Gotowe bibliografie tematyczne / Coalescence de binaire compacte

Spis treści

  1. Artykuły w czasopismach
  2. Rozprawy doktorskie
  3. Książki
  4. Części książek
  5. Streszczenia konferencji

Gotowa bibliografia na temat „Coalescence de binaire compacte”

Autor: Grafiati
Data publikacji: 23 listopada 2024
Data aktualizacji: 31 lipca 2025

Utwórz poprawne odniesienie w stylach APA, MLA, Chicago, Harvard i wielu innych

Wybierz rodzaj źródła:

Zobacz listy aktualnych artykułów, książek, rozpraw, streszczeń i innych źródeł naukowych na temat „Coalescence de binaire compacte”.

Przycisk „Dodaj do bibliografii” jest dostępny obok każdej pracy w bibliografii. Użyj go – a my automatycznie utworzymy odniesienie bibliograficzne do wybranej pracy w stylu cytowania, którego potrzebujesz: APA, MLA, Harvard, Chicago, Vancouver itp.

Możesz również pobrać pełny tekst publikacji naukowej w formacie „.pdf” i przeczytać adnotację do pracy online, jeśli odpowiednie parametry są dostępne w metadanych.

Artykuły w czasopismach na temat "Coalescence de binaire compacte"

1

Spera, Mario, Alessandro Alberto Trani, and Mattia Mencagli. "Compact Binary Coalescences: Astrophysical Processes and Lessons Learned." Galaxies 10, no. 4 (2022): 76. http://dx.doi.org/10.3390/galaxies10040076.

Pełny tekst źródła
Streszczenie:
On 11 February 2016, the LIGO and Virgo scientific collaborations announced the first direct detection of gravitational waves, a signal caught by the LIGO interferometers on 14 September 2015, and produced by the coalescence of two stellar-mass black holes. The discovery represented the beginning of an entirely new way to investigate the Universe. The latest gravitational-wave catalog by LIGO, Virgo and KAGRA brings the total number of gravitational-wave events to 90, and the count is expected to significantly increase in the next years, when additional ground-based and space-born interferomet
Style APA, Harvard, Vancouver, ISO itp.
2

Graziani, Luca. "Hunting for Dwarf Galaxies Hosting the Formation and Coalescence of Compact Binaries." Physics 1, no. 3 (2019): 412–29. http://dx.doi.org/10.3390/physics1030030.

Pełny tekst źródła
Streszczenie:
Here we introduce the latest version of the GAMESH model, capable to consistently account for the formation and evolution of compact binary systems along the cosmic assembly of a Milky Way (MW)-like galaxy, centered on a local group volume resolving a large population of dwarf satellites. After describing the galaxy assembly process and how the formation of binary systems is accounted for, we summarize some recent findings on the properties and evolution of low-metallicity dwarf galaxies hosting the birth/coalescence of stellar/compact binaries generating GW150914-like signals. Finally, we foc
Style APA, Harvard, Vancouver, ISO itp.
3

Kalogera, V. "Close Binaries with Two Compact Objects." International Astronomical Union Colloquium 177 (2000): 579–84. http://dx.doi.org/10.1017/s0252921100060668.

Pełny tekst źródła
Streszczenie:
AbstractThe coalescence of close binary systems with two compact objects (neutron stars and black holes) are considered to be promising sources of gravitational waves for the currently built laser interferometers. Here, I review the current Galactic coalescence estimates derived both theoretically and empirically. I discuss the uncertainties involved as well as ways of obtaining an upper limit to the coalescence rate of two neutron stars.
Style APA, Harvard, Vancouver, ISO itp.
4

Abac, A. G., R. Abbott, I. Abouelfettouh, et al. "Observation of Gravitational Waves from the Coalescence of a 2.5–4.5 M ⊙ Compact Object and a Neutron Star." Astrophysical Journal Letters 970, no. 2 (2024): L34. http://dx.doi.org/10.3847/2041-8213/ad5beb.

