Searching for the nano-Hertz stochastic gravitational wave background with the Chinese Pulsar Timing Array Data Release I
arXiv:2306.16216 · doi:10.1088/1674-4527/acdfa5
Abstract
Observing and timing a group of millisecond pulsars (MSPs) with high rotational stability enables the direct detection of gravitational waves (GWs). The GW signals can be identified from the spatial correlations encoded in the times-of-arrival of widely spaced pulsar-pairs. The Chinese Pulsar Timing Array (CPTA) is a collaboration aiming at the direct GW detection with observations carried out using Chinese radio telescopes. This short article serves as a `table of contents' for a forthcoming series of papers related to the CPTA Data Release 1 (CPTA DR1) which uses observations from the Five-hundred-meter Aperture Spherical radio Telescope (FAST). Here, after summarizing the time span and accuracy of CPTA DR1, we report the key results of our statistical inference finding a correlated signal with amplitude for spectral index in the range of assuming a GW background (GWB) induced quadrupolar correlation. The search for the Hellings-Downs (HD) correlation curve is also presented, where some evidence for the HD correlation has been found that a 4.6- statistical significance is achieved using the discrete frequency method around the frequency of 14 nHz. We expect that the future International Pulsar Timing Array data analysis and the next CPTA data release will be more sensitive to the nHz GWB, which could verify the current results.
18 pages, 6 figures, submitted to "Research in astronomy and astrophysics" 22nd March 2022
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- Supersymmetric hybrid inflation and current-carrying metastable cosmic strings in
- Waveform models for the gravitational-wave memory effect: Extreme mass-ratio limit and final memory offset
- Anisotropy of Nanohertz Gravitational Wave Background and Source Clustering from Supermassive Binary Black Holes Based on Cosmological Simulation
- Constraints on the Sharpness of the Curvature Power Spectrum
- Connecting Inflation to the NANOGrav 15-year Data Set via Massive Gravity
- Detecting gravitational waves with light
- Reconstructing inflationary potential from NANOGrav 15-year Data: A robust study using Non-Bunch Davies initial condition
- Exploring the Orbital Alignments of Galactic Close White Dwarf Binaries with LISA
- The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
- Probing the mass relation between supermassive black holes and dark matter halos at high redshifts by gravitational wave experiments
- Primary gravitational waves at high frequencies I: Origin of suppression in the power spectrum
- Enhancement of small-scale induced gravitational waves from the soliton/oscillon domination
- Tensor bispectrum mediated by an excited scalar field during inflation
- Effects of Coronal Mass Ejection on PSR J1022+1001 and Possible Mode Change of PSR J2145-0750 in the InPTA DR2
- A narrow-band parameterization for the stochastic gravitational wave background
- Constraints on ultra-slow-roll inflation with the NANOGrav 15-Year Dataset
- Confronting primordial black holes with LIGO-Virgo-KAGRA and the Einstein Telescope
- Testing quantum gravity with primordial gravitational waves
- Lensing point-spread function of coherent astrophysical sources and non-trivial wave effects
- Efficient prescription to search for linear gravitational wave memory from hyperbolic black hole encounters and its application to the NANOGrav 12.5-year dataset
- In Search of the Biggest Bangs since the Big Bang
- Hybrid inflation and gravitational waves from accidentally light scalars
- Is PSR J05144002E in a PBH-NS binary?
- Search for the non-linearities of gravitational wave background in NANOGrav 15-year data set
- Bubbles kick off primordial black holes to form more binaries
- Cosmological scaling of precursor domain walls
- Multi-messenger Astronomy with Quenched Superradiance
- Hemisphere-averaged Hellings-Downs curve between pulsar pairs for a gravitational wave source
- Accurate pulsar timing array residual variances and correlation of the stochastic gravitational wave background
- Signal-to-noise Ratio Analytic Formulae of the Inspiral Binary Black Holes in TianQin
- Analysis of the Gravitational Wave Background Using Gamma-Ray Pulsar Timing Arrays with Next-Generation Detectors
- Scalar-induced gravitational wave from domain wall perturbation
- Exploring the anisotropic gravitational wave background from all-sky mock gravitational wave event catalogues
- Rapid inference for individual binaries and a stochastic background with pulsar timing array data
- Gravitational wave and dark matter from Axion-Higgs string
- Theoretical Radio Signals from Radio-Band Gravitational Waves Converted from the Neutron Star Magnetic Field
- Fundamental quantum limits for detecting ultrahigh frequency gravitational waves
- Improving DM estimates using low-frequency scattering-broadening estimates
- Non-Gaussianity of Tensor Induced Density Perturbations
- Can a time evolving, asymmetric broad line region mimic a massive black hole binary?
