physics, cosmology and astrophysics. In this review article, three kinds of sources of gravitational waves and relevant physics will be discussed, namely gravitational waves produced during the inflation and preheating phases of the Universe, the gravitational waves produced during the first-order phase transition as the Universe cools down and the gravitational waves from the three phases: inspiral, merger and ringdown of a compact binary system, respectively. We will also discuss the gravitational waves as a standard siren to explore the evolution of the Universe.
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Szostek, R., P. Góralski, and K. Szostek. "Gravitational waves in Newton’s gravitation and criticism of gravitational waves resulting from the General Theory of Relativity (LIGO)." Bulletin of the Karaganda University. "Physics" Series 96, no. 4 (December 30, 2019): 39–56. http://dx.doi.org/10.31489/2019ph4/39-56.

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The most important conclusion from this article is that from the General Theory of Relativity do not result any gravitational waves, but just ordinary modulation of the gravitational field intensities caused by rotating of bodies. If the LIGO team has measured anything, it is only this modulation, rather than the gravitational wave understood as the carrier of gravity. This discussion shows that using too complicated mathematics in physics leads to erroneous interpretation of results (in this case, perhaps the tensor analysis is guilty). Formally, various things can be calculated, but without knowing what such analysis means, they can be attributed misinterpreted. Since the modulation of gravitational field intensities has been called a gravitational wave in contemporary physics, we have also done so, although it is misleading. In the article it was shown, that from the Newton’s law of gravitation resulted an existence of gravitational waves very similar to these, which result from the General Theory of Relativity (GTR). The article shows differences between the course of gravitational waves that result from Newton’s gravitation, and the course of gravitational waves that result from the General Theory of Relativity, which measurement was announced by the LIGO (Laser Interferometer Gravitational-Wave Observatory) [1–3]. According to both theories, gravitational waves are cyclical changes of the gravitational field intensities. The article proposes a method of testing a laser interferometer for gravitational wave measurement used in the LIGO Observatory. Criticism of results published by the LIGO team was also presented.
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Wen, Zhao, Zhang Xing, Liu Xiao-jin, Zhang Yang, Wang Yun-yong, Zhang Fan, Zhao Yu-hang, et al. "Gravitational Waves and Gravitational-wave Sourcestwo." Chinese Astronomy and Astrophysics 42, no. 4 (October 2018): 487–526. http://dx.doi.org/10.1016/j.chinastron.2018.10.010.

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Singh, Amit, Ivan Li, Otto Hannuksela, Tjonnie Li, and Kyungmin Kim. "Classifying Lensed Gravitational Waves in the Geometrical Optics Limit with Machine Learning." American Journal of Undergraduate Research 16, no. 2 (September 30, 2019): 5–16. http://dx.doi.org/10.33697/ajur.2019.019.

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Gravitational waves are theorized to be gravitationally lensed when they propagate near massive objects. Such lensing effects cause potentially detectable repeated gravitational wave patterns in ground- and space-based gravitational wave detectors. These effects are difficult to discriminate when the lens is small and the repeated patterns superpose. Traditionally, matched filtering techniques are used to identify gravitational-wave signals, but we instead aim to utilize machine learning techniques to achieve this. In this work, we implement supervised machine learning classifiers (support vector machine, random forest, multi-layer perceptron) to discriminate such lensing patterns in gravitational wave data. We train classifiers with spectrograms of both lensed and unlensed waves using both point-mass and singular isothermal sphere lens models. As the result, classifiers return F1 scores ranging from 0:852 to 0:996, with precisions from 0:917 to 0:992 and recalls ranging from 0:796 to 1:000 depending on the type of classifier and lensing model used. This supports the idea that machine learning classifiers are able to correctly determine lensed gravitational wave signals. This also suggests that in the future, machine learning classifiers may be used as a possible alternative to identify lensed gravitational wave events and to allow us to study gravitational wave sources and massive astronomical objects through further analysis. KEYWORDS: Gravitational Waves; Gravitational Lensing; Geometrical Optics; Machine Learning; Classification; Support Vector Machine; Random Tree Forest; Multi-layer Perceptron
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Argyris, John, and Corneliu Ciubotariu. "A Proposal of New Gravitational Experiments." Modern Physics Letters A 12, no. 40 (December 28, 1997): 3105–19. http://dx.doi.org/10.1142/s0217732397003228.