Pełny tekst źródła
Streszczenie:
Abstract We report the observation of a coalescing compact binary with component masses 2.5–4.5 M ⊙ and 1.2–2.0 M ⊙ (all measurements quoted at the 90% credible level). The gravitational-wave signal GW230529_181500 was observed during the fourth observing run of the LIGO–Virgo–KAGRA detector network on 2023 May 29 by the LIGO Livingston observatory. The primary component of the source has a mass less than 5 M ⊙ at 99% credibility. We cannot definitively determine from gravitational-wave data alone whether either component of the source is a neutron star or a black hole. However, given existing
Style APA, Harvard, Vancouver, ISO itp.
5

Rasio, Frederic A., and Stuart L. Shapiro. "Hydrodynamic Evolution of Coalescing Compact Binaries." Symposium - International Astronomical Union 165 (1996): 17–28. http://dx.doi.org/10.1017/s0074180900055522.

Pełny tekst źródła
Streszczenie:
In addition to their possible relevance to gamma-ray bursts, coalescing binary neutron stars have long been recognized as important sources of gravitational radiation that should become detectable with the new generation of laser interferometers such as LIGO. Hydrodynamics plays an essential role near the end of the coalescence when the two stars finally merge into a single object. The shape of the corresponding burst of gravitational waves provides a direct probe into the interior structure of a neutron star and the nuclear equation of state. The interpretation of the gravitational waveform d
Style APA, Harvard, Vancouver, ISO itp.
6

WEN, LINQING, and QI CHU. "EARLY DETECTION AND LOCALIZATION OF GRAVITATIONAL WAVES FROM COMPACT BINARY COALESCENCES." International Journal of Modern Physics D 22, no. 11 (2013): 1360011. http://dx.doi.org/10.1142/s0218271813600110.

Pełny tekst źródła
Streszczenie:
With the first detection of gravitational waves expected in the next decade, increasing efforts are made toward the electromagnetic follow-up observations of gravitational wave events. In this paper, I discuss the prospect of real-time detection and source localization for gravitational waves from neutron star–neutron star binary or neutron star–black hole binary coalescences before their merger. I show that several low-latency search pipelines are already under intensive development with the aim to provide real-time detections of these events. There will also be fast responding and/or wide-fi
Style APA, Harvard, Vancouver, ISO itp.
7

Shapiro, Stuart L. "Gravitomagnetic Induction during the Coalescence of Compact Binaries." Physical Review Letters 77, no. 22 (1996): 4487–90. http://dx.doi.org/10.1103/physrevlett.77.4487.

Pełny tekst źródła
Style APA, Harvard, Vancouver, ISO itp.
8

Chen, Bing-Guang, Tong Liu, Yan-Qing Qi, et al. "Effects of Vertical Advection on Multimessenger Signatures of Black Hole Neutrino-dominated Accretion Flows in Compact Binary Coalescences." Astrophysical Journal 941, no. 2 (2022): 156. http://dx.doi.org/10.3847/1538-4357/aca406.

Pełny tekst źródła
Streszczenie:
Abstract In the coalescence events of binary neutron star (NS) or a black hole (BH) and an NS, a BH hyperaccretion disk might be eventually formed. At very high mass accretion rates, MeV neutrinos will be emitted from this disk, which is called a neutrino-dominated accretion flow (NDAF). Neutrino annihilation in the space out of the disk is energetic enough to launch ultrarelativistic jets to power gamma-ray bursts. Moreover, vertical advection might exist in NDAFs, which can generate the magnetic buoyancy bubbles to release gamma-ray photons. In this paper, we visit the effects of the vertica
Style APA, Harvard, Vancouver, ISO itp.
9

Yu, Shenghua, Youjun Lu, and C. Simon Jeffery. "Orbital evolution of neutron-star–white-dwarf binaries by Roche lobe overflow and gravitational wave radiation." Monthly Notices of the Royal Astronomical Society 503, no. 2 (2021): 2776–90. http://dx.doi.org/10.1093/mnras/stab626.

Pełny tekst źródła
Streszczenie:
ABSTRACT We investigate the effects of mass transfer and gravitational wave (GW) radiation on the orbital evolution of contact neutron-star–white-dwarf (NS–WD) binaries, and the detectability of these binaries by space GW detectors (e.g. Laser Interferometer Space Antenna, LISA; Taiji; Tianqin). A NS–WD binary becomes contact when the WD component fills its Roche lobe, at which the GW frequency ranges from ∼0.0023 to 0.72 Hz for WD with masses ∼0.05–1.4 M⊙. We find that some high-mass NS–WD binaries may undergo direct coalescence after unstable mass transfer. However, the majority of NS–WD bin
Style APA, Harvard, Vancouver, ISO itp.
10

MacLeod, Morgan, Kishalay De, and Abraham Loeb. "Dusty, Self-obscured Transients from Stellar Coalescence." Astrophysical Journal 937, no. 2 (2022): 96. http://dx.doi.org/10.3847/1538-4357/ac8c31.

