Relevant bibliographies by topics / Gravitational waves

Academic literature on the topic 'Gravitational waves'

Author: Grafiati
Published: 4 June 2021
Last updated: 29 July 2024

Create a spot-on reference in APA, MLA, Chicago, Harvard, and other styles

Select a source type:

Contents

Consult the lists of relevant articles, books, theses, conference reports, and other scholarly sources on the topic 'Gravitational waves.'

Next to every source in the list of references, there is an 'Add to bibliography' button. Press on it, and we will generate automatically the bibliographic reference to the chosen work in the citation style you need: APA, MLA, Harvard, Chicago, Vancouver, etc.

You can also download the full text of the academic publication as pdf and read online its abstract whenever available in the metadata.

Journal articles on the topic "Gravitational waves"

1

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.

Full text
Abstract:
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.
APA, Harvard, Vancouver, ISO, and other styles
2

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.

Full text
Abstract:
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.
APA, Harvard, Vancouver, ISO, and other styles
3

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.

Full text
Abstract:
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?
APA, Harvard, Vancouver, ISO, and other styles
4

Trautman, Andrzej. "Gravitational waves." Journal of Physics: Conference Series 873 (July 2017): 012012. http://dx.doi.org/10.1088/1742-6596/873/1/012012.

Full text
APA, Harvard, Vancouver, ISO, and other styles
5

Robertson, Norna A. "Gravitational Waves." Classical and Quantum Gravity 18, no. 15 (July 18, 2001): 3081. http://dx.doi.org/10.1088/0264-9381/18/15/701.

Full text
APA, Harvard, Vancouver, ISO, and other styles
6

Ferreira, Pedro. "Gravitational waves." New Scientist 207, no. 2767 (July 2010): vi. http://dx.doi.org/10.1016/s0262-4079(10)61579-5.

Full text
APA, Harvard, Vancouver, ISO, and other styles
7

Davier, Michel. "Gravitational waves." Nuclear Physics B - Proceedings Supplements 87, no. 1-3 (June 2000): 453–63. http://dx.doi.org/10.1016/s0920-5632(00)00720-9.

Full text
APA, Harvard, Vancouver, ISO, and other styles
8

Blair, David. "Gravitational waves." Endeavour 16, no. 1 (January 1992): 37–42. http://dx.doi.org/10.1016/0160-9327(92)90115-6.

Full text
APA, Harvard, Vancouver, ISO, and other styles
9

LEE, Hyung Mok. "Gravitational Waves." Physics and High Technology 20, no. 3 (March 31, 2011): 35. http://dx.doi.org/10.3938/phit.20.012.

Full text
APA, Harvard, Vancouver, ISO, and other styles
10

Sathyaprakash, B. S., and Waiter Winkler. "Gravitational waves." Europhysics News 32, no. 6 (November 2001): 240–41. http://dx.doi.org/10.1051/epn:2001614.

Full text
APA, Harvard, Vancouver, ISO, and other styles
More sources

Dissertations / Theses on the topic "Gravitational waves"

1

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.

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

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/.

Full text
Abstract:
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.
APA, Harvard, Vancouver, ISO, and other styles
3

Onuk, Ahmet Emre. "Collision Of Gravitational Waves: Axisymmetric Pp Waves." Master's thesis, METU, 2007. http://etd.lib.metu.edu.tr/upload/12608696/index.pdf.

Full text
Abstract:
The collision of impulsive gravitational waves, electromagnetic plane waves with collinear polarization and, especially, plane fronted parallel waves (pp waves) are considered. The solution of axisymmetric pp waves is reviewed and the structures of the resulting space-times are investigated with the help of curvature invariants.
APA, Harvard, Vancouver, ISO, and other styles
4

Moore, Christopher James. "Gravitational waves : understanding black holes." Thesis, University of Cambridge, 2016. https://www.repository.cam.ac.uk/handle/1810/257043.

