Gotowe bibliografie tematyczne / Laser interferometer space antenna (satellite artificiel)

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Gotowa bibliografia na temat „Laser interferometer space antenna (satellite artificiel)”

Autor: Grafiati
Data publikacji: 2 listopada 2024
Data aktualizacji: 31 lipca 2025

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Artykuły w czasopismach na temat "Laser interferometer space antenna (satellite artificiel)"

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Liu, He-Shan, Zi-Ren Luo, and Wei Sha. "In-orbit performance of the laser interferometer of Taiji-1 experimental satellite." International Journal of Modern Physics A 36, no. 11n12 (2021): 2140004. http://dx.doi.org/10.1142/s0217751x21400042.

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Taiji-1, which is the first experimental satellite for space gravitational wave detection in China, relies on key technologies which include the laser interferometer, the gravitational reference sensor (GRS), the micro-thruster and the satellite platform. Similarly to the Laser Interferometer Space Antenna (LISA) pathfinder, except for the science interferometer, the optical bench (OB) of Taiji-1 contains reference and test mass (TM) interferometers. Limited by the lower mechanical strength of the carrier rocket and by the orbit environment, the OB of Taiji-1 is made of invar steel and fused s
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Gan, Li, Davor Mance, and Peter Zweifel. "Actuation to sensing crosstalk investigation in the inertial sensor front-end electronics of the laser interferometer space antenna pathfinder satellite." Sensors and Actuators A: Physical 167, no. 2 (2011): 574–80. http://dx.doi.org/10.1016/j.sna.2011.03.011.

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Korol, Valeriya, Vasily Belokurov, Christopher J. Moore, and Silvia Toonen. "Weighing Milky Way satellites with LISA." Monthly Notices of the Royal Astronomical Society: Letters 502, no. 1 (2021): L55—L60. http://dx.doi.org/10.1093/mnrasl/slab003.

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ABSTRACT White dwarf stars are a well-established tool for studying Galactic stellar populations. Two white dwarfs in a tight binary system offer us an additional messenger – gravitational waves – for exploring the Milky Way and its immediate surroundings. Gravitational waves produced by double white dwarf (DWD) binaries can be detected by the future Laser Interferometer Space Antenna (LISA). Numerous and widespread DWDs have the potential to probe shapes, masses, and formation histories of the stellar populations in the Galactic neighbourhood. In this work we outline a method for estimating t
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NI, WEI-TOU. "EMPIRICAL FOUNDATIONS OF THE RELATIVISTIC GRAVITY." International Journal of Modern Physics D 14, no. 06 (2005): 901–21. http://dx.doi.org/10.1142/s0218271805007139.

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In 1859, Le Verrier discovered the mercury perihelion advance anomaly. This anomaly turned out to be the first relativistic-gravity effect observed. During the 141 years to 2000, the precisions of laboratory and space experiments, and astrophysical and cosmological observations on relativistic gravity have been improved by 3 orders of magnitude. In 1999, we envisaged a 3–6 order improvement in the next 30 years in all directions of tests of relativistic gravity. In 2000, the interferometric gravitational wave detectors began their runs to accumulate data. In 2003, the measurement of relativist
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Lamberts, Astrid, Sarah Blunt, Tyson B. Littenberg, Shea Garrison-Kimmel, Thomas Kupfer, and Robyn E. Sanderson. "Predicting the LISA white dwarf binary population in the Milky Way with cosmological simulations." Monthly Notices of the Royal Astronomical Society 490, no. 4 (2019): 5888–903. http://dx.doi.org/10.1093/mnras/stz2834.

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ABSTRACT White dwarf binaries with orbital periods below 1 h will be the most numerous sources for the space-based gravitational wave detector Laser Interferometer Space Antenna (LISA). Based on thousands of individually resolved systems, we will be able to constrain binary evolution and provide a new map of the Milky Way and its close surroundings. In this paper we predict the main properties of populations of different types of detached white dwarf binaries detected by LISA over time. For the first time, we combine a high-resolution cosmological simulation of a Milky Way-mass galaxy (taken f
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Korol, V., S. Toonen, A. Klein, et al. "Populations of double white dwarfs in Milky Way satellites and their detectability with LISA." Astronomy & Astrophysics 638 (June 2020): A153. http://dx.doi.org/10.1051/0004-6361/202037764.

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Context. Milky Way dwarf satellites are unique objects that encode the early structure formation and therefore represent a window into the high redshift Universe. So far, their study has been conducted using electromagnetic waves only. The future Laser Interferometer Space Antenna (LISA) has the potential to reveal Milky Way satellites through gravitational waves emitted by double white dwarf (DWD) binaries. Aims. We investigate gravitational wave signals that will be detectable by LISA as a possible tool for the identification and characterisation of the Milky Way satellites. Methods. We used
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Beck, Marcel, Shreevathsa Chalathadka Subrahmanya, and Oliver Gerberding. "Adjustable picometer-stable interferometers for testing space-based gravitational wave detectors." Classical and Quantum Gravity, June 6, 2025. https://doi.org/10.1088/1361-6382/ade1c7.

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Abstract Space-based gravitational wave detectors, such as the Laser Interferometer Space Antenna (LISA), use picometer-precision laser interferometry to detect gravitational waves at frequencies from 1 Hz down to below 0.1 mHz. Laser interferometers used for on-ground prototyping and testing of such instruments are typically constructed by permanently bonding or gluing optics onto an ultra-stable bench made of low-expansion glass ceramic. This design minimizes temperature coupling to length and tilt, which dominates the noise at low frequencies due to finite temperature stability achievable i
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Rozprawy doktorskie na temat "Laser interferometer space antenna (satellite artificiel)"

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Dichtl, Maximilian. "Aspects of cosmological first order phase transitions : propagation of ultra-relativistic shells, heavy dark matter, and baryogenesis." Electronic Thesis or Diss., Sorbonne université, 2024. http://www.theses.fr/2024SORUS181.

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Les transitions de phase du premier ordre (PT) dans l'univers primitif se produisent par la nucléation de bulles dont les parois peuvent se dilater à des vitesses ultra-relativistes. Les interactions du bain thermique à la paroi produisent des particules qui s'accumulent dans des coquilles à la paroi. Les coquilles évoluent jusqu'à ce qu'elles entrent en collision avec celles des bulles voisines. Dans cette thèse, nous étudions d'abord l'évolution de ces coquilles, en incluant pour la première fois les interactions de changement de nombre de la coquille à l'intérieur d'elle-même et avec le bai
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Streszczenia konferencji na temat "Laser interferometer space antenna (satellite artificiel)"

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Sánchez Maestro, Raúl, Joost Veenman, Jorge Cardin, Jonathan Grzymisch, and Valentin Preda. "GNC functional architecture design and implementation of the LISA drag-free control system." In ESA 12th International Conference on Guidance Navigation and Control and 9th International Conference on Astrodynamics Tools and Techniques. ESA, 2023. http://dx.doi.org/10.5270/esa-gnc-icatt-2023-119.

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The LISA (Laser Interferometer Space Antenna) mission is one of the most challenging endeavours to be undertaken by ESA whose objective is to study gravitational waves. The mission consists of three identical spacecraft in a triangular formation, with an inter-satellite distance of 2.5 million km, flying in a heliocentric orbit. Each spacecraft contains two test masses (TM) that are confined within an electrode housing with electrostatic sensing and actuation capability. Two telescopes are present, pointing towards the two other spacecraft, which includes a sophisticated optical metrology syst
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