Pełny tekst źródła
Streszczenie:
Abstract We discuss the central role that dust condensation plays in shaping the observational appearance of outflows from coalescing binary systems. As binaries begin to coalesce, they shock-heat and expel material into their surroundings. Depending on the properties of the merging system, this material can expand to the point where molecules and dust form, dramatically increasing the gas opacity. We use the existing population of luminous red novae to constrain the thermodynamics of these ejecta, then apply our findings to the progressive obscuration of merging systems in the lead up to thei
Style APA, Harvard, Vancouver, ISO itp.
Więcej źródeł

Rozprawy doktorskie na temat "Coalescence de binaire compacte"

1

Andres, Nicolas. "Optimisation de la chaîne d'analyse MBTA et développement d'une méthode d'étalonnage de la réponse fréquentielle du détecteur d'onde gravitationnelle Virgo." Electronic Thesis or Diss., Chambéry, 2023. http://www.theses.fr/2023CHAMA029.

Pełny tekst źródła
Streszczenie:
La collaboration LIGO Virgo a marqué les débuts de l'astronomie gravitationnelle en apportant une preuve directe de leur existence en Septembre 2015. Ce domaine connaît depuis un bel essor dont chaque découverte permet une avancée dans les disciplines telles que l'astrophysique, la cosmologie et la physique fondamentale. À l'issue de chaque période d'observation, les détecteurs sont arrêtés et de nombreux aspects sont améliorés. Ce travail s'inscrit durant la phase de préparation entre la période O3 et O4 débutant en mai 2024 visant à configurer les interféromètres dans leurs états avancés en
Style APA, Harvard, Vancouver, ISO itp.
2

Kiendrébéogo, Ramodgwendé Weizmann. "Développements pour l'observation et la caractérisation des sources multi-messagers d'ondes gravitationnelles lors des campagnes d'observation LIGO-Virgo-KAGRA." Electronic Thesis or Diss., Université Côte d'Azur, 2024. http://www.theses.fr/2024COAZ5034.

Pełny tekst źródła
Streszczenie:
Les campagnes d'observation d'Advanced LIGO/Virgo ont révélé la physique complexe des fusions d'étoiles à neutrons binaires (BNS) et de trous noirs binaires. En 2017, la découverte simultanée des ondes gravitationnelles (OG) et des contreparties électromagnétiques (EM) d'une fusion de BNS a offert une vision détaillée de ce phénomène, avec de nombreux résultats en astrophysique, notamment sur la matière ultra-dense. Cependant, depuis lors, aucune nouvelle détection multi-messagers n'a été réalisée. Cela est dû aux défis des alertes rapides des OG, de la réactivité des télescopes et du traiteme
Style APA, Harvard, Vancouver, ISO itp.
3

MacLeod, Duncan. "Improving the sensitivity of searches for gravitational waves from compact binary coalescences." Thesis, Cardiff University, 2013. http://orca.cf.ac.uk/50885/.

Pełny tekst źródła
Streszczenie:
The detection of gravitational waves from the coalescence of two compact objects has been brought to within touching distance by the construction and operation of a global network of laser-interferometer detectors. However, the amplitude of the radiation from these events is so low that direct detection will require the combined innovations of advanced interferometry and detector characterisation, along with powerful methods of extracting weak, but modelled, signals from the background detector noise. This work focuses on enhancing the probability of such detection through improved identi�cati
Style APA, Harvard, Vancouver, ISO itp.
4

Renvoizé, Vincent. "Hydrodynamique et évolution d'objets compacts : binaires serrées et naines blanches." Lyon, École normale supérieure (sciences), 2002. http://www.theses.fr/2002ENSL0221.

