Astro2010 Decadal Survey Whitepaper: Coordinated Science in the Gravitational and Electromagnetic Skies
arXiv:0902.1527 · doi:10.1016/j.asr.2012.09.019
Abstract
It is widely expected that the coming decade will witness the first direct detection of gravitational waves (GWs). The ground-based LIGO and Virgo GW observatories are being upgraded to advanced sensitivity, and are expected to observe a significant binary merger rate. The launch of The Laser Interferometer Space Antenna (LISA) would extend the GW window to low frequencies, opening new vistas on dynamical processes involving massive (M >~ 10^5 M_Sun) black holes. GW events are likely to be accompanied by electromagnetic (EM) counterparts and, since information carried electromagnetically is complementary to that carried gravitationally, a great deal can be learned about an event and its environment if it becomes possible to measure both forms of radiation in concert. Measurements of this kind will mark the dawn of trans-spectral astrophysics, bridging two distinct spectral bands of information. The aim of this whitepaper is to articulate future directions in both theory and observation that are likely to impact broad astrophysical inquiries of general interest. What will EM observations reflect on the nature and diversity of GW sources? Can GW sources be exploited as complementary probes of cosmology? What cross-facility coordination will expand the science returns of gravitational and electromagnetic observations?
7 pages (plus one coverpage), submitted to the US Astro2010 Decadal Survey. This is a living document, with updates expected to be posted to this archive. Those interested in contributing should contact J. S. Bloom
References in corpus (39)
- Dynamics of dark energy
- Physics, Astrophysics and Cosmology with Gravitational Waves
- Formation of Supermassive Black Holes
- The international pulsar timing array project: using pulsars as a gravitational wave detector
- The stochastic gravitational-wave background from massive black hole binary systems: implications for observations with Pulsar Timing Arrays
- An Upper Limit on the Stochastic Gravitational-Wave Background of Cosmological Origin
- Gravitational wave stochastic background from cosmic (super)strings
- Gravitational waves from resolvable massive black hole binary systems and observations with Pulsar Timing Arrays
- Direct Formation of Supermassive Black Holes via Multi-Scale Gas Inflows in Galaxy Mergers
- GRB 080503: Implications of a Naked Short Gamma-Ray Burst Dominated by Extended Emission
- General relativistic simulations of magnetized binary neutron star mergers
- Fully General Relativistic Simulations of Black Hole-Neutron Star Mergers
- Probing reheating temperature of the universe with gravitational wave background
- Host Galaxies Catalog Used in LIGO Searches for Compact Binary Coalescence Events
- Implications for the Origin of GRB 070201 from LIGO Observations
- Beating the spin-down limit on gravitational wave emission from the Vela pulsar
- Reconstructing the massive black hole cosmic history through gravitational waves
- Merger of black hole and neutron star in general relativity: Tidal disruption, torus mass, and gravitational waves
- Massive Black Hole Binary Inspirals: Results from the LISA Parameter Estimation Taskforce
- Neutron-Rich Freeze-Out in Viscously Spreading Accretion Disks Formed from Compact Object Mergers
- Space laser interferometers can determine the thermal history of the early Universe
- Major Galaxy Mergers and the Growth of Supermassive Black Holes in Quasars
- Localizing coalescing massive black hole binaries with gravitational waves
- Delensing Gravitational Wave Standard Sirens with Shear and Flexion Maps
- Identifying Decaying Supermassive Black Hole Binaries from their Variable Electromagnetic Emission
- Gravitational waves from merging compact binaries
- Observing white dwarfs orbiting massive black holes in the gravitational wave and electro-magnetic window
- Pre-Merger Localization of Gravitational-Wave Standard Sirens With LISA I: Harmonic Mode Decomposition
- The inflationary gravitational-wave background and measurements of the scalar spectral index
- B-Pol: Detecting Primordial Gravitational Waves Generated During Inflation
- Weak lensing effects in the measurement of the dark energy equation of state with LISA
- The Experimental Probe of Inflationary Cosmology (EPIC): A Mission Concept Study for NASA's Einstein Inflation Probe
- Orbit optimization for ASTROD-GW and its time delay interferometry with two arms using CGC ephemeris
- LISA as a dark energy probe
- Gravitational waves, dark energy and inflation
- Linking optical and infrared observations with gravitational wave sources through variability
- Cosmic Polarization Rotation, Cosmological Models, and the Detectability of Primordial Gravitational Waves
- Gravitational Wave Bursts from Collisions of Primordial Black Holes in Clusters
- Possible use of self-calibration to reduce systematic uncertainties in determining distance-redshift relation via gravitational radiation from merging binaries
Cited by in corpus (40)
- Effect of a High Opacity on the Light Curves of Radioactively Powered Transients from Compact Object Mergers
- The long-term evolution of neutron star merger remnants - II. Radioactively powered transients
- Triangulation of gravitational wave sources with a network of detectors
- Dark Matter and Fundamental Physics with the Cherenkov Telescope Array
- Outflows from accretion disks formed in neutron star mergers: effect of black hole spin
- Imprints of neutrino-pair flavor conversions on nucleosynthesis in ejecta from neutron-star merger remnants
- Unification of inflation and dark energy {\it à la} quintessential inflation
- THESEUS: a key space mission concept for Multi-Messenger Astrophysics
- A Revised View of the Transient Radio Sky
- The Deep and Transient Universe in the SVOM Era: New Challenges and Opportunities - Scientific prospects of the SVOM mission
- GRB beaming and gravitational-wave observations
- Swift follow-up observations of candidate gravitational-wave transient events
- Linking electromagnetic and gravitational radiation in coalescing binary neutron stars
- Electromagnetic Counterparts to Black Hole Mergers
- Gravitational wave detection in space
- The Transient Gravitational-Wave Sky
- Astrophysics of Super-massive Black Hole Mergers
- Identifying the Host Galaxy of Gravitational Wave Signals
- Multi-messenger approaches to binary supermassive black holes in the "continuous-wave" regime
- Reconstructing the Properties of Dark Energy using Standard Sirens
- Orbit optimization for ASTROD-GW and its time delay interferometry with two arms using CGC ephemeris
- Numerical simulation of time delay interferometry for a LISA-like mission with the simplification of having only one interferometer
- Gravitational Wave Memory from Gamma Ray Bursts' Jets
- Blindly Detecting Merging Supermassive Black Holes with Radio Surveys
- Orbit optimization and time delay interferometry for inclined ASTROD-GW formation with half-year precession-period
- Numerical simulation of time delay interferometry for eLISA/NGO
- Astrophysical Prior Information and Gravitational-wave Parameter Estimation
- The Transient High-Energy Sky and Early Universe Surveyor (THESEUS)
- Electromagnetic Counterparts of Gravitational Wave Sources : Mergers of Compact Objects
- Multi-messenger astronomy of gravitational-wave sources with flexible wide-area radio transient surveys
- Light from the Cosmic Frontier: Gamma-Ray Bursts
- Probing neutron stars with gravitational waves
- Compton echoes from nearby Gamma-Ray Bursts
- Estimates of the early EM emission from compact binary mergers
- Multi-Messenger Astronomy with Extremely Large Telescopes
- The Dynamic Radio Sky: An Opportunity for Discovery
- Large-Scale Image Processing with the ROTSE Pipeline for Follow-Up of Gravitational Wave Events
- Gravitational Wave Astrophysics: Opening the New Frontier
- Revealing the First Stellar and Supermassive Black Holes to EXIST
- Surveying the Extreme Sky with EXIST