publications | Hazgrav

2024

CMB and energy conservation limits on nanohertz gravitational waves

David Wright, John T. Giblin, and Jeffrey Hazboun

Sep 2024

Abs arXiv Bib Code

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.
@article{Wright:2024awr, 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 = sep, year = {2024}, dimensions = {true}, }
Tuning a PTA in the detection era

Jeremy G. Baier, Jeffrey S. Hazboun, and Joseph D. Romano

Aug 2024

Abs arXiv Bib Code

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.
@article{Baier:2024gke, 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 = aug, year = {2024}, dimensions = {true}, }
Gravitational wave peeps from EMRIs and their implication for LISA signal confusion noise

Daniel J. Oliver, Aaron D. Johnson, Joel Berrier, and 2 more authors

Class. Quant. Grav., May 2024

Abs arXiv

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.

The NANOGrav 15 yr Data Set: Running of the Spectral Index

Gabriella Agazie, and others

Aug 2024

@article{Agazie:2024kdi,
  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 = aug,
  year = {2024},
  dimensions = {true}
}

The NANOGrav 15 yr data set: Posterior predictive checks for gravitational-wave detection with pulsar timing arrays

Gabriella Agazie, and others

Jul 2024

arXiv Bib

@article{Agazie:2024stg,
  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 = jul,
  year = {2024},
}

The Anomalous Acceleration of PSR J2043+1711: Long-Period Orbital Companion or Stellar Flyby?

Thomas Donlon, and others

Jul 2024

arXiv Bib

@article{Donlon:2024lvd,
  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 = jul,
  year = {2024},
}

The NANOGrav 15 yr Data Set: Chromatic Gaussian Process Noise Models for Six Pulsars

Bjorn Larsen, and others

Astrophys. J., Jul 2024

arXiv Bib

@article{Larsen:2024vrt,
  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},
  dimensions = {true}
}

The NANOGrav 15 yr Data Set: Looking for Signs of Discreteness in the Gravitational-wave Background

Gabriella Agazie, and others

Apr 2024

arXiv Bib

@article{Agazie:2024jbf,
  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 = apr,
  year = {2024},
}

The NANOGrav 15 yr Data Set: Search for Transverse Polarization Modes in the Gravitational-wave Background

Gabriella Agazie, and others

Astrophys. J. Lett., Apr 2024

arXiv Bib

@article{NANOGrav:2023ygs,
  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},
  dimensions = {true}
}

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

Gabriella Agazie, and others

Astrophys. J., Apr 2024

arXiv Bib

@article{NANOGrav:2023wsz,
  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},
  dimensions = {true}
}

Comparing Recent Pulsar Timing Array Results on the Nanohertz Stochastic Gravitational-wave Background

G. Agazie, and others

Astrophys. J., Apr 2024

arXiv Bib

@article{InternationalPulsarTimingArray:2023mzf,
  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},
  dimensions = {true}
}

The NANOGrav 12.5 yr Data Set: Search for Gravitational Wave Memory

Gabriella Agazie, and others

Astrophys. J., Apr 2024

arXiv Bib

@article{NANOGrav:2023vfo,
  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},
  dimensions = {true}
}

NANOGrav 15-year gravitational-wave background methods

Aaron D. Johnson, and others

Phys. Rev. D, Apr 2024

arXiv Bib

@article{NANOGrav:2023icp,
  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},
  dimensions = {true}
}

An Unusual Pulse Shape Change Event in PSR J1713+0747 Observed with the Green Bank Telescope and CHIME

Ross J. Jennings, and others

Astrophys. J., Apr 2024

arXiv Bib

@article{Jennings:2022cuj,
  author = {Jennings, Ross J. and others},
  title = {{An Unusual Pulse Shape Change Event in PSR J1713+0747 Observed with the Green Bank Telescope and CHIME}},
  eprint = {2210.12266},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.HE},
  doi = {10.3847/1538-4357/ad2930},
  journal = {Astrophys. J.},
  volume = {964},
  number = {2},
  pages = {179},
  year = {2024},
  dimensions = {true}
}

2023

How to Detect an Astrophysical Nanohertz Gravitational Wave Background

Bence Bécsy, and others

Astrophys. J., Apr 2023

arXiv Bib

@article{Becsy:2023qul,
  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},
  dimensions = {true}
}