- Probing supermassive black hole scalarization with Pulsar Timing Arrays
- Implications of pulsar timing arrays for Gauss-Bonnet Inflation
- Lorentz Violation with Gravitational Waves: Constraints from NANOGrav and IPTA Data
- Magnetogenesis from Sawtooth Coupling: Gravitational Wave Probe of Reheating
- Black holes as telescopes: Discovering supermassive binaries through quasi-periodic lensed starlight
- Self-Interacting Dark-Matter Spikes and the Final-Parsec Problem: Bayesian constraints from the NANOGrav 15-Year Gravitational-Wave Background
- Signature of polarized ultralight vector dark matter in pulsar timing arrays
- Scalar-induced gravitational waves in spatially covariant gravity
- Gravitational waves from axion inflation in the gradient expansion formalism. Part II. Fermionic axion inflation
- Scalar-induced gravitational waves including isocurvature perturbations with lattice simulations
- Finite Populations & Finite Time: The Non-Gaussianity of a Gravitational Wave Background
- The Indian Pulsar Timing Array Data Release 2: II. Customised Single-Pulsar Noise Analysis and Noise Budget
- Perturbative limits on axion-SU(2) gauge dynamics during inflation from the energy density of spin-2 particles
- How large are curvature perturbations from slow first-order phase transitions? A gauge-invariant analysis
- An updated constraint for the Gravitational Wave Background from the Gamma-ray Pulsar Timing Array
- Searching for continuous gravitational waves in the Parkes Pulsar Timing Array Data Release 3
- Detecting milli-Hz gravitational waves with optical resonators
- Searching for supermassive black holes binaries within SRG/eROSITA-De I: Properties of the X-ray selected candidates
- Long-term Timing Results of Ecliptic Pulsars Observed with I-LOFAR
- Insights into Supermassive Black Hole Mergers from the Gravitational Wave Background
- Identifying the Quadrupolar Nature of Gravitational Wave Background through Space-based Missions
- LISA and -ray telescopes as multi-messenger probes of a first-order cosmological phase transition
- Reheating after the Supercooled Phase Transitions with Radiative Symmetry Breaking
- From Symmetry Breaking to Majoron Cosmology: Insights from NANOGrav 15-year Data
- Prospects for joint multiband detection of intermediate-mass black holes by LGWA and the Einstein Telescope
- General Fourier expansion of post-Newtonian binary dynamics based on a quasi-Keplerian framework
- Collapsing domain walls with -violating coupling to thermalized fermions and their impact on gravitational wave detections
- Modeling the Beam of Gravitational Radiation from a Cosmic String Loop
- Estimating the gravitational wave background anisotropy: a Bayesian approach boosted by cross-correlation angular power spectrum
- Supermassive black hole formation in the initial collapse of axion dark matter
- Comprehensive analysis of dissipative effects in the induced gravitational waves
- Inflationary gravitational wave background as a tail effect
- Quantum sensing of high-frequency gravitational waves with ion crystals
- Observable Gravitational Wave Strain at Second Order
- Black hole merger rates for LISA and LGWA from semi-analytical modelling of light seeds
- Gravitational waves from dark domain walls
- High-Redshift Merger Model for Low-Frequency Gravitational Wave Background
- Spontaneous baryogenesis and generation of gravitational waves in a new model of quintessential -attractor
- Stochastic gravitational wave background anisotropies from inflation with non-Bunch-Davies states
- Searching for unresolved massive black hole pairs through AGN photometric variability
- Gravitational Lensing of Gravitational Waves from Astrophysical Sources: Theory, Detection, and Applications
- The NANOGrav 15 yr Data Set: Customized Chromatic Noise Models
- Multiwavelength identification of millisecond pulsar candidates in the Galactic bulge
- Eikonal gravitational-wave lensing in Einstein-aether theory
- Primordial Black Holes from Spatially Varying Cosmological Constant Induced by Field Fluctuations in Extra Dimensions
- Postsphaleron darkogenesis
- Multi-wavelength properties of LISA detectable events
- SageNet: Fast Neural Network Emulation of the Stiff-amplified Gravitational Waves from Inflation
- First Light And Reionization Epoch Simulations (FLARES) -- XIX: Supermassive black hole mergers in the early Universe and their environmental dependence