Full text
Abstract:
This thesis concerns the use of observations of gravitational waves as tools for astronomy and fundamental physics. Gravitational waves are small ripples in spacetime produced by rapidly accelerating masses; their existence has been predicted for almost 100 years, but the first direct evidence of their existence came only very recently with the announcement in February 2016 of the detection by the LIGO and VIRGO collaborations. Part I of this thesis presents an introduction to gravitational wave astronomy, including a detailed discussion of a wide range of gravitational wave sources, their signal morphologies, and the experimental detectors used to observe them. Part II of this thesis concerns a particular data analysis problem which often arises when trying to infer the source properties from a gravitational wave observation. The use of an inaccurate signal model can cause significant systematic errors in the inferred source parameters. The work in this section concerns a proposed technique, called the Gaussian process marginalised likelihood, for overcoming this problem. Part III of this thesis concerns the possibility of testing if the gravitational field around an astrophysical black hole conforms to the predictions of general relativity and the cosmic censorship hypothesis. It is expected that the gravitational field should be well described by the famous Kerr solution. Two approaches for testing this hypothesis are considered; one using X-ray observations and one using gravitational waves. The results from these two approaches are compared and contrasted. Finally, the conclusions and a discussion of future prospects are presented in part IV of this thesis.
APA, Harvard, Vancouver, ISO, and other styles
5

Siemens, Xavier. "Gravitational waves and cosmic strings /." Thesis, Connect to Dissertations & Theses @ Tufts University, 2002.

Find full text
Abstract:
Thesis (Ph.D.)--Tufts University, 2002.
Adviser: Alexander Vilenkin. Submitted to the Dept. of Physics. Includes bibliographical references (leaves 95-98). Access restricted to members of the Tufts University community. Also available via the World Wide Web;
APA, Harvard, Vancouver, ISO, and other styles
6

Bello, Arufe Aaron. "Gravitational Waves in General Relativity." Thesis, Umeå universitet, Institutionen för fysik, 2017. http://urn.kb.se/resolve?urn=urn:nbn:se:umu:diva-136721.

Full text
Abstract:
In this paper, we write a summary about general relativity and, in particular,gravitational waves. We start by discussing the mathematics that generalrelativity uses, as well as the geometry in general relativity's spacetime. Afterwards,we explain linearized general relativity and derive the linearizedversions of Einstein's equations. From here, we construct wave solutionsand explain the polarization of gravitational waves. The quadrupole formulais derived, and generation and detection of gravitational waves is brie ydiscussed. Finally, LIGO and its latest discovery of gravitational waves isreviewed.
APA, Harvard, Vancouver, ISO, and other styles
7

Lagger, Cyril Oscar. "Gravitational Waves and Fundamental Physics." Thesis, The University of Sydney, 2019. http://hdl.handle.net/2123/20810.

Full text
Abstract:
This thesis investigates the implications of gravitational waves (GWs) for particle physics and cosmology. We first give an overview of the current state of general relativity and quantum field theory. We also emphasize where GWs may come into play to shed new light on unsolved problems in physics. First, we make use of GWs to constrain the scale of non-commutative space-time. Assuming such quantum fuzziness, we compute the equations of motion of a binary black hole and the associated generation of GWs. Compared to general relativity, leading non-commutative effects produce a post-Newtonian correction of order (v/c)^4. Using the recent GW150914 signal, we find that the scale of non-commutativity is bounded to be below or at the order of the Planck scale. This represents an improvement of ~15 orders of magnitude compared to previous constraints. Second, we study the production of GWs from cosmological phase transitions. We consider two unrelated extensions of the standard model: a non-linear realization of the electroweak gauge group and a model with hidden scale invariance. In the first case, the Higgs vacuum configuration is altered by a cubic coupling giving the possibility to have a strong and prolonged electroweak first-order transition. In our second model, the electroweak transition cannot proceed until it is triggered by a first-order QCD chiral symmetry breaking around 130 MeV. We compute that the stochastic GW background produced during these two phase transitions is expected to be in the detection range of pulsar timing arrays. Finally, we investigate the backreaction of particle production on false vacuum decay. We present a formalism which makes use of the reduced density matrix of the system to quantify the impact of these particles on the decay rate of a scalar field in flat space-time. We then apply this method to a toy model potential and we exhibit different scenarios with either significant or negligible backreaction.
APA, Harvard, Vancouver, ISO, and other styles
8

