Academic literature on the topic 'Laser interferometer space antenna (satellite artificiel)'
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Journal articles on the topic "Laser interferometer space antenna (satellite artificiel)"
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 (February 22, 2021): 2140004. http://dx.doi.org/10.1142/s0217751x21400042.
Full textGan, 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 (June 2011): 574–80. http://dx.doi.org/10.1016/j.sna.2011.03.011.
Full textKorol, 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 (January 14, 2021): L55—L60. http://dx.doi.org/10.1093/mnrasl/slab003.
Full textNI, WEI-TOU. "EMPIRICAL FOUNDATIONS OF THE RELATIVISTIC GRAVITY." International Journal of Modern Physics D 14, no. 06 (June 2005): 901–21. http://dx.doi.org/10.1142/s0218271805007139.
Full textLamberts, 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 (October 10, 2019): 5888–903. http://dx.doi.org/10.1093/mnras/stz2834.
Full textKorol, V., S. Toonen, A. Klein, V. Belokurov, F. Vincenzo, R. Buscicchio, D. Gerosa, 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.
Full textDissertations / Theses on the topic "Laser interferometer space antenna (satellite artificiel)"
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.
Full textFirst order phase transitions (PT) in the early universe happen via the nucleation of bubbles whose walls can expand at ultra-relativistic velocities. Interactions of the thermal bath at the wall produce particles which accumulate in shells at the wall. The shells evolve until they collide with those from neighboring bubbles. In this thesis we first study the evolution of these shells, including for the first time number changing interactions of the shell within itself and with the thermal bath. In particular, we calculate the rates of the dominant 3 → 2 scattering processes, and find they can be more important than all other processes considered in previous literature. We identify the regions of parameter space of the PT where the shells free stream, i.e. they have negligible interactions within themselves and with the bath. We then use these results to predict the rate and energy with which particles of opposite bubbles collide. We find that these particle collisions can reach scattering energies much larger than the scale of the PT, which in turn can be used to produce highly energetic particles or particles much heavier than the scale of the PT, realising a cosmological 'bubbletron'. As an example, we show that one can produce heavy dark matter with masses above 10^3 TeV for scales of the PT of around 10 MeV, and with masses above the GUT scale for scales of the PT above about 10^9 GeV. PTs with ultra-relativistic walls are also relevant for any other process relying on out-of-equilibrium particle production. If the interaction between particles in the shell also violates Baryon number, C, and CP, then all three Sakharov conditions are satisifed, and one can use these PTs to explain the baryon asymmetry of the universe. We do so by proposing a mechanism of baryogenesis from supercooled confining PTs. We also compute the gravitational wave signature due to the PT in all the above scenarios. We find they could be seen by pulsar timing arrays and gravitational wave interferometers like LISA and the Einstein Telescope, realizing a new link between these telescopes and the possible origin of dark matter and of the baryon asymmetry of the universe
Conference papers on the topic "Laser interferometer space antenna (satellite artificiel)"
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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