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Since "evidently the construction of a laboratory generator of gravitational radiation is an unattractive enterprise in the absence of new engineering or a new idea or both" [C. W. Misner, K. S. Thorne and J. A. Wheeler, Gravitation (Freeman, 1973), p. 979], we propose in this letter some new experiments on the physics of gravitation. These experiments refer to: simulation of accelerations produced by a gravity wave, a source of high-frequency gravitational waves, a direct current gravitational machine, materials with high gravitomagnetic permeability, and finally the possibility of an attenuation of the gravitational attraction. The new ideas involve essentially first the concept of a detector or a source of gravitational radiation in the form of a body in which the motions of particles are precisely the same as those induced by a real gravitational wave in that body, and second, to design a detector having two principal components placed at a distance of λ/2 along the direction of propagation of a gravity wave. We define a new type of gravitomagnetic field generated directly by the time-dependent tidal accelerations of the gravitational wave, and we also define a new concept: the gravitational superconductor.
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Winterberg, Friedwardt. "Explanation of the Quantum-Mechanical Particle-Wave Duality through the Emission of Watt-Less Gravitational Waves by the Dirac Equation." Zeitschrift für Naturforschung A 71, no. 1 (January 1, 2016): 53–57. http://dx.doi.org/10.1515/zna-2015-0331.

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AbstractAn explanation of the quantum-mechanical particle-wave duality is given by the watt-less emission of gravitational waves from a particle described by the Dirac equation. This explanation is possible through the existence of negative energy, and hence negative mass solutions of Einstein’s gravitational field equations. They permit to understand the Dirac equation as the equation for a gravitationally bound positive–negative mass (pole–dipole particle) two-body configuration, with the mass of the Dirac particle equal to the positive mass of the gravitational field binding the positive with the negative mass particle, and with the mass particles making a luminal “Zitterbewegung” (quivering motion), emitting a watt-less oscillating positive–negative space curvature wave. It is shown that this thusly produced “Zitterbewegung” reproduces the quantum potential of the Madelung-transformed Schrödinger equation. The watt-less gravitational wave emitted by the quivering particles is conjectured to be de Broglie’s pilot wave. The hypothesised connection of the Dirac equation to gravitational wave physics could, with the failure to detect gravitational waves by the LIGO antennas and pulsar timing arrays, give a clue to extended theories of gravity, or a correction of astrophysical models for the generation of such waves.
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Ferreira, Ivan S., C. Frajuca, Nadja S. Magalhaes, M. D. Maia, and Claudio M. G. Sousa. "The laser gravitational compass: A spheroidal interferometric gravitational observatory." International Journal of Modern Physics A 35, no. 02n03 (January 24, 2020): 2040020. http://dx.doi.org/10.1142/s0217751x20400205.

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Using the observational properties of Einstein’s gravitational field it is shown that a minimum of four non-coplanar mass probes are necessary for a Michelson and Morley interferometer to detect gravitational waves within the context of General Relativity. With fewer probes, some alternative theories of gravitation can also explain the observations. The conversion of the existing gravitational wave detectors to four probes is also suggested.
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Yuan, Tony. "Gravitational fields and gravitational waves." Physics Essays 35, no. 2 (June 26, 2022): 208–19. http://dx.doi.org/10.4006/0836-1398-35.2.208.