Corbin, Vincent Dominique Andre. "Studying cosmological sources of gravitational waves." Diss., Montana State University, 2010. http://etd.lib.montana.edu/etd/2010/corbin/CorbinV1210.pdf.

Full text
Abstract:
This dissertation presents two aspects of the study of cosmology through gravitational waves. The first aspect involves direct observation of past eras of the Universe's formation. The detection of the Cosmic Microwave Background Radiation was one of the most important cosmological discoveries of the last century. With the development of interferometric gravitational wave detectors, we may be in a position to detect its gravitational equivalent in this century. The Cosmic Gravitational Background is likely to be isotropic and stochastic, making it difficult to distinguish from instrument noise. The contribution from the gravitational background can be isolated by cross-correlating the signals from two or more independent detectors. Here we extend previous studies that considered the cross-correlation of two Michelson channels by calculating the optimal signal to noise ratio that can be achieved by combining the full set of interferometry variables that are available with a six link triangular interferometer. We apply our results to the detector design described in the Big Bang Observer mission concept study and find that it could detect a background with Omega gw > 2.2 x 10 ̄¹⁷. The second aspect consists in studying astrophysical sources that detain crucial information on the Universe's evolution. We focus our attention on black holes binary sytems. These systems contain information on the rate of merger between galaxies, which in turn is key to unlock the mystery of inflation. Pulsar timing is a promising technique for detecting low frequency sources of gravitational waves, such as massive and supermassive black hole binaries. Here we show that the timing data from an array of pulsars can be used to recover the physical parameters describing an individual black hole binary to good accuracy, even for moderately strong signals. A novel aspect of our analysis is that we include the distance to each pulsar as a search parameter, which allows us to utilize the full gravitational wave signal. This doubles the signal power, improves the sky location determination by an order of magnitude, and allows us to extract the mass and the distance to the black hole binary.
APA, Harvard, Vancouver, ISO, and other styles
9

Gholami, Ghadikolaei Iraj. "Data analysis of continuous gravitational waves." Phd thesis, Universität Potsdam, 2007. http://opus.kobv.de/ubp/volltexte/2008/1880/.

Full text
Abstract:
This thesis describes two main projects; the first one is the optimization of a hierarchical search strategy to search for unknown pulsars. This project is divided into two parts; the first part (and the main part) is the semi-coherent hierarchical optimization strategy. The second part is a coherent hierarchical optimization strategy which can be used in a project like Einstein@Home. In both strategies we have found that the 3-stages search is the optimum strategy to search for unknown pulsars. For the second project we have developed a computer software for a coherent Multi-IFO (Interferometer Observatory) search. To validate our software, we have worked on simulated data as well as hardware injected signals of pulsars in the fourth LIGO science run (S4). While with the current sensitivity of our detectors we do not expect to detect any true Gravitational Wave signals in our data, we can still set upper limits on the strength of the gravitational waves signals. These upper limits, in fact, tell us how weak a signal strength we would detect. We have also used our software to set upper limits on the signal strength of known isolated pulsars using LIGO fifth science run (S5) data.
Diese Dissertation besteht aus zwei Projekten: Im ersten Projekt wird die Optimierung einer hierarchischen Strategie zum Auffinden von 'unbekannten' Pulsaren beschrieben. Der erste Teil besteht dabei aus einer semi-kohärenten und der zweite Teil aus einer kohärenten Optimierungsstrategie, wie sie in Projekten wie Einstein@Home verwendet werden kann. In beiden Ansätzen erwies sich eine 3-Stufensuche als optimale Suchstrategie für 'unbekannte' Pulsare. Für das zweite Projekt entwickelten wir eine Software für eine kohärente Multi-IFO (Interferometer Observatory) Suche. Zum Validieren der Software verwendeten wir sowohl simulierte Daten als auch Hardware induzierte Signale von Pulsaren aus dem vierten 'LIGO Science run' (S4). Wir erwarten nicht, mit der aktuellen Empfindlichkeit unserer Detektoren echte GW- Signale aufzunehmen, können jedoch obere Grenzen für die Stärke der Gravitationswellen-Signale bestimmen. Diese oberen Grenzen geben uns an, wie schwach ein gerade noch detektierbares Signal werden kann. Ferner benutzten wir die Software um eine obere Grenze für bekannte, isolierte Pulsare zu bestimmen, wobei wir Daten aus dem fünften 'LIGO Science run (S5) verwendeten.
APA, Harvard, Vancouver, ISO, and other styles
10