- Supercooled Audible Axions
- The impact of outliers on pulsar timing arrays
- Detectability of massive binary black holes with sub-mHz gravitational wave missions
- On the calculation of p-values for quadratic statistics in Pulsar Timing Arrays
- Cylindrical Gravitational Waves in Einstein-Aether Theory
- Gravitational Waves and Primordial Black Holes produced by Dark Meta Stable Vacuum Decay
- Upper limits on microhertz gravitational waves from supermassive black-hole binaries using PSR J1909-3744 data from the second IPTA data release
- The Dark Side of the Moon: Listening to Scalar-Induced Gravitational Waves
- Circularly polarized gravitational waves from parity-violating scalar-tensor theory
- Linear perturbations of an exact gravitational wave in the Bianchi IV universe
- Detection of the stochastic gravitational wave background with the space-borne gravitational-wave detector network
- Scalar-Induced Gravitational Waves in Palatini Gravity
- Gravitational Wave Measurement of the - Intrinsic Scatter at High Redshift
- Secondary gravitational waves against a strong gravitational wave in the Bianchi VI universe
- Extending the micro-Hertz detection horizons via orbital resonance effect for geocentric gravitational wave antennas
- Purely quadratic non-Gaussianity from tachyonic instability: Primordial black holes and scalar-induced gravitational waves
- Hawking area law in quantum gravity
- Pulsar scintillation studies with LOFAR III. Annual variations in PSR~J08147429
- Bayesian leave-one-out cross-validation for astrophysical model comparison using gravitational-wave background data
- Model-agnostic gravitational-wave background characterization algorithm
- Evaluating statistical significance for massive black hole binary mergers with space-based gravitational wave detectors
- Distinguishing gravity theories with networks of space-based gravitational-wave detectors
- Gravitational-wave standard sirens and application in cosmology
- Measuring black hole spin through gravitational lensing of pulsars
- Full analytic expressions of overlap reduction functions for anisotropies of the stochastic gravitational-wave background with pulsar timing arrays
- Repulsive quantum gravitoelectric-gravitomagnetic interaction
- Can we hear beats with pulsar timing arrays?
- Time-dependent deflection reconstruction: new technique to search for gravitational waves with the cosmic microwave background
- Spin and flavor oscillations of neutrinos in gravitational fields
- A Population Study for Searching Supermassive Binary Black Holes in Active Galactic Nuclei: Continuum Spectral Features and Periodic Variabilities
- Stochastic gravitational wave background due to core collapse resulting in neutron stars
- Flattened bispectrum of the scalar-induced gravitational waves
- Measuring the crust-superfluid coupling time-scale for 105 UTMOST pulsars with a Kalman filter
- Charged spherically symmetric black holes in the Lyra geometry and a preliminary investigation on the overcharging process
- Pulsar timing array analysis in a Legendre polynomial basis
- Assessing the performance of future space-based detectors: Astrophysical foregrounds and individual sources
- Gravitational lensing of gravitational waves: universal characteristics of strongly lensed memory waveforms
- Bispectrum of induced gravitational waves in the poltergeist mechanism
- Superconducting Strings in
- Searching Stochastic Gravitational Wave Background Landscape Across Frequency Bands
- Measuring the speed of scalar induced gravitational waves from observations
- Novel Solar System Probes for Primordial Black Holes
- Testing No slip model with pulsar timing arrays: NANOGrav and IPTA
- Gravitational Wave Mountains: current-carrying domain walls
- Spatial Correlation between Pulsars from Interfering Gravitational-Wave Sources in Massive Gravity
- Applicability of multi-component study on Bayesian searches for targeted anisotropic stochastic gravitational-wave background
- A simple example of "non-minimal" Pre-Big Bang scenario
- Pulsars identified in the LOFAR Two-metre Sky Survey at 144 MHz
- Initial acquisition requirements for optical cavities in the space gravitational wave antennae DECIGO and B-DECIGO
- Rapid sinking and efficient mergers of supermassive black holes in compact high-redshift galaxies
- Ultralight scalar dark matter versus nonadiabatic perfect fluid dark matter in pulsar timing