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papers.bib
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---
---
@string{aps = {American Physical Society,}}
@article{Wright:2024awr,
bibtex_show={true},
author = "Wright, David and Giblin, John T. and Hazboun, Jeffrey",
title = "{CMB and energy conservation limits on nanohertz gravitational waves}",
eprint = "2409.15572",
archivePrefix = "arXiv",
primaryClass = "gr-qc",
month = "9",
year = "2024",
preview={wright_bounds_24.png},
altmetric={true},
dimensions={true},
selected={true},
abstract={The recent evidence for a stochastic gravitational wave background (GWB) in the nanohertz band, announced by pulsar timing array (PTA) collaborations around the world, has been posited to be sourced by either a population of supermassive black holes binaries or perturbations of spacetime near the inflationary era, generated by a zoo of various new physical phenomena. Gravitational waves (GWs) from these latter models would be explained by extensions to the standard model of cosmology and possibly to the standard model of particle physics. While PTA datasets can be used to characterize the parameter spaces of these models, energy conservation and limits from the cosmic microwave background (CMB) can be used a priori to bound those parameter spaces. Here we demonstrate that taking a simple rule for energy conservation and using CMB bounds on the radiation energy density can set stringent limits on the parameters for these models.},
code={https://github.com/davecwright3/rule-of-thumb}
}
@article{Baier:2024gke,
bibtex_show={true},
author = "Baier, Jeremy G. and Hazboun, Jeffrey S. and Romano, Joseph D.",
title = "{Tuning a PTA in the detection era}",
eprint = "2409.00336",
archivePrefix = "arXiv",
primaryClass = "astro-ph.HE",
month = "8",
year = "2024",
preview={baier_tuning_24.png},
altmetric={true},
dimensions={true},
selected={true},
abstract={As pulsar timing arrays (PTAs) transition into the detection era of the stochastic gravitational wave background (GWB), it is important for PTA collaborations to review, and possibly revise, their observing campaigns. The source of the GWB is unknown, and it may take years to pin down its nature. An astrophysical ensemble of supermassive binary black holes is one very likely source for the GWB. Evidence for such a background should come in the form of detectable anisotropies in the GWB and resolvable binary signals. A ``single source'' would be a boon for gravitational astrophysics, as such a source would emit gravitational waves for millions of years in the PTA frequency band. Earlier studies have shown that the observational strategies for finding single sources are somewhat different than for finding the statistical correlations needed for the detection of a stochastic background. Here we present generic methods for studying the effects of various observational strategies, taking advantage of detector sensitivity curves, i.e., noise-averaged, frequency-domain detection statistics. The statistical basis for these methods is presented along with myriad examples of how to tune a detector towards single, deterministic signals or a stochastic background. The importance of the uncorrelated half of the GWB, i.e. the pulsar-term, will be discussed as one of the most important sources of noise in the observational era of PTAs.},
code={https://github.com/jeremy-baier/pta_tuning}
}
@article{Oliver:2023xan,
author = "Oliver, Daniel J. and Johnson, Aaron D. and Berrier, Joel and Glampedakis, Kostas and Kennefick, Daniel",
title = "{Gravitational wave peeps from EMRIs and their implication for LISA signal confusion noise}",