Williamson, Andrew Robert. "Gravitational waves with gamma-ray bursts." Thesis, Cardiff University, 2016. http://orca.cf.ac.uk/96479/.

Full text
Abstract:
Gravitational waves have now twice been detected emanating from the merging of binary black hole systems. In this thesis we detail the methods used to search for binary merger gravitational wave signals associated with short gamma-ray bursts, focusing on systems that include at least one neutron star. We first cover the background theory behind gravitational wave emission, the means of detection via interferometry, and the types of astrophysical sources that could be detected now or in the near future. We follow this with a review of gamma-ray burst theory and observations, focusing in particular those bursts with short durations. These are likely to be caused by the mergers of binaries that include a neutron star and a black hole, or two neutron stars - events of great interest to gravitational wave astronomy. We then discuss the methods used to search gravitational wave data in a targeted way, using the prior observation of a short gamma-ray bursts to focus the analysis and improve the chances of making a detection. We also summarise early searches of this kind and present the results of a search carried out on LIGO and Virgo data spanning 2005-2010, targeting short gamma-ray bursts detected by the InterPlanetary Network. We then turn our attention to the current, second generation of gravitational wave detectors. We present a detailed calculation of the prospects of success for the targeted short gamma-ray burst search technique, and find that we might reasonably expect to make up to a few detections per year around the turn of the decade. We then outline a new search structure for use during the second generation of detectors, and an astrophysical event alert system for the control rooms of gravitational wave observatories. We end with a presentation of the results of the new and improved search carried out during the first observing run of Advanced LIGO.
APA, Harvard, Vancouver, ISO, and other styles
More sources

Books on the topic "Gravitational waves"

1

Kembhavi, Ajit, and Pushpa Khare. Gravitational Waves. Singapore: Springer Singapore, 2020. http://dx.doi.org/10.1007/978-981-15-5709-5.

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

Maggiore, Michele. Gravitational waves. Oxford: Oxford University Press, 2008.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
3

Kitchin, C. R. Understanding Gravitational Waves. Cham: Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-74207-2.

Full text
APA, Harvard, Vancouver, ISO, and other styles
4

Tikhookeanskiĭ okeanologicheskiĭ institut (Rossiĭskai͡a︡ akademii͡a︡ nauk), ed. Vzaimodeĭstvie gravitonov vysokikh ėnergiĭ s fermionami. Vladivostok: [s.n.], 1993.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
5

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

Find full text
APA, Harvard, Vancouver, ISO, and other styles
6

Feldbaum, David M. Gravitational Waves: An Overview. Cham: Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-031-02613-3.

Full text
APA, Harvard, Vancouver, ISO, and other styles
7

Kenath, Arun, and Chandra Sivaram. Physics of Gravitational Waves. Cham: Springer International Publishing, 2023. http://dx.doi.org/10.1007/978-3-031-30463-7.