The NANOGrav 15 yr Data Set: Evidence for a Gravitational-wave Background

Gabriella Agazie, and others

Astrophys. J. Lett., Apr 2023

arXiv Bib Video

@article{NANOGrav:2023gor,
  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},
  dimensions = {true},
}

The NANOGrav 15 yr Data Set: Constraints on Supermassive Black Hole Binaries from the Gravitational-wave Background

Gabriella Agazie, and others

Astrophys. J. Lett., Apr 2023

arXiv Bib

@article{NANOGrav:2023hfp,
  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},
  dimensions = {true}
}

The NANOGrav 15 yr Data Set: Detector Characterization and Noise Budget

Gabriella Agazie, and others

Astrophys. J. Lett., Apr 2023

arXiv Bib

@article{NANOGrav:2023ctt,
  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},
  dimensions = {true}
}

The NANOGrav 15 yr Data Set: Bayesian Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries

Gabriella Agazie, and others

Astrophys. J. Lett., Apr 2023

arXiv Bib

@article{NANOGrav:2023pdq,
  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},
  dimensions = {true}
}

The NANOGrav 15 yr Data Set: Search for Signals from New Physics

Adeela Afzal, and others

Astrophys. J. Lett., Apr 2023

[Erratum: Astrophys.J.Lett. 971, L27 (2024), Erratum: Astrophys.J. 971, L27 (2024)]

arXiv Bib

@article{NANOGrav:2023hvm,
  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)]},
  dimensions = {true}
}

The NANOGrav 15 yr Data Set: Observations and Timing of 68 Millisecond Pulsars

Gabriella Agazie, and others

Astrophys. J. Lett., Apr 2023

arXiv Bib

@article{NANOGrav:2023hde,
  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},
  dimensions = {true}
}

The NANOGrav 15 yr Data Set: Search for Anisotropy in the Gravitational-wave Background

Gabriella Agazie, and others

Astrophys. J. Lett., Apr 2023

arXiv Bib

@article{NANOGrav:2023tcn,
  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},
  dimensions = {true}
}

Analytic distribution of the optimal cross-correlation statistic for stochastic gravitational-wave-background searches using pulsar timing arrays

Jeffrey S. Hazboun, Patrick M. Meyers, Joseph D. Romano, and 2 more authors

Phys. Rev. D, Apr 2023

arXiv Bib

@article{Hazboun:2023tiq,
  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},
  dimensions = {true}
}

Searching for continuous Gravitational Waves in the second data release of the International Pulsar Timing Array

M. Falxa, and others

Mon. Not. Roy. Astron. Soc., Apr 2023

arXiv Bib

@article{IPTA:2023ero,
  author = {Falxa, M. and others},
  collaboration = {IPTA},
  title = {{Searching for continuous Gravitational Waves in the second data release of the International Pulsar Timing Array}},
  eprint = {2303.10767},
  archiveprefix = {arXiv},
  primaryclass = {gr-qc},
  doi = {10.1093/mnras/stad812},
  journal = {Mon. Not. Roy. Astron. Soc.},
  volume = {521},
  number = {4},
  pages = {5077--5086},
  year = {2023},
  dimensions = {true}
}

The NANOGrav 12.5 yr Data Set: Bayesian Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries

Zaven Arzoumanian, and others

Astrophys. J. Lett., Apr 2023

arXiv Bib

@article{NANOGrav:2023bts,
  author = {Arzoumanian, Zaven and others},
  collaboration = {NANOGrav},
  title = {{The NANOGrav 12.5 yr Data Set: Bayesian Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries}},
  eprint = {2301.03608},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.GA},
  doi = {10.3847/2041-8213/acdbc7},
  journal = {Astrophys. J. Lett.},
  volume = {951},
  number = {2},
  pages = {L28},
  year = {2023},
  dimensions = {true}
}

2022

Disentangling Multiple Stochastic Gravitational Wave Background Sources in PTA Data Sets

Andrew R. Kaiser, Nihan S. Pol, Maura A. McLaughlin, and 7 more authors

Astrophys. J., Apr 2022

arXiv Bib

@article{Kaiser:2022cma,
  author = {Kaiser, Andrew R. and Pol, Nihan S. and McLaughlin, Maura A. and Chen, Siyuan and Hazboun, Jeffrey S. and Kelley, Luke Zoltan and Simon, Joseph and Taylor, Stephen R. and Vigeland, Sarah J. and Witt, Caitlin A.},
  title = {{Disentangling Multiple Stochastic Gravitational Wave Background Sources in PTA Data Sets}},
  eprint = {2208.02307},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.CO},
  doi = {10.3847/1538-4357/ac86cc},
  journal = {Astrophys. J.},
  volume = {938},
  number = {2},
  pages = {115},
  year = {2022},
  dimensions = {true}
}