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The relative velocity between objects with finite velocity affects the reaction between them. This effect is known as general Doppler effect. The Laser Interferometer Gravitational-Wave Observatory (LIGO) discovered gravitational waves and found their speed to be equal to the speed of light c. Gravitational waves are generated following a disturbance in the gravitational field; they affect the gravitational force on an object. Just as light waves are subject to the Doppler effect, so are gravitational waves. This article explores the following research questions concerning gravitational waves: Is there a linear relationship between gravity and velocity? Can the speed of a gravitational wave represent the speed of the gravitational field (the speed of the action of the gravitational field upon the object)? What is the speed of the gravitational field? What is the spatial distribution of gravitational waves? Do gravitational waves caused by the revolution of the Sun affect planetary precession? Can we modify Newton's gravitational equation through the influence of gravitational waves?
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Biesiada, Marek, and Sreekanth Harikumar. "Gravitational Lensing of Continuous Gravitational Waves." Universe 7, no. 12 (December 17, 2021): 502. http://dx.doi.org/10.3390/universe7120502.

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Continuous gravitational waves are analogous to monochromatic light and could therefore be used to detect wave effects such as interference or diffraction. This would be possible with strongly lensed gravitational waves. This article reviews and summarises the theory of gravitational lensing in the context of gravitational waves in two different regimes: geometric optics and wave optics, for two widely used lens models such as the point mass lens and the Singular Isothermal Sphere (SIS). Observable effects due to the wave nature of gravitational waves are discussed. As a consequence of interference, GWs produce beat patterns which might be observable with next generation detectors such as the ground based Einstein Telescope and Cosmic Explorer, or the space-borne LISA and DECIGO. This will provide us with an opportunity to estimate the properties of the lensing system and other cosmological parameters with alternative techniques. Diffractive microlensing could become a valuable method of searching for intermediate mass black holes formed in the centres of globular clusters. We also point to an interesting idea of detecting the Poisson–Arago spot proposed in the literature.
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Shankaranarayanan, S. "Strong gravity signatures in the polarization of gravitational waves." International Journal of Modern Physics D 28, no. 14 (October 2019): 1944020. http://dx.doi.org/10.1142/s0218271819440206.

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General Relativity is a hugely successful description of gravitation. However, both theory and observations suggest that General Relativity might have significant classical and quantum corrections in the Strong Gravity regime. Testing the strong field limit of gravity is one of the main objectives of the future gravitational wave detectors. One way to detect strong gravity is through the polarization of gravitational waves. For quasi-normal modes of black-holes in General Relativity, the two polarization states of gravitational waves have the same amplitude and frequency spectrum. Using the principle of energy conservation, we show that the polarizations differ for modified gravity theories. We obtain a diagnostic parameter for polarization mismatch that provides a unique way to distinguish General Relativity and modified gravity theories in gravitational wave detectors.
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Dissertations / Theses on the topic "Gravitational wave"

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Takahashi, Ryuichi. "Wave Effects in the Gravitational Lensing of Gravitational Waves from Chirping Binaries." 京都大学 (Kyoto University), 2004. http://hdl.handle.net/2433/147805.

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Herrera, Martín Antonio. "Wave dark matter as a gravitational lens for electromagnetic and gravitational waves." Thesis, University of Glasgow, 2018. http://theses.gla.ac.uk/9027/.