Pełny tekst źródła
Streszczenie:
Le travail présenté est constitué de trois parties indépendantes. Dans la première partie, on étudie à l'aide de la technique SPH (Smoothed Particle Hydrodynamics) la déformation du secondaire au contact de Roche dans les variables cataclysmiques (CV). Ces déformations conduisent à une période orbitable plus grande que celle prévue par la troisième loi de Képler. La prise en compte de cette modification dans des modèles dévolution de CV explique partiellement pourquoi la période des CV observées a un minimum vers 80 minutes. La deuxième partie traite des binaires serrées de naines blanches. On
Style APA, Harvard, Vancouver, ISO itp.
5

Grover, Katherine L. "Physics and astrophysics with gravitational waves from compact binary coalescence in ground based interferometers." Thesis, University of Birmingham, 2015. http://etheses.bham.ac.uk//id/eprint/6410/.

Pełny tekst źródła
Streszczenie:
Advanced ground based laser interferometer gravitational wave detectors are due to come online in late 2015 and are expected to make the first direct detections of gravitational waves, with compact binary coalescence widely regarded as one of the most promising sources for detection. In Chapter I I compare two techniques for predicting the uncertainty of sky localization of these sources with full Bayesian inference. I find that timing triangulation alone tends to over-estimate the uncertainty and that average predictions can be brought to better agreement by the inclusion of phase consistency
Style APA, Harvard, Vancouver, ISO itp.
6

Germain, Vincent. "De l'étalonnage d'Advanced Virgo à la recherche d'ondes gravitationnelles émises par des coalescences de binaires compactes." Thesis, Université Grenoble Alpes (ComUE), 2017. http://www.theses.fr/2017GREAY101/document.

Pełny tekst źródła
Streszczenie:
L'ère de l'astronomie gravitationnelle a commencé avec la première détection d'une onde gravitationnelle le 14 septembre 2015, par la collaboration LIGO-Virgo. Les premières détections proviennent de coalescences de trous noirs de quelques dizaines de masses solaires. Le détecteur européen Advanced Virgo a redémarré en 2017 pour participer aux prochaines détections d'ondes gravitationnelles et localiser les sources astrophysiques.Cette thèse a pour sujet les différentes étapes du processus de détection des ondes gravitationnelles : de l'étalonnage du détecteur Advanced Virgo à l'analyse en tem
Style APA, Harvard, Vancouver, ISO itp.
7

Indik, Nathaniel [Verfasser]. "Optimal Template Placement for Searches of Gravitational Waves from Precessing Compact Binary Coalescences / Nathaniel Indik." Hannover : Gottfried Wilhelm Leibniz Universität, 2018. http://d-nb.info/1160378878/34.

Pełny tekst źródła
Style APA, Harvard, Vancouver, ISO itp.
8

Chan, Man Leong. "Optimization of electromagnetic follow up observations and localization of gravitational wave signals from compact binary coalescences." Thesis, University of Glasgow, 2018. http://theses.gla.ac.uk/31007/.

Pełny tekst źródła
Streszczenie:
Many gravitational wave sources will produce electromagnetic signals as they emit gravitational waves. An important example is binary neutron star mergers. The joint observations and discoveries of the electromagnetic signatures of these gravitational wave sources can produce substantial scientific benefits in physics, astrophysics and cosmology. To maximize the scientific outcomes of such gravitational events as much as possible, the detections of their electromagnetic signatures are necessary. The first detection of the inspiral signals from binary neutron stars by LIGO and VIRGO, and the ob
Style APA, Harvard, Vancouver, ISO itp.
9

McKechan, David J. A. "On the use of higher order wave forms in the search for gravitational waves emitted by compact binary coalescences." Thesis, Cardiff University, 2010. http://orca.cf.ac.uk/54982/.

Pełny tekst źródła
Streszczenie:
This thesis concerns the use, in gravitational wave data analysis, of higher order wave form models of the gravitational radiation emitted by compact binary coalescences. We begin with an introductory chapter that includes an overview of the theory of general relativity, gravitational radiation and ground-based interferometric gravitational wave detectors. We then discuss, in Chapter 2, the gravitational waves emitted by compact binary coalescences, with an explanation of higher order waveforms and how they differ from leading order waveforms we also introduce the post-Newtonian formalism. In
Style APA, Harvard, Vancouver, ISO itp.
10

Nitoglia, Elisa. "Gravitational-wave data analysis for standard and non-standard sources of compact binary coalescences in the third LIGO-Virgo observing run." Electronic Thesis or Diss., Lyon 1, 2023. http://www.theses.fr/2023LYO10143.