The International Pulsar Timing Array second data release: Search for an isotropic gravitational wave background

J. Antoniadis, and others

Mon. Not. Roy. Astron. Soc., Apr 2022

arXiv Bib

@article{Antoniadis:2022pcn,
  author = {Antoniadis, J. and others},
  title = {{The International Pulsar Timing Array second data release: Search for an isotropic gravitational wave background}},
  eprint = {2201.03980},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.HE},
  doi = {10.1093/mnras/stab3418},
  journal = {Mon. Not. Roy. Astron. Soc.},
  volume = {510},
  number = {4},
  pages = {4873--4887},
  year = {2022},
  dimensions = {true}
}

A Detection of Red Noise in PSR J1824–2452A and Projections for PSR B1937+21 Using NICER X-Ray Timing Data

Jeffrey S. Hazboun, and others

Astrophys. J., Apr 2022

arXiv Bib

@article{Hazboun:2021two,
  author = {Hazboun, Jeffrey S. and others},
  title = {{A Detection of Red Noise in PSR J1824\textendash{}2452A and Projections for PSR B1937+21 Using NICER X-Ray Timing Data}},
  eprint = {2112.02160},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.HE},
  doi = {10.3847/1538-4357/ac54ae},
  journal = {Astrophys. J.},
  volume = {928},
  number = {1},
  pages = {67},
  year = {2022},
  dimensions = {true}
}

Bayesian Solar Wind Modeling with Pulsar Timing Arrays

Jeffrey S. Hazboun, and others

Astrophys. J., Apr 2022

arXiv Bib

@article{NANOGrav:2021yqt,
  author = {Hazboun, Jeffrey S. and others},
  collaboration = {NANOGrav},
  title = {{Bayesian Solar Wind Modeling with Pulsar Timing Arrays}},
  eprint = {2111.09361},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.SR},
  doi = {10.3847/1538-4357/ac5829},
  journal = {Astrophys. J.},
  volume = {929},
  number = {1},
  pages = {39},
  year = {2022},
  dimensions = {true}
}

2021

The NANOGrav 12.5-year Data Set: Search for Non-Einsteinian Polarization Modes in the Gravitational-wave Background

Zaven Arzoumanian, and others

Astrophys. J. Lett., Apr 2021

arXiv Bib

@article{NANOGrav:2021ini,
  author = {Arzoumanian, Zaven and others},
  collaboration = {NANOGrav},
  title = {{The NANOGrav 12.5-year Data Set: Search for Non-Einsteinian Polarization Modes in the Gravitational-wave Background}},
  eprint = {2109.14706},
  archiveprefix = {arXiv},
  primaryclass = {gr-qc},
  doi = {10.3847/2041-8213/ac401c},
  journal = {Astrophys. J. Lett.},
  volume = {923},
  number = {2},
  pages = {L22},
  year = {2021},
  dimensions = {true}
}

Searching for Gravitational Waves from Cosmological Phase Transitions with the NANOGrav 12.5-Year Dataset

Zaven Arzoumanian, and others

Phys. Rev. Lett., Apr 2021

arXiv Bib

@article{NANOGrav:2021flc,
  author = {Arzoumanian, Zaven and others},
  collaboration = {NANOGrav},
  title = {{Searching for Gravitational Waves from Cosmological Phase Transitions with the NANOGrav 12.5-Year Dataset}},
  eprint = {2104.13930},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.CO},
  doi = {10.1103/PhysRevLett.127.251302},
  journal = {Phys. Rev. Lett.},
  volume = {127},
  number = {25},
  pages = {251302},
  year = {2021},
  dimensions = {true}
}

The Pulsar Signal Simulator: A Python package for simulating radio signal data from pulsars