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The majority of the matter in the known universe is believed to be in the form of Dark Matter, and its widely accepted description is done by Cold Dark Matter (CDM). Nevertheless, its exact properties and composition are still unknown, and it is one of the most active areas of research in Cosmology. The use of Cold Dark Matter has been successful to describe the general behaviour of Dark Matter at large scales. However, it has encountered problems explaining phenomena at other regimes as on the scale of galaxy halos. Therefore, other models have been proposed over time which are able to retain the reasonable success of CDM on large scales and extent it to other regimes where CDM has problems to explain the observed data. One of such models is Scalar field Dark Matter (SFDM). Its properties allow it to produce similar results at large scales and solve the problems encountered at galactic scales. Nevertheless, the difficulty to obtain direct observations of Dark Matter makes it difficult to give a definitive comparison between the models. Therefore, it is important to study dark matter through different methods of analysis that would allow to increase the validity of its scope, and these methods are constantly being researched. In this work, a particular density profile known as Wave Dark Matter is implemented as a gravitational lens to study its behaviour in the cases where it produces strong lensing of light and of gravitational waves. Analytical functions for the description of a soliton core and a soliton core + NFW tail are applied to a sub-sample of 6 galaxies from The Sloan Lens ACS Survey to constrain the lensing parameters and their relation with the profile. Furthermore, by considering the soliton core to be the main contributor to the mass profile, this is implemented as a lens for the case of the wave approximation and further to describe the major effects of the lens on gravitational waves. It was found that the soliton core is too compact and dense in order to reproduce the observed values of the data for the lensed galaxies. However, adding a NFW tail alleviates the problem and reaches radii and masses within the range reported in the literature, although the size of the NFW tail cannot be properly constrained. Meanwhile for gravitational waves, it was found that the lensing parameters of the soliton core, if they are expected to describe a galaxy, will be such that they are more likely to be observed spaceborne gravitational wave detectors. In summary, therefore, a wave dark matter soliton in combination with a NFW tail is able to represent a galaxy, and the combination of ligh and gravitational waves should give new insight on the validity of the profile as a description of Dark Matter galactic haloes.
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Talukder, Dipongkar. "Multi-baseline gravitational wave radiometry." Pullman, Wash. : Washington State University, 2008. http://www.dissertations.wsu.edu/Thesis/Fall2008/d_talukder_112408.pdf.

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Thesis (M.S. in physics)--Washington State University, December 2008.
Title from PDF title page (viewed on June 19, 2009). "Department of Physics and Astronomy." Includes bibliographical references (p. 44-46).
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O'Shaughnessy, Richard William Thorne Kip S. "Topics in gravitational wave astronomy /." Diss., Pasadena, Calif. : California Institute of Technology, 2004. http://resolver.caltech.edu/CaltechETD:etd-08052003-161044.

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Lovelace, Geoffrey Mark Thorne Kip S. Thorne Kip S. "Topics in gravitational-wave physics /." Diss., Pasadena, Calif. : California Institute of Technology, 2007. http://resolver.caltech.edu/CaltechETD:etd-05232007-115433.

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Shaddock, Daniel Anthony, and Daniel Shaddock@jpl nasa gov. "Advanced Interferometry for Gravitational Wave Detection." The Australian National University. Faculty of Science, 2001. http://thesis.anu.edu.au./public/adt-ANU20020227.171850.

