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"Lisa"
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New horizons for fundamental physics with LISA
by
Fleury, Pierre
,
Orlando, Giorgio
,
Gualtieri, Leonardo
in
Astrophysics
,
Black holes
,
Consortia
2022
The Laser Interferometer Space Antenna (LISA) has the potential to reveal wonders about the fundamental theory of nature at play in the extreme gravity regime, where the gravitational interaction is both strong and dynamical. In this white paper, the Fundamental Physics Working Group of the LISA Consortium summarizes the current topics in fundamental physics where LISA observations of gravitational waves can be expected to provide key input. We provide the briefest of reviews to then delineate avenues for future research directions and to discuss connections between this working group, other working groups and the consortium work package teams. These connections must be developed for LISA to live up to its science potential in these areas.
Journal Article
A double life : discovering motherhood
Motherhood splits a woman's life forever, into a before and an after. Harper brings her sense of humor as she explores the emotional and biological transformations that motherhood entails, and documents her own journey across this great divide.
Cosmology with the Laser Interferometer Space Antenna
2023
The Laser Interferometer Space Antenna (LISA) has two scientific objectives of cosmological focus: to probe the expansion rate of the universe, and to understand stochastic gravitational-wave backgrounds and their implications for early universe and particle physics, from the MeV to the Planck scale. However, the range of potential cosmological applications of gravitational-wave observations extends well beyond these two objectives. This publication presents a summary of the state of the art in LISA cosmology, theory and methods, and identifies new opportunities to use gravitational-wave observations by LISA to probe the universe.
Journal Article
Have a nice guilt trip
\"Everyone's favorite mother-daughter writing duo is back with a new collection of warm and witty stories that will strike a chord with every woman. With twenty-something Francesca navigating New York City, Lisa holding down the fort in the suburbs, and Mother Mary making frequent and always entertaining appearances, there are plenty of opportunities for family-induced guilt, fighting, laughter, and love. As Lisa says, \"Bottom line, if you're a mom, you'll feel guilty all the time, and this is true because you're a daughter as well, and God only knows how many times you failed your poor mother.\" So come along for the ride as Lisa and Francesca continue on the road of life acquiring men and puppies...Ok, to be honest, Lisa is acquiring the puppies, while Francesca is lucky enough to have dates with actual men. They'll leave it to readers to decide which is more desirable and/or or easier to train.\"--Page 4 of cover.
Primordial black holes and their gravitational-wave signatures
by
García-Bellido, Juan
,
Vennin, Vincent
,
Bagui, Eleni
in
Astrophysics
,
Astrophysics and Astroparticles
,
Binary stars
2025
In the recent years, primordial black holes (PBHs) have emerged as one of the most interesting and hotly debated topics in cosmology. Among other possibilities, PBHs could explain both some of the signals from binary black hole mergers observed in gravitational-wave detectors and an important component of the dark matter in the Universe. Significant progress has been achieved both on the theory side and from the point of view of observations, including new models and more accurate calculations of PBH formation, evolution, clustering, merger rates, as well as new astrophysical and cosmological probes. In this work, we review, analyze and combine the latest developments in order to perform end-to-end calculations of the various gravitational-wave signatures of PBHs. Different ways to distinguish PBHs from stellar black holes are emphasized. Finally, we discuss their detectability with LISA, the first planned gravitational-wave observatory in space.
Journal Article
Astrophysics with the Laser Interferometer Space Antenna
2023
The Laser Interferometer Space Antenna (LISA) will be a transformative experiment for gravitational wave astronomy, and, as such, it will offer unique opportunities to address many key astrophysical questions in a completely novel way. The synergy with ground-based and space-born instruments in the electromagnetic domain, by enabling multi-messenger observations, will add further to the discovery potential of LISA. The next decade is crucial to prepare the astrophysical community for LISA’s first observations. This review outlines the extensive landscape of astrophysical theory, numerical simulations, and astronomical observations that are instrumental for modeling and interpreting the upcoming LISA datastream. To this aim, the current knowledge in three main source classes for LISA is reviewed; ultra-compact stellar-mass binaries, massive black hole binaries, and extreme or interme-diate mass ratio inspirals. The relevant astrophysical processes and the established modeling techniques are summarized. Likewise, open issues and gaps in our understanding of these sources are highlighted, along with an indication of how LISA could help making progress in the different areas. New research avenues that LISA itself, or its joint exploitation with upcoming studies in the electromagnetic domain, will enable, are also illustrated. Improvements in modeling and analysis approaches, such as the combination of numerical simulations and modern data science techniques, are discussed. This review is intended to be a starting point for using LISA as a new discovery tool for understanding our Universe.
Journal Article
Renoir : the body, the senses
by
Bell, Esther, editor
,
Bailey, Colin B., contributor
,
Clark Art Institute, publisher
in
Renoir, Auguste, 1841-1919 Exhibitions.
,
Yuskavage, Lisa, 1962- Interviews.
,
Nude in art Exhibitions.
2019
Best known as part of the influential vanguard of Impressionist artists that experimented with new painting techniques in the late 19th century, Pierre-Auguste Renoir (1841-1919) was deeply inspired by classical traditions and returned again and again to the canonical subject of the nude. Tracing the entire arc of Renoir's career, this volume examines the different approaches the artist employed in his various depictions of the subject-from his works that respond to Gustave Courbet, Edouard Manet, Edgar Degas, and Paul Cezanne, to his late, and still controversial, depictions of bathers that inspired the next generation of artists. Eminent scholars not only look at the different ways that Renoir used the nude as a means of personal expression but also analyze Renoir's art in terms of a modern feminist critique of the male gaze. Offering the first-ever comprehensive investigation of Renoir's nudes, this beautifully illustrated study includes approximately 50 works, including paintings, pastels, drawings, and sculptures. The book also features an interview with the contemporary figurative painter Lisa Yuskavage that considers Renoir's continuing influence and the historical significance of the female nude in art. Exhibition: Clark Art Institute, Williamstown, USA (08.06-22.09.2018); Kimbell Art Museum, Fort Worth, USA (27.10.2019-26.01.2020).
Time-delay interferometry
by
Tinto, Massimo
,
Dhurandhar, Sanjeev V.
in
Astrophysics and Astroparticles
,
Classical and Quantum Gravitation
,
Cosmology
2021
Equal-arm detectors of gravitational radiation allow phase measurements many orders of magnitude below the intrinsic phase stability of the laser injecting light into their arms. This is because the noise in the laser light is common to both arms, experiencing exactly the same delay, and thus cancels when it is differenced at the photo detector. In this situation, much lower level secondary noises then set the overall performance. If, however, the two arms have different lengths (as will necessarily be the case with space-borne interferometers), the laser noise experiences different delays in the two arms and will hence not directly cancel at the photo detector. To solve this problem, a technique involving heterodyne interferometry with unequal arm lengths and independent phase-difference readouts has been proposed. It relies on properly time-shifting and linearly combining independent Doppler measurements, and for this reason it has been called time-delay interferometry (TDI). This article provides an overview of the theory, mathematical foundations, and experimental aspects associated with the implementation of TDI. Although emphasis on the application of TDI to the Laser Interferometer Space Antenna mission appears throughout this article, TDI can be incorporated into the design of any future space-based mission aiming to search for gravitational waves via interferometric measurements. We have purposely left out all theoretical aspects that data analysts will need to account for when analyzing the TDI data combinations.
Journal Article