Pełny tekst źródła
Streszczenie:
Cette thèse de doctorat présente une enquête approfondie sur la détection des signaux d'ondes gravitationnelles provenant de fusions binaires compactes, en mettant l'accent particulier sur l'analyse des données de la troisième campagne d'observation de la Collaboration LIGO-Virgo. Le manuscrit commence par fournir une introduction aux principes fondamentaux de la théorie de la relativité générale, y compris la prédiction de l'existence des ondes gravitationnelles et un aperçu des sources astrophysiques qui génèrent ces ondes. Il fournit également une description détaillée des interféromètres,
Style APA, Harvard, Vancouver, ISO itp.
Więcej źródeł

Książki na temat "Coalescence de binaire compacte"

1

Colpi, Monica, Piergiorgio Casella, Vittorio Gorini, Ugo Moschella, and Andrea Possenti, eds. Physics of Relativistic Objects in Compact Binaries: From Birth to Coalescence. Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-9264-0.

Pełny tekst źródła
Style APA, Harvard, Vancouver, ISO itp.
2

Maggiore, Michele. GWs from compact binaries. Theory. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198570899.003.0005.

Pełny tekst źródła
Streszczenie:
An introduction to recent analytic and numerical breakthroughs in the modelisation of the final phases of the coalescence of compact binaries. Effective one-body technique. Numerical relativity. Spinning binaries. Superkicks and recoil of the final BH. Astrophysical consequences. Coalescences of neutron-star binaries.
Style APA, Harvard, Vancouver, ISO itp.
3

Physics of relativistic objects in compact binaries: From birth to coalescence. Springer, 2009.

Znajdź pełny tekst źródła
Style APA, Harvard, Vancouver, ISO itp.
4

Casella, Piergiorgio, Andrea Possenti, Monica Colpi, Vittorio Gorini, and Ugo Moschella. Physics of Relativistic Objects in Compact Binaries: From Birth to Coalescence. Springer Netherlands, 2014.

Znajdź pełny tekst źródła
Style APA, Harvard, Vancouver, ISO itp.

Części książek na temat "Coalescence de binaire compacte"

1

Pretorius, Frans. "Binary Black Hole Coalescence." In Physics of Relativistic Objects in Compact Binaries: From Birth to Coalescence. Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-9264-0_9.

Pełny tekst źródła
Style APA, Harvard, Vancouver, ISO itp.
2

Bulik, Tomasz. "The Coalescence Rates of Compact Object Binaries." In Gravitational Wave Astrophysics. Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-10488-1_2.

Pełny tekst źródła
Style APA, Harvard, Vancouver, ISO itp.
3

Heuvel, E. P. J. van den. "The Formation and Evolution of Relativistic Binaries." In Physics of Relativistic Objects in Compact Binaries: From Birth to Coalescence. Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-9264-0_4.

Pełny tekst źródła
Style APA, Harvard, Vancouver, ISO itp.
4

Israel, Gian Luca, and Simone Dall'Osso. "White Dwarfs in Ultrashort Binary Systems." In Physics of Relativistic Objects in Compact Binaries: From Birth to Coalescence. Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-9264-0_8.

Pełny tekst źródła
Style APA, Harvard, Vancouver, ISO itp.
5

Damour, Thibault. "Binary Systems as Test-Beds of Gravity Theories." In Physics of Relativistic Objects in Compact Binaries: From Birth to Coalescence. Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-9264-0_1.

Pełny tekst źródła
Style APA, Harvard, Vancouver, ISO itp.
6

Kramer, Michael. "Exploiting Binary Pulsars as Laboratories of Gravity Theories." In Physics of Relativistic Objects in Compact Binaries: From Birth to Coalescence. Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-9264-0_2.

Pełny tekst źródła
Style APA, Harvard, Vancouver, ISO itp.
7

Stella, L. "Strong Gravitational Field Diagnostics in Binary Systems Containing a Compact Object." In Physics of Relativistic Objects in Compact Binaries: From Birth to Coalescence. Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-9264-0_7.

Pełny tekst źródła
Style APA, Harvard, Vancouver, ISO itp.
8

Colpi, Monica, and Bernadetta Devecchi. "Dynamical Formation and Evolution of Neutron Star and Black Hole Binaries in Globular Clusters." In Physics of Relativistic Objects in Compact Binaries: From Birth to Coalescence. Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-9264-0_5.