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In this thesis we investigate advanced techniques for the readout and control of various interferometers. In particular, we present experimental investigations of interferometer configurations and control techniques to be used in second generation interferometric gravitational wave detectors. We also present a new technique, tilt locking, for the readout and control of optical interferometers. ¶ We report the first experimental demonstration of a Sagnac interferometer with resonant sideband extraction (RSE). We measure the frequency response to modulation of the length of the arms and demonstrate an increase in signal bandwidth of by a factor of 6.5 compared to the Sagnac with arm cavities only. We compare Sagnac interferometers based on optical cavities with cavity-based Michelson interferometers and find that the Sagnac configuration has little overall advantage in a cavity-based system. ¶ A system for the control and signal extraction of a power recycled Michelson interferometer with RSE is presented. This control system employs a frontal modulation scheme requiring a phase modulated carrier field and a phase modulated subcarrier field. The system is capable of locking all 5 length degrees of freedom and allows the signal cavity to be detuned over the entire range of possibilities, in principle, whilst maintaining lock. We analytically investigate the modulation/demodulation techniques used to obtain these error signals, presenting an introductory explanation of single sideband modulation/demodulation and double demodulation. ¶ This control system is implemented on a benchtop prototype interferometer. We discuss technical problems associated with production of the input beam modulation components and present several solutions. Operation of the interferometer is demonstrated for a wide range of detunings. The frequency response of the interferometer is measured for various detuned points and we observe good agreement with theoretical predictions. The ability of the control system to maintain lock as the interferometer is detuned is experimentally demonstrated. ¶ Tilt locking, a new technique to obtain an error signal to lock a laser to an optical cavity, is presented. This technique produces an error signal by efficient measurement of the interference between the TEM00 and TEM10 modes. We perform experimental and theoretical comparisons with the widely used Pound-Drever-Hall (PDH) technique. We derive the quantum noise limit to the sensitivity of a measurement of the beam position, and using this result calculate the shot noise limited sensitivity of tilt locking. We show that tilt locking has a quantum efficiency of 80%, compared to 82% for the PDH technique. We present experimental demonstrations of tilt locking in several applications including frequency stabilisation, continuous-wave second harmonic generation, and injection locking of a Nd:YAG slab laser. In each of these cases, we demonstrate that the performance of tilt locking is not the limiting factor of the lock stability, and show that it achieves similar performance to the PDH based system. ¶ Finally, we discuss how tilt locking can be effectively applied to two beam interferometers. We show experimentally how a two beam interferometer typically gives excellent isolation against errors arising from changes in the photodetector position, and experimentally demonstrate the use of tilt locking as a signal readout system for a Sagnac interferometer.
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Dickson, Christopher. "Coincidence analysis of gravitational wave data." Thesis, Cardiff University, 1993. http://orca.cf.ac.uk/6809/.

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Tinto, M. "Theoretical aspects of gravitational wave detection." Thesis, Bucks New University, 1987. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.380273.

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Rubbo, Louis Joseph. "Gravitational wave astronomy using spaceborne detectors." Diss., Montana State University, 2004. http://etd.lib.montana.edu/etd/2004/rubbo/RubboL0805.pdf.

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Fredriksson, Felicia. "Investigating residuals from gravitational wave events GW151012 and GW151226." Thesis, Uppsala universitet, Teoretisk fysik, 2019. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-389464.

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Books on the topic "Gravitational wave"

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NATO Advanced Research Workshop on Gravitational Wave Data Analysis (1987 Cardiff, Wales). Gravitational wave data analysis. Dordrecht [Holland]: Kluwer Academic Publishers, 1989.

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Sopuerta, Carlos F., ed. Gravitational Wave Astrophysics. Cham: Springer International Publishing, 2015. http://dx.doi.org/10.1007/978-3-319-10488-1.

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Schutz, B. F., ed. Gravitational Wave Data Analysis. Dordrecht: Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-1185-7.

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Blair, D. G., L. Ju, C. Zhao, and E. J. Howell, eds. Advanced Gravitational Wave Detectors. Cambridge: Cambridge University Press, 2009. http://dx.doi.org/10.1017/cbo9781139046916.

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Schutz, B. F. Gravitational Wave Data Analysis. Dordrecht: Springer Netherlands, 1989.

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Bambi, Cosimo, Stavros Katsanevas, and Konstantinos D. Kokkotas, eds. Handbook of Gravitational Wave Astronomy. Singapore: Springer Singapore, 2020. http://dx.doi.org/10.1007/978-981-15-4702-7.

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Creighton, Jolien D. E., and Warren G. Anderson. Gravitational-Wave Physics and Astronomy. Weinheim, Germany: Wiley-VCH Verlag GmbH & Co. KGaA, 2011. http://dx.doi.org/10.1002/9783527636037.

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Jaranowski, Piotr. Analysis of gravitational-wave data. Cambridge: Cambridge University Press, 2009.

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Andrzej, Królak, ed. Analysis of gravitational-wave data. Cambridge: Cambridge University Press, 2009.