eprint = "2305.05793",
archivePrefix = "arXiv",
primaryClass = "gr-qc",
doi = "10.1088/1361-6382/ad40f2",
journal = "Class. Quant. Grav.",
volume = "41",
number = "11",
pages = "115004",
month = "5",
year = "2024",
inspirehep_id={2658414},
altmetric={true},
dimensions={true},
preview={oliver_peeps.jpg},
abstract={Scattering events around the center of massive galaxies will occasionally toss a stellar-mass compact object into an orbit around the massive black hole (MBH) at the center, beginning an extreme mass ratio inspiral (EMRI). The early stages of such a highly eccentric orbit are not likely to produce detectable gravitational waves (GWs), as the source will only be in a suitable frequency band briefly when it is close to periapsis during each long-period orbit. This repeated burst of emission, firmly in the millihertz band, is the GW peep. While a single peep is not likely to be detectable, if we consider an ensemble of such subthreshold sources, spread across the Universe, together they may produce an unresolvable background noise that could obscure sources otherwise detectable by the Laser Interferometer Space Antenna. Previous studies of the extreme mass ratio signal confusion background focused either on parabolic orbits near the MBH or events closer to merger. We seek to improve this characterization by implementing numerical kludge waveforms that can calculate highly eccentric orbits with relativistic effects. Our focus is on orbits at the point of capture that are farther away from the MBH. Here we present the waveforms and spectra of peeps generated from recent calculations of EMRIs/extreme mass ratio bursts capture parameters and discuss how these can be used to estimate the signal confusion noise generated by such events. We demonstrate the effects of changing the orbital parameters on the resulting spectra as well as showing direct comparisons to parabolic orbits and why the GW 'peep' needs to be studied further. The results of this study will be expanded upon in a further paper that aims to provide an update on the EMRI signal confusion noise problem.}
}
@article{Agazie:2024kdi,
bibtex_show={true},
author = "Agazie, Gabriella and others",
title = "{The NANOGrav 15 yr Data Set: Running of the Spectral Index}",
eprint = "2408.10166",
archivePrefix = "arXiv",
primaryClass = "astro-ph.HE",
month = "8",
year = "2024",
preview={nanograv-logo.png},
altmetric={true},
dimensions={true}
}
@article{Agazie:2024stg,
bibtex_show={true},
author = "Agazie, Gabriella and others",
title = "{The NANOGrav 15 yr data set: Posterior predictive checks for gravitational-wave detection with pulsar timing arrays}",
eprint = "2407.20510",
archivePrefix = "arXiv",
primaryClass = "astro-ph.HE",
month = "7",
year = "2024",
preview={nanograv-logo.png}
}
@article{Donlon:2024lvd,
bibtex_show={true},
author = "Donlon, Thomas and others",
title = "{The Anomalous Acceleration of PSR J2043+1711: Long-Period Orbital Companion or Stellar Flyby?}",
eprint = "2407.06482",
archivePrefix = "arXiv",
primaryClass = "astro-ph.SR",
month = "7",
year = "2024",
preview={nanograv-logo.png}
}
@article{Larsen:2024vrt,
bibtex_show={true},
author = "Larsen, Bjorn and others",
title = "{The NANOGrav 15 yr Data Set: Chromatic Gaussian Process Noise Models for Six Pulsars}",
eprint = "2405.14941",
archivePrefix = "arXiv",
primaryClass = "astro-ph.HE",
doi = "10.3847/1538-4357/ad5291",
journal = "Astrophys. J.",
volume = "972",
number = "1",
pages = "49",
year = "2024",
preview={nanograv-logo.png},
altmetric={true},
dimensions={true}
}
@article{Agazie:2024jbf,
bibtex_show={true},
author = "Agazie, Gabriella and others",