Pełny tekst źródła
Style APA, Harvard, Vancouver, ISO itp.
9

Lazzati, Davide, and Rosalba Perna. "Short Gamma Ray Bursts: Marking the Birth of Black Holes from Coalescing Compact Binaries." In Physics of Relativistic Objects in Compact Binaries: From Birth to Coalescence. Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-9264-0_6.

Pełny tekst źródła
Style APA, Harvard, Vancouver, ISO itp.
10

D'Amico, Nichi, and Marta Burgay. "Perspective in the Search for Relativistic Pulsars." In Physics of Relativistic Objects in Compact Binaries: From Birth to Coalescence. Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-9264-0_3.

Pełny tekst źródła
Style APA, Harvard, Vancouver, ISO itp.

Streszczenia konferencji na temat "Coalescence de binaire compacte"

1

Buonanno, Alessandra, Ye-Fei Yuan, Xiang-Dong Li, and Dong Lai. "Binary Black Hole Coalescence." In ASTROPHYSICS OF COMPACT OBJECTS: International Conference on Astrophysics of Compact Objects. AIP, 2008. http://dx.doi.org/10.1063/1.2840417.

Pełny tekst źródła
Style APA, Harvard, Vancouver, ISO itp.
2

Caudill, Sarah. "Techniques for gravitational-wave detection of compact binary coalescence." In 2018 26th European Signal Processing Conference (EUSIPCO). IEEE, 2018. http://dx.doi.org/10.23919/eusipco.2018.8553549.

Pełny tekst źródła
Style APA, Harvard, Vancouver, ISO itp.
3

DEN BROECK, CHRIS VAN. "COMPACT BINARY COALESCENCE AND THE SCIENCE CASE FOR EINSTEIN TELESCOPE." In Proceedings of the MG12 Meeting on General Relativity. WORLD SCIENTIFIC, 2012. http://dx.doi.org/10.1142/9789814374552_0302.

Pełny tekst źródła
Style APA, Harvard, Vancouver, ISO itp.
4

Takeda, Hiroki, Yuta Michimura, Kentaro Komori, et al. "Polarization test of gravitational waves from compact binary coalescences." In Proceedings of the MG15 Meeting on General Relativity. WORLD SCIENTIFIC, 2022. http://dx.doi.org/10.1142/9789811258251_0247.

Pełny tekst źródła
Style APA, Harvard, Vancouver, ISO itp.
5

Marion, F., Vicky Kologera, and Marc van der Sluys. "Searches for Gravitational Waves from Compact Binary Coalescences with the LIGO and Virgo Detectors." In INTERNATIONAL CONFERENCE ON BINARIES: In celebration of Ron Webbink’s 65th Birthday. AIP, 2010. http://dx.doi.org/10.1063/1.3536398.

Pełny tekst źródła
Style APA, Harvard, Vancouver, ISO itp.
6

Verma, Chetan, Amit Reza, Dilip Krishnaswamy, Sarah Caudill, and Gurudatt Gaur. "Employing deep learning for detection of gravitational waves from compact binary coalescences." In INNOVATIONS IN COMPUTATIONAL AND COMPUTER TECHNIQUES: ICACCT-2021. AIP Publishing, 2022. http://dx.doi.org/10.1063/5.0108682.

Pełny tekst źródła
Style APA, Harvard, Vancouver, ISO itp.
7

Sasaoka, Seiya, Yilun Hou, Diego Sebastian Dominguez, et al. "Deep Learning for Detecting Gravitational Waves from Compact Binary Coalescences and Its Visualization by Grad-CAM." In 38th International Cosmic Ray Conference. Sissa Medialab, 2023. http://dx.doi.org/10.22323/1.444.1498.

Pełny tekst źródła
Style APA, Harvard, Vancouver, ISO itp.
Możesz być także zainteresowany rozszerzonymi bibliografiami na temat „Coalescence de binaire compacte” dla poszczególnych typów źródeł:
Artykuły w czasopismach Rozprawy doktorskie
Oferujemy zniżki na wszystkie plany premium dla autorów, których prace zostały uwzględnione w tematycznych zestawieniach literatury. Skontaktuj się z nami, aby uzyskać unikalny kod promocyjny!

Do bibliografii