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Jaranowski, Piotr. Analysis of gravitational-wave data. Cambridge: Cambridge University Press, 2009.

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Book chapters on the topic "Gravitational wave"

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Cripe, Jonathan. "Gravitational Waves and Gravitational Wave Detectors." In Springer Theses, 1–26. Cham: Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-45031-1_1.

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Kembhavi, Ajit, and Pushpa Khare. "Gravitational Wave Detectors." In Gravitational Waves, 93–112. Singapore: Springer Singapore, 2020. http://dx.doi.org/10.1007/978-981-15-5709-5_7.

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Kembhavi, Ajit, and Pushpa Khare. "Gravitational Wave Detections." In Gravitational Waves, 113–32. Singapore: Springer Singapore, 2020. http://dx.doi.org/10.1007/978-981-15-5709-5_8.

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Kembhavi, Ajit, and Pushpa Khare. "Future Gravitational Wave Detectors." In Gravitational Waves, 133–48. Singapore: Springer Singapore, 2020. http://dx.doi.org/10.1007/978-981-15-5709-5_9.

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Buonanno, Alessandra. "Gravitational Wave Astronomy." In Astronomy at the Frontiers of Science, 87–106. Dordrecht: Springer Netherlands, 2011. http://dx.doi.org/10.1007/978-94-007-1658-2_5.

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Weber, J. "Gravitational Wave Experiments." In High-Energy Physics, 199–209. Boston, MA: Springer US, 1985. http://dx.doi.org/10.1007/978-1-4684-8848-7_15.

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Poggiani, Rosa. "Gravitational Wave Astronomy." In UNITEXT for Physics, 123–39. Cham: Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-44729-2_15.

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Kokkotas, Konstantinos D. "Gravitational Wave Astronomy." In Reviews in Modern Astronomy, 140–66. Weinheim, Germany: Wiley-VCH Verlag GmbH & Co. KGaA, 2008. http://dx.doi.org/10.1002/9783527622993.ch7.

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FERRARI, VALERIA. "GRAVITATIONAL WAVE SOURCES." In Frontiers of Fundamental Physics, 83–91. Dordrecht: Springer Netherlands, 2006. http://dx.doi.org/10.1007/1-4020-4339-2_13.

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Ferrari, Valeria, Leonardo Gualtieri, and Paolo Pani. "Gravitational wave sources." In General Relativity and its Applications, 267–98. Boca Raton: CRC Press, 2020.: CRC Press, 2020. http://dx.doi.org/10.1201/9780429491405-14.

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Conference papers on the topic "Gravitational wave"

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Tsupko, Oleg. "Gravitational lensing by gravitational wave pulse." In The Manchester Microlensing Conference: The 12th International Conference and ANGLES Microlensing Workshop. Trieste, Italy: Sissa Medialab, 2008. http://dx.doi.org/10.22323/1.054.0063.

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Fritschel, Peter. "Gravitational Wave Interferometry." In Frontiers in Optics. Washington, D.C.: OSA, 2009. http://dx.doi.org/10.1364/fio.2009.jmb1.

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Fontana, Giorgio. "Gravitational Wave Propulsion." In SPACE TECHNOLOGY AND APPLICATIONS INT.FORUM-STAIF 2005: Conf.Thermophys in Micrograv;Conf Comm/Civil Next Gen.Space Transp; 22nd Symp Space Nucl.Powr Propuls.;Conf.Human/Robotic Techn.Nat'l Vision Space Expl.; 3rd Symp Space Colon.; 2nd Symp.New Frontiers. AIP, 2005. http://dx.doi.org/10.1063/1.1867262.

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Bassi, Angelo. "Gravitational decoherence and gravitational-wave function collapse." In Optical, Opto-Atomic, and Entanglement-Enhanced Precision Metrology, edited by Selim M. Shahriar and Jacob Scheuer. SPIE, 2019. http://dx.doi.org/10.1117/12.2515594.

