Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- D. Stern3 profiles493 · h 97
- F. Harrison2 profiles182 · h 58
- P. Eisenhardt3 profiles168 · h 59
- S. Boggs124 · h 60
- F. Christensen123 · h 58
- C. Hailey120 · h 59
- W. Craig2 profiles120 · h 49
- S. Stanford2 profiles117 · h 75
- S. Turyshev116 · h 38
- D. Walton2 profiles108 · h 53
- K. Stapelfeldt104 · h 70
- D. Mawet98 · h 53
- California Institute of TechnologyUS4.7k papers
- Centre National de la Recherche ScientifiqueFR2k papers
- Center for Astrophysics Harvard & SmithsonianUS1.3k papers
- Goddard Space Flight CenterUS1.2k papers
- University of California, BerkeleyUS1.2k papers
- University of ArizonaUS1k papers
- Infrared Processing and Analysis CenterUS1k papers
- University College LondonGB984 papers
- Princeton UniversityUS924 papers
- University of CambridgeGB871 papers
- Institut d'Astrophysique de ParisFR858 papers
- Space Telescope Science InstituteUS808 papers
19 papers · 2 filters
General relativistic observables of the GRAIL mission
Slava G. Turyshev, Viktor T. Toth, Mikhail V. Sazhin
We present a realization of astronomical relativistic reference frames in the solar system and its application to the GRAIL mission. We model the necessary spacetime coordinate tra…
Testing General Relativity with Low-Frequency, Space-Based Gravitational-Wave Detectors
Jonathan R. Gair, Michele Vallisneri, Shane L. Larson +1
We review the tests of general relativity that will become possible with space-based gravitational-wave detectors operating in the ~0.01mHz - 1Hz low-frequency band. The fundamenta…
Prospects for probing strong gravity with a pulsar-black hole system
N. Wex, K. Liu, R. P. Eatough +3
The discovery of a pulsar (PSR) in orbit around a black hole (BH) is expected to provide a superb new probe of relativistic gravity and BH properties. Apart from a precise mass mea…
Extended gravity with generalized scalar field and kinetic term dependences
Tiberiu Harko, Francisco S. N. Lobo, Olivier Minazzoli
We generalize previous work by considering a novel gravitational model with an action given by an arbitrary function of the Ricci scalar, the matter Lagrangian density, a scalar fi…
Outlook for detection of GW inspirals by GRB-triggered searches in the Advanced detector era
Alexander Dietz, Nickolas Fotopoulos, Leo Singer +1
Short, hard gamma-ray bursts (GRBs) are believed to originate from the coalescence of two neutron stars (NSs) or a NS and a black hole (BH). If this scenario is correct, then short…
The classical mechanics of non-conservative systems
Chad R. Galley
Hamilton's principle of stationary action lies at the foundation of theoretical physics and is applied in many other disciplines from pure mathematics to economics. Despite its uti…
New derivation of the Lagrangian of a perfect fluid with a barotropic equation of state
Olivier Minazzoli, Tiberiu Harko
In this paper we give a simple proof that when the particle number is conserved, the Lagrangian of a barotropic perfect fluid is , where $ρ…
Searching for gravitational waves from binary coalescence
S. Babak, R. Biswas, P. R. Brady +25
We describe the implementation of a search for gravitational waves from compact binary coalescences in LIGO and Virgo data. This all-sky, all-time, multi-detector search for binary…
Testing general relativity with gravitational waves: a reality check
Michele Vallisneri
The observations of gravitational-wave signals from astrophysical sources such as binary inspirals will be used to test General Relativity for self consistency and against alternat…
Reply to "Comment on 'Finite size corrections to the radiation reaction force in classical electrodynamics'"
Chad R. Galley, Adam K. Leibovich, Ira Z. Rothstein
We reply to P. Forgács, T. Herpay, and P. Kovács (arXiv: 1202.6289).
Specialized Orthonormal Frames and Embedding
Frank B. Estabrook
We discuss some specializations of the frames of flat orthonormal frame bundles over geometries of indefinite signature, and the resulting symmetries of families of embedded Rieman…
Caustic echoes from a Schwarzschild black hole
Anıl Zenginoğlu, Chad R. Galley
We present the first numerical construction of the scalar Schwarzschild Green function in the time-domain, which reveals several universal features of wave propagation in black hol…
Towards beating the curse of dimensionality for gravitational waves using Reduced Basis
Frank Herrmann, Scott E. Field, Chad R. Galley +2
Using the Reduced Basis approach, we efficiently compress and accurately represent the space of waveforms for non-precessing binary black hole inspirals, which constitutes a four d…
Radiation reaction at 3.5 post-Newtonian order in effective field theory
Chad R. Galley, Adam K. Leibovich
We derive the radiation reaction forces on a compact binary inspiral through 3.5 order in the post-Newtonian expansion using the effective field theory approach. We utilize a recen…
Chameleon effect and the Pioneer anomaly
John D. Anderson, J. R. Morris
The possibility that the apparent anomalous acceleration of the Pioneer 10 and 11 spacecraft may be due, at least in part, to a chameleon field effect is examined. A small spacecra…
Support for the thermal origin of the Pioneer anomaly
Slava G. Turyshev, Viktor T. Toth, Gary Kinsella +3
We investigate the possibility that the anomalous acceleration of the Pioneer 10 and 11 spacecraft is due to the recoil force associated with an anisotropic emission of thermal rad…
Lunar Laser Ranging Tests of the Equivalence Principle
James G. Williams, Slava G. Turyshev, Dale Boggs
The Lunar Laser Ranging (LLR) experiment provides precise observations of the lunar orbit that contribute to a wide range of science investigations. In particular, time series of h…
Low-frequency gravitational-wave science with eLISA/NGO
Pau Amaro-Seoane, Sofiane Aoudia, Stanislav Babak +27
We review the expected science performance of the New Gravitational-Wave Observatory (NGO, a.k.a. eLISA), a mission under study by the European Space Agency for launch in the early…
Non-sky-averaged sensitivity curves for space-based gravitational-wave observatories
Michele Vallisneri, Chad R. Galley
(abridged) The signal-to-noise ratio (SNR) is used in gravitational-wave observations as the basic figure of merit for detection confidence and, together with the Fisher matrix, fo…