Full text
APA, Harvard, Vancouver, ISO, and other styles
8

Seminar "Gravitat͡sionnai͡a ėnergii͡a i gravitat͡sionnye volny" (6th 1993 Dubna, Chekhovskiĭ raĭon, Russia). Trudy VI seminara "Gravitat͡sionnai͡a ėnergii͡a i gravitat͡sionnye volny", Dubna, 26-30 okti͡abri͡a 1993 goda. Dubna: OII͡AI, 1994.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
9

Dhurandhar, Sanjeev, and Sanjit Mitra. General Relativity and Gravitational Waves. Cham: Springer International Publishing, 2022. http://dx.doi.org/10.1007/978-3-030-92335-8.

Full text
APA, Harvard, Vancouver, ISO, and other styles
10

Babak, Stanislav. Gravitational Waves from Coalescing Binaries. Cham: Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-031-02612-6.

Full text
APA, Harvard, Vancouver, ISO, and other styles
More sources

Book chapters on the topic "Gravitational waves"

1

Kembhavi, Ajit, and Pushpa Khare. "Introduction." In Gravitational Waves, 1–4. Singapore: Springer Singapore, 2020. http://dx.doi.org/10.1007/978-981-15-5709-5_1.

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

Kembhavi, Ajit, and Pushpa Khare. "Electromagnetic Radiation: The Key to Understanding the Universe." In Gravitational Waves, 5–32. Singapore: Springer Singapore, 2020. http://dx.doi.org/10.1007/978-981-15-5709-5_2.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

Kembhavi, Ajit, and Pushpa Khare. "Gravity: The Force that Governs the Universe." In Gravitational Waves, 33–54. Singapore: Springer Singapore, 2020. http://dx.doi.org/10.1007/978-981-15-5709-5_3.

Full text
APA, Harvard, Vancouver, ISO, and other styles
4

Kembhavi, Ajit, and Pushpa Khare. "Gravitational Waves: The New Window to the Universe." In Gravitational Waves, 55–60. Singapore: Springer Singapore, 2020. http://dx.doi.org/10.1007/978-981-15-5709-5_4.

Full text
APA, Harvard, Vancouver, ISO, and other styles
5

Kembhavi, Ajit, and Pushpa Khare. "Compact Sources of Gravitational Waves." In Gravitational Waves, 61–81. Singapore: Springer Singapore, 2020. http://dx.doi.org/10.1007/978-981-15-5709-5_5.

Full text
APA, Harvard, Vancouver, ISO, and other styles
6

Kembhavi, Ajit, and Pushpa Khare. "Evidence for the Existence of Gravitational Waves: The Binary Pulsar." In Gravitational Waves, 83–91. Singapore: Springer Singapore, 2020. http://dx.doi.org/10.1007/978-981-15-5709-5_6.

Full text
APA, Harvard, Vancouver, ISO, and other styles
7

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.

Full text
APA, Harvard, Vancouver, ISO, and other styles
8

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.

Full text
APA, Harvard, Vancouver, ISO, and other styles
9

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.

Full text
APA, Harvard, Vancouver, ISO, and other styles
10

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.

Full text
APA, Harvard, Vancouver, ISO, and other styles

Conference papers on the topic "Gravitational waves"

1

Danzmann, Karsten. "Gravitational waves." In European Physical Society Europhysics Conference on High Energy Physics. Trieste, Italy: Sissa Medialab, 2010. http://dx.doi.org/10.22323/1.084.0015.

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

SIGG, DANIEL. "GRAVITATIONAL WAVES." In (TASI 98). WORLD SCIENTIFIC, 2000. http://dx.doi.org/10.1142/9789812813497_0012.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

Lueck, Harald. "Detecting gravitational waves." In SPIE Astronomical Telescopes + Instrumentation, edited by James Hough and Gary H. Sanders. SPIE, 2004. http://dx.doi.org/10.1117/12.553785.

Full text
APA, Harvard, Vancouver, ISO, and other styles
4

Wickramasinghe, T. "Detection of gravitational waves from gravitationally lensed systems." In RELATIVISTIC ASTROPHYSICS: 20th Texas Symposium. AIP, 2001. http://dx.doi.org/10.1063/1.1419664.