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Weldon, Thomas P., and Kathryn L. Smith. "Gravitationally-Small Gravitational Antennas, the Chu Limit, and Exploration of Veselago-Inspired Notions of Gravitational Metamaterials." In 2019 Thirteenth International Congress on Artificial Materials for Novel Wave Phenomena (Metamaterials). IEEE, 2019. http://dx.doi.org/10.1109/metamaterials.2019.8900861.

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Hogan, Craig J. "Cosmological gravitational wave backgrounds." In The second international laser interferometer space antenna symposium (LISA) on the detection and observation of gravitational waves in space. AIP, 1998. http://dx.doi.org/10.1063/1.57425.

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MAHARAJ, MANOJ S. "B4: GRAVITATIONAL WAVE SOURCES." In Proceedings of the 16th International Conference. WORLD SCIENTIFIC, 2002. http://dx.doi.org/10.1142/9789812776556_0027.

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MANDIC, V. "STOCHASTIC GRAVITATIONAL-WAVE BACKGROUND." In Proceedings of the MG13 Meeting on General Relativity. WORLD SCIENTIFIC, 2015. http://dx.doi.org/10.1142/9789814623995_0336.

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Finn, L. S. "Toward gravitational wave detection." In Third edoardo amaldi conference on gravitational waves. AIP, 2000. http://dx.doi.org/10.1063/1.1291910.

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Jones, D. I. "Gravitational wave observations of pulsars." In THE ASTROPHYSICS OF GRAVITATIONAL WAVE SOURCES. AIP, 2003. http://dx.doi.org/10.1063/1.1629447.

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Reports on the topic "Gravitational wave"

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Dimopoulos, Savas, Peter W. Graham, Jason M. Hogan, Mark A. Kasevich, and Surjeet Rajendran. Gravitational Wave Detection with Atom Interferometry. Office of Scientific and Technical Information (OSTI), January 2008. http://dx.doi.org/10.2172/922600.

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Dimopoulos, Savas, Peter W. Graham, Jason M. Hogan, Mark A. Kasevich, and Surjeet Rajendran. An Atomic Gravitational Wave Interferometric Sensor (AGIS). Office of Scientific and Technical Information (OSTI), August 2008. http://dx.doi.org/10.2172/935683.

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Meadors, Grant. Gravitational-Wave Astronomy's Future Among the Stars. Office of Scientific and Technical Information (OSTI), February 2022. http://dx.doi.org/10.2172/1846119.

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Barker, Drew R. Sensitivity Analysis of a Space-borne Gravitational Wave Detector. Fort Belvoir, VA: Defense Technical Information Center, May 2004. http://dx.doi.org/10.21236/ada425794.

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Miller, Jonah Maxwell. Gravitational Waves. Office of Scientific and Technical Information (OSTI), October 2017. http://dx.doi.org/10.2172/1402567.

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Vilasi, Gaetano. • On the Polarization of Gravitational Waves. GIQ, 2012. http://dx.doi.org/10.7546/giq-9-2008-320-333.

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Alexander, S. Leptogenesis from Gravitational Waves and CP Violation. Office of Scientific and Technical Information (OSTI), March 2004. http://dx.doi.org/10.2172/826770.

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Senatore, Leonardo. New Sources of Gravitational Waves During Inflation. Office of Scientific and Technical Information (OSTI), February 2012. http://dx.doi.org/10.2172/1035109.

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Meadors, Grant, Shira Goldhaber-Gordon, and Lexington Smith. Deep learning to help find continuous gravitational waves. Office of Scientific and Technical Information (OSTI), November 2021. http://dx.doi.org/10.2172/1830555.

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Alexander, S. Birefringent Gravitational Waves and the Consistency Check of Inflation. Office of Scientific and Technical Information (OSTI), November 2004. http://dx.doi.org/10.2172/839588.

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