title = "{The NANOGrav 15 yr Data Set: Looking for Signs of Discreteness in the Gravitational-wave Background}",
eprint = "2404.07020",
archivePrefix = "arXiv",
primaryClass = "astro-ph.HE",
month = "4",
year = "2024",
preview={nanograv-logo.png}
}
@article{NANOGrav:2023ygs,
bibtex_show={true},
author = "Agazie, Gabriella and others",
collaboration = "NANOGrav",
title = "{The NANOGrav 15 yr Data Set: Search for Transverse Polarization Modes in the Gravitational-wave Background}",
eprint = "2310.12138",
archivePrefix = "arXiv",
primaryClass = "gr-qc",
doi = "10.3847/2041-8213/ad2a51",
journal = "Astrophys. J. Lett.",
volume = "964",
number = "1",
pages = "L14",
year = "2024",
preview={nanograv-logo.png},
altmetric={true},
dimensions={true}
}
@article{NANOGrav:2023wsz,
bibtex_show={true},
author = "Agazie, Gabriella and others",
collaboration = "NANOGrav",
title = "{The NANOGrav 12.5 yr Data Set: A Computationally Efficient Eccentric Binary Search Pipeline and Constraints on an Eccentric Supermassive Binary Candidate in 3C 66B}",
eprint = "2309.17438",
archivePrefix = "arXiv",
primaryClass = "astro-ph.HE",
doi = "10.3847/1538-4357/ad1f61",
journal = "Astrophys. J.",
volume = "963",
number = "2",
pages = "144",
year = "2024",
preview={nanograv-logo.png},
altmetric={true},
dimensions={true}
}
@article{Becsy:2023qul,
bibtex_show={true},
author = "B\'ecsy, Bence and others",
title = "{How to Detect an Astrophysical Nanohertz Gravitational Wave Background}",
eprint = "2309.04443",
archivePrefix = "arXiv",
primaryClass = "gr-qc",
doi = "10.3847/1538-4357/ad09e4",
journal = "Astrophys. J.",
volume = "959",
number = "1",
pages = "9",
year = "2023",
preview={nanograv-logo.png},
altmetric={true},
dimensions={true}
}
@article{InternationalPulsarTimingArray:2023mzf,
bibtex_show={true},
author = "Agazie, G. and others",
collaboration = "International Pulsar Timing Array",
title = "{Comparing Recent Pulsar Timing Array Results on the Nanohertz Stochastic Gravitational-wave Background}",
eprint = "2309.00693",
archivePrefix = "arXiv",
primaryClass = "astro-ph.HE",
doi = "10.3847/1538-4357/ad36be",
journal = "Astrophys. J.",
volume = "966",
number = "1",
pages = "105",
year = "2024",
preview={nanograv-logo.png},
altmetric={true},
dimensions={true}
}
@article{NANOGrav:2023vfo,
bibtex_show={true},
author = "Agazie, Gabriella and others",
collaboration = "NANOGrav",
title = "{The NANOGrav 12.5 yr Data Set: Search for Gravitational Wave Memory}",
eprint = "2307.13797",
archivePrefix = "arXiv",
primaryClass = "gr-qc",
doi = "10.3847/1538-4357/ad0726",
journal = "Astrophys. J.",
volume = "963",
number = "1",
pages = "61",
year = "2024",
preview={nanograv-logo.png},
altmetric={true},
dimensions={true}
}
@article{NANOGrav:2023icp,
bibtex_show={true},
author = "Johnson, Aaron D. and others",
collaboration = "NANOGrav",
title = "{NANOGrav 15-year gravitational-wave background methods}",
eprint = "2306.16223",
archivePrefix = "arXiv",
primaryClass = "astro-ph.HE",
doi = "10.1103/PhysRevD.109.103012",
journal = "Phys. Rev. D",
volume = "109",
number = "10",
pages = "103012",
year = "2024",
preview={nanograv-logo.png},
altmetric={true},
dimensions={true}
}
@article{NANOGrav:2023gor,
bibtex_show={true},
author = "Agazie, Gabriella and others",
collaboration = "NANOGrav",
title = "{The NANOGrav 15 yr Data Set: Evidence for a Gravitational-wave Background}",
eprint = "2306.16213",
archivePrefix = "arXiv",
primaryClass = "astro-ph.HE",
doi = "10.3847/2041-8213/acdac6",
journal = "Astrophys. J. Lett.",
volume = "951",
number = "1",
pages = "L8",
year = "2023",
preview={nanograv-logo.png},
altmetric={true},
dimensions={true},
selected={true},
video={https://www.youtube.com/embed/c2EKbvnee3o?si=PcMVjfv16pwAiiWB}