Full text
APA, Harvard, Vancouver, ISO, and other styles
5

PIZZELLA, G. "SEARCH FOR GRAVITATIONAL WAVES." In Proceedings of the Sixth School. WORLD SCIENTIFIC, 2002. http://dx.doi.org/10.1142/9789812777492_0015.

Full text
APA, Harvard, Vancouver, ISO, and other styles
6

LEE, K. J., R. X. XU, and G. J. QIAO. "PULSARS AND GRAVITATIONAL WAVES." In Proceedings of the Ninth Asia-Pacific International Conference. WORLD SCIENTIFIC, 2010. http://dx.doi.org/10.1142/9789814307673_0016.

Full text
APA, Harvard, Vancouver, ISO, and other styles
7

Ferrari, Valeria. "Sources of gravitational waves." In Cosmology and particle physics. AIP, 2001. http://dx.doi.org/10.1063/1.1363524.

Full text
APA, Harvard, Vancouver, ISO, and other styles
8

MILLER, J. C. "THEORY OF GRAVITATIONAL WAVES." In Proceedings of the 7th School. WORLD SCIENTIFIC, 2005. http://dx.doi.org/10.1142/9789812701893_0014.

Full text
APA, Harvard, Vancouver, ISO, and other styles
9

Yang, Sheng. "Searching electromagnetic counterpart of gravitational waves." In Gravitational-waves Science&Technology Symposium. Trieste, Italy: Sissa Medialab, 2018. http://dx.doi.org/10.22323/1.325.0037.

Full text
APA, Harvard, Vancouver, ISO, and other styles
10

Cesarini, Elisabetta, M. Lorenzini, A. Amato, G. Cagnoli, Q. Cassar, J. Dickmann, M. Granata, et al. "The Virgo Coating Collaboration: a detailed study on thermoelasticity in crystalline materials and other research lines." In Gravitational-waves Science&Technology Symposium. Trieste, Italy: Sissa Medialab, 2018. http://dx.doi.org/10.22323/1.325.0006.

Full text
APA, Harvard, Vancouver, ISO, and other styles

Reports on the topic "Gravitational waves"

1

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

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

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

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

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.

Full text
APA, Harvard, Vancouver, ISO, and other styles
4

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.

Full text
APA, Harvard, Vancouver, ISO, and other styles
5

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.

Full text
APA, Harvard, Vancouver, ISO, and other styles
6

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.

Full text
APA, Harvard, Vancouver, ISO, and other styles
7

Meadors, Grant David. Discovering hidden signals from gravitational waves and our universe. Office of Scientific and Technical Information (OSTI), October 2019. http://dx.doi.org/10.2172/1571577.

Full text
APA, Harvard, Vancouver, ISO, and other styles
8

Lanza, Robert Jr. Experimental Limits on Gravitational Waves in the MHz frequency Range. Office of Scientific and Technical Information (OSTI), March 2015. http://dx.doi.org/10.2172/1329051.

Full text
APA, Harvard, Vancouver, ISO, and other styles
9

Lim, Hyun. What’s Up Gravitational Waves! More Messages from Ripples of Spacetime. Office of Scientific and Technical Information (OSTI), November 2020. http://dx.doi.org/10.2172/1716733.

Full text
APA, Harvard, Vancouver, ISO, and other styles
10

Palmese, Antonella. Unveiling the unseen with the Dark Energy Survey: gravitational waves and dark matter. Office of Scientific and Technical Information (OSTI), January 2018. http://dx.doi.org/10.2172/1497090.

Full text
APA, Harvard, Vancouver, ISO, and other styles
You might also be interested in the extended bibliographies on the topic 'Gravitational waves' for particular source types:
Journal articles Dissertations / Theses Books
We offer discounts on all premium plans for authors whose works are included in thematic literature selections. Contact us to get a unique promo code!

To the bibliography