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LISA Sensitivity and SNR Calculations
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This Technical Note (LISA reference LISA-LCST-SGS-TN-001) describes the computation of the noise power spectral density, the sensitivity curve and the signal-to-noise ratio for LISA (Laser Interferometer Antenna). It is an applicable document for ESA (European Space Agency) and the reference for the LISA Science Requirement Document.
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Cited by 22 Pith papers
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Constraining Dipole Radiation with Multiband Gravitational Waves from Eccentric Binary Black Holes
Multiband observations of eccentric binary black holes can constrain dipole-radiation deviations from general relativity to |b| ≲ 10^{-7} for a GW231123-like event when combining one year of space-based data with grou...
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Gravitational lensing of gravitational waves: universal characteristics of strongly lensed memory waveforms
Strongly lensed gravitational-wave memory waveforms acquire universal parity signatures—odd for type I/III images, even for type II—that can identify image type via a simple step-function approximation.
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Identifying Monochromatic Signals in LISA and Taiji via Spectral Split: Gravitational Waves versus Ultralight Dark Matter
Orbital motion of a space GW detector creates sideband patterns that differ between gravitational waves and ultralight dark matter, enabling discrimination by counting harmonics.
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Distinguishing Monochromatic Signals in LISA and Taiji: Ultralight Dark Matter versus Gravitational Waves
Null-response interferometric channels can separate monochromatic ultralight dark matter signals from gravitational waves in LISA and Taiji, most effectively at high frequencies.
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Population synthesis and detection prospects for Galactic long-period transients with LISA
If long-period radio transients are phase-locked white-dwarf binaries, LISA could detect between 0.05% and 6% of the Galactic population, with enough precision on frequency, amplitude, and sky position to guide radio ...
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Impact of eccentricity and higher-modes on neutron star-black hole parameter estimation
Eccentric NSBH signals like GW200105 contain much more information about masses, mass ratio, and effective spin per unit SNR than circular signals, but not about sky position or distance.
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Strong First-Order Electroweak Phase Transitions and Gravitational Waves in the Normal Two-Higgs-Doublet Model: A Comparative Study of the Four Yukawa Types and Thermal Resummation Schemes
In the Normal 2HDM, SFOEWPTs are single-step and alignment-favoring across all four Yukawa types, yet Parwani versus Arnold–Espinosa resummation changes the viable heavy-mass range from ~1.6 TeV to ≲800 GeV and leaves...
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Clock-noise subtraction in geometric time-delay interferometry for space-based gravitational-wave parameter estimation
Generalized clock-noise observables for the four delay/advance link types cancel USO residuals in arbitrary two-path geometric TDI, restoring sensitivity and tightening monochromatic-source parameter constraints.
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Probing Quadratically Coupled Ultralight Dark Matter with the Laser Interferometer Space Antenna
LISA forecasts for quadratically coupled ultralight dark matter show competitive or superior sensitivity to terrestrial and astrophysical probes in selected mass windows, free of screening.
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Systematic biases in parameter estimation on LISA binaries. II. The effect of excluding higher harmonics for spin-aligned, high-mass binaries
Omitting higher-order waveform harmonics can cause severe, spin-dependent parameter biases for massive LISA black-hole binaries, including confident localization in the wrong sky region.
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Reconsidering the consistent use of precessing, higher order multipole models for gravitational wave analyses
A matched-filter SNR threshold on precession and higher-multipole content can select cheaper waveform models per event while keeping inferred black-hole mass and spin populations consistent, cutting analysis cost by t...
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Probing Flavour Deconstruction via Primordial Gravitational Waves
Flavour deconstruction phase transitions can generate detectable gravitational waves, but their spectra typically peak above the millihertz range, making LISA detection possible yet not guaranteed.
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Identifying galactic binary systems of neutron stars and black holes with LISA
LISA could measure individual component masses for about 10% of detected galactic black hole binaries and about 50% of neutron star binaries, enabling classification of the compact objects.
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Purely quadratic non-Gaussianity from tachyonic instability: Primordial black holes and scalar-induced gravitational waves
Purely quadratic non-Gaussianity from tachyonic instability allows narrow curvature spectra to exponentially suppress primordial black hole overproduction via correlation coefficient ρ approaching -1 while retaining s...
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Beyond Gaussian Assumptions: A new robust statistical framework for gravitational-wave data analysis
A heavy-tailed hyperbolic likelihood, applied across the full frequency band, gives gravitational-wave parameter estimates that are as good as standard methods in Gaussian noise and less biased in glitchy or overlappi...
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Bayesian analysis of the complex singlet model with phase transition gravitational waves
Bayesian forecasts for the Taiji detector constrain complex singlet model parameters through electroweak phase transition gravitational wave signals.
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Measuring gravitational wave spectrum from electroweak phase transition and Higgs self-couplings
Using simulated Taiji data, the authors show that a stochastic gravitational-wave signal from an electroweak phase transition in the singlet-extended Standard Model can constrain the Higgs cubic and quartic self-couplings.
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On the use and interpretation of signal-model indistinguishability measures for gravitational-wave astronomy
Using mismatch distances computed at best-fit parameters, per parameter, the paper predicts accurate bias SNRs for aligned-spin binary black hole measurements and derives waveform accuracy requirements for next-genera...
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Multimessenger prospects of quasi-periodic eruptions
Known quasi-periodic eruptions are unlikely to have LISA-detectable gravitational-wave counterparts, so future searches should focus on rare short-period “golden” QPEs.
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Fundamental Noise and Gravitational-Wave Sensitivity of the Laser Interferometer Lunar Antenna (LILA)
The Moon's normal-mode resonances would amplify gravitational-wave signals enough for the proposed LILA interferometer to reach astrophysically useful sensitivity from millihertz to decihertz.
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Gamma-Rays and Gravitational Waves from Inelastic Higgs Portal Dark Matter
An inelastic complex-scalar Higgs portal dark matter model can evade direct detection, explain the Galactic Center gamma-ray excess, and produce a first-order electroweak phase transition with a gravitational wave sig...
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From inflation to hot big bang -- a tutorial on cosmological perturbations
A tutorial deriving cosmological perturbation equations from inflation through reheating, with explicit gauge-invariant computations and Python scripts.
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