Jeffrey S. Hazboun, Brent Shapiro-Albert, Paul T. Baker, and 7 more authors

J. Open Source Softw., Apr 2021

Bib

@article{Hazboun:2021ibf,
  author = {Hazboun, Jeffrey S. and Shapiro-Albert, Brent and Baker, Paul T. and Henkel, Amelia M. and Wagner, Cassidy M. and Hesse, Jacob and Brook, Paul R. and Lam, Michael T. and McLaughlin, Maura A. and Garver-Daniels, Nathan},
  title = {{The Pulsar Signal Simulator: A Python package for simulating radio signal data from pulsars}},
  doi = {10.21105/joss.02757},
  journal = {J. Open Source Softw.},
  volume = {6},
  number = {58},
  pages = {2757},
  year = {2021},
  dimensions = {true}
}

The NANOGrav 11 yr Data Set: Limits on Supermassive Black Hole Binaries in Galaxies within 500 Mpc

Zaven Arzoumanian, and others

Astrophys. J., Apr 2021

arXiv Bib

@article{NANOGrav:2021sdv,
  author = {Arzoumanian, Zaven and others},
  collaboration = {NANOGrav},
  title = {{The NANOGrav 11 yr Data Set: Limits on Supermassive Black Hole Binaries in Galaxies within 500 Mpc}},
  eprint = {2101.02716},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.GA},
  doi = {10.3847/1538-4357/abfcd3},
  journal = {Astrophys. J.},
  volume = {914},
  number = {2},
  pages = {121},
  year = {2021},
  dimensions = {true}
}

Common-spectrum process versus cross-correlation for gravitational-wave searches using pulsar timing arrays

Joseph D. Romano, Jeffrey S. Hazboun, Xavier Siemens, and 1 more author

Phys. Rev. D, Apr 2021

arXiv Bib

@article{Romano:2020sxq,
  author = {Romano, Joseph D. and Hazboun, Jeffrey S. and Siemens, Xavier and Archibald, Anne M.},
  title = {{Common-spectrum process versus cross-correlation for gravitational-wave searches using pulsar timing arrays}},
  eprint = {2012.03804},
  archiveprefix = {arXiv},
  primaryclass = {gr-qc},
  doi = {10.1103/PhysRevD.103.063027},
  journal = {Phys. Rev. D},
  volume = {103},
  number = {6},
  pages = {063027},
  year = {2021},
  dimensions = {true}
}

Astrophysics Milestones for Pulsar Timing Array Gravitational-wave Detection

Nihan S. Pol, and others

Astrophys. J. Lett., Apr 2021

arXiv Bib

@article{NANOGrav:2020spf,
  author = {Pol, Nihan S. and others},
  collaboration = {NANOGrav},
  title = {{Astrophysics Milestones for Pulsar Timing Array Gravitational-wave Detection}},
  eprint = {2010.11950},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.HE},
  doi = {10.3847/2041-8213/abf2c9},
  journal = {Astrophys. J. Lett.},
  volume = {911},
  number = {2},
  pages = {L34},
  year = {2021},
  dimensions = {true}
}

A Study in Frequency-Dependent Effects on Precision Pulsar Timing Parameters with the Pulsar Signal Simulator

Brent J. Shapiro-Albert, Jeffrey S. Hazboun, Maura A. McLaughlin, and 1 more author

Astrophys. J., Apr 2021

arXiv Bib

@article{Shapiro-Albert:2020tts,
  author = {Shapiro-Albert, Brent J. and Hazboun, Jeffrey S. and McLaughlin, Maura A. and Lam, Michael T.},
  title = {{A Study in Frequency-Dependent Effects on Precision Pulsar Timing Parameters with the Pulsar Signal Simulator}},
  eprint = {2010.07301},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.HE},
  doi = {10.3847/1538-4357/abdc29},
  journal = {Astrophys. J.},
  volume = {909},
  number = {2},
  pages = {219},
  year = {2021},
  dimensions = {true}
}

Multimessenger Pulsar Timing Array Constraints on Supermassive Black Hole Binaries Traced by Periodic Light Curves

Chengcheng Xin, Chiara M. F. Mingarelli, and Jeffrey S. Hazboun

Astrophys. J., Apr 2021

arXiv Bib

@article{Xin:2020owo,
  author = {Xin, Chengcheng and Mingarelli, Chiara M. F. and Hazboun, Jeffrey S.},
  title = {{Multimessenger Pulsar Timing Array Constraints on Supermassive Black Hole Binaries Traced by Periodic Light Curves}},
  