}
@article{NANOGrav:2023hfp,
bibtex_show={true},
author = "Agazie, Gabriella and others",
collaboration = "NANOGrav",
title = "{The NANOGrav 15 yr Data Set: Constraints on Supermassive Black Hole Binaries from the Gravitational-wave Background}",
eprint = "2306.16220",
archivePrefix = "arXiv",
primaryClass = "astro-ph.HE",
doi = "10.3847/2041-8213/ace18b",
journal = "Astrophys. J. Lett.",
volume = "952",
number = "2",
pages = "L37",
year = "2023",
preview={nanograv-logo.png},
altmetric={true},
dimensions={true}
}
@article{NANOGrav:2023ctt,
bibtex_show={true},
author = "Agazie, Gabriella and others",
collaboration = "NANOGrav",
title = "{The NANOGrav 15 yr Data Set: Detector Characterization and Noise Budget}",
eprint = "2306.16218",
archivePrefix = "arXiv",
primaryClass = "astro-ph.HE",
doi = "10.3847/2041-8213/acda88",
journal = "Astrophys. J. Lett.",
volume = "951",
number = "1",
pages = "L10",
year = "2023",
preview={nanograv-logo.png},
altmetric={true},
dimensions={true}
}
@article{NANOGrav:2023pdq,
bibtex_show={true},
author = "Agazie, Gabriella and others",
collaboration = "NANOGrav",
title = "{The NANOGrav 15 yr Data Set: Bayesian Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries}",
eprint = "2306.16222",
archivePrefix = "arXiv",
primaryClass = "astro-ph.HE",
doi = "10.3847/2041-8213/ace18a",
journal = "Astrophys. J. Lett.",
volume = "951",
number = "2",
pages = "L50",
year = "2023",
preview={nanograv-logo.png},
altmetric={true},
dimensions={true}
}
@article{NANOGrav:2023hvm,
bibtex_show={true},
author = "Afzal, Adeela and others",
collaboration = "NANOGrav",
title = "{The NANOGrav 15 yr Data Set: Search for Signals from New Physics}",
eprint = "2306.16219",
archivePrefix = "arXiv",
primaryClass = "astro-ph.HE",
reportNumber = "FERMILAB-PUB-23-589-T",
doi = "10.3847/2041-8213/acdc91",
journal = "Astrophys. J. Lett.",
volume = "951",
number = "1",
pages = "L11",
year = "2023",
note = "[Erratum: Astrophys.J.Lett. 971, L27 (2024), Erratum: Astrophys.J. 971, L27 (2024)]",
preview={nanograv-logo.png},
altmetric={true},
dimensions={true}
}
@article{NANOGrav:2023hde,
bibtex_show={true},
author = "Agazie, Gabriella and others",
collaboration = "NANOGrav",
title = "{The NANOGrav 15 yr Data Set: Observations and Timing of 68 Millisecond Pulsars}",
eprint = "2306.16217",
archivePrefix = "arXiv",
primaryClass = "astro-ph.HE",
doi = "10.3847/2041-8213/acda9a",
journal = "Astrophys. J. Lett.",
volume = "951",
number = "1",
pages = "L9",
year = "2023",
preview={nanograv-logo.png},
altmetric={true},
dimensions={true}
}
@article{NANOGrav:2023tcn,
bibtex_show={true},
author = "Agazie, Gabriella and others",
collaboration = "NANOGrav",
title = "{The NANOGrav 15 yr Data Set: Search for Anisotropy in the Gravitational-wave Background}",
eprint = "2306.16221",
archivePrefix = "arXiv",
primaryClass = "astro-ph.HE",
doi = "10.3847/2041-8213/acf4fd",
journal = "Astrophys. J. Lett.",
volume = "956",
number = "1",
pages = "L3",
year = "2023",
preview={nanograv-logo.png},
altmetric={true},
dimensions={true}
}
@article{Hazboun:2023tiq,
bibtex_show={true},
author = "Hazboun, Jeffrey S. and Meyers, Patrick M. and Romano, Joseph D. and Siemens, Xavier and Archibald, Anne M.",
title = "{Analytic distribution of the optimal cross-correlation statistic for stochastic gravitational-wave-background searches using pulsar timing arrays}",
eprint = "2305.01116",
archivePrefix = "arXiv",
primaryClass = "gr-qc",
doi = "10.1103/PhysRevD.108.104050",
journal = "Phys. Rev. D",
volume = "108",
number = "10",
pages = "104050",
year = "2023",
altmetric={true},
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