Beyond LISA: Exploring Future Gravitational Wave Missions
arXiv:gr-qc/0506015 · doi:10.1103/PhysRevD.72.083005
Abstract
The Advanced Laser Interferometer Antenna (ALIA) and the Big Bang Observer (BBO) have been proposed as follow on missions to the Laser Interferometer Space Antenna (LISA). Here we study the capabilities of these observatories, and how they relate to the science goals of the missions. We find that the Advanced Laser Interferometer Antenna in Stereo (ALIAS), our proposed extension to the ALIA mission, will go considerably further toward meeting ALIA's main scientific goal of studying intermediate mass black holes. We also compare the capabilities of LISA to a related extension of the LISA mission, the Laser Interferometer Space Antenna in Stereo (LISAS). Additionally, we find that the initial deployment phase of the BBO would be sufficient to address the BBO's key scientific goal of detecting the Gravitational Wave Background, while still providing detailed information about foreground sources.
9 pages, 10 figures, published version
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- Constraining scotogenic dark matter and primordial black holes using gravitational waves
- Modeling the Beam of Gravitational Radiation from a Cosmic String Loop
- Comprehensive analysis of dissipative effects in the induced gravitational waves
- A quantisation procedure in the presence of an initial Kasner singularity: primordial gravitational waves from triaxially anisotropic pre-inflation
- Stochastic gravitational wave from graviton bremsstrahlung in inflaton decay into massive spin 3/2 particles
- Stochastic gravitational wave background anisotropies from inflation with non-Bunch-Davies states
- Observing Double White Dwarfs with the Lunar GW Antenna
- Complementary signatures of attractor inflation in CMB and cosmic string Gravitational Waves
- Simulating first-order phase transition during inflation
- Time evolution of the equation of state during perturbative reheating and its impact on the inflationary tensor perturbation spectrum
- Constraints and detection capabilities of GW polarizations with space-based detectors in different TDI combinations
- Precision requirements and innovative manufacturing for ultrahigh precision laser interferometry of gravitational-wave astronomy
- Model-agnostic gravitational-wave background characterization algorithm
- Primordial gravitational waves: Model effects on time evolution and spectrum
- Initial acquisition requirements for optical cavities in the space gravitational wave antennae DECIGO and B-DECIGO
- Reconstructing ACT-compatible and GW170817-compatible Einstein-Gauss-Bonnet Inflation from the Observational Indices
- Purely quadratic non-Gaussianity from tachyonic instability: Primordial black holes and scalar-induced gravitational waves
- Study of gravitational waves from phase transitions in three-component dark matter
- A singlet scalar assisted Leptogenesis and Pseudo-Scalar Dark Matter
- Dynamical-System analysis of single-axion monodromy inflation with periodically-modulated potentials
- Probing Bose-enhanced Inflaton Decay with Gravitational Waves
- Cosmic Collider Gravitational Waves sourced by Right-handed Neutrino production from Bubbles: Testing Seesaw, Leptogenesis and Dark Matter
- Baryogenesis via relativistic bubble walls
- Probing the Neutrino Seesaw Scale with Gravitational Waves
- The new generation lunar gravitational wave detectors: sky map resolution and joint analysis
- Gravitational Wave Probe of Singlet-Doublet Dark Matter Induced Radiative Neutrino Mass
- Gravitational Radiation from Accelerating Jets
- Mutated hilltop inflation in light of Planck/ACT observations
- Dark Matter Freeze-in from a Reheaton
- Primordial observables of explicit diffeomorphism violation in gravity
- Model-independent constraints on inflation and reheating
- Continuous Gravitational Waves from Supersoft X-ray Sources: Promising Targets for deci-Hz Detectors
- Testing Nambu-Goto approximation of cosmic string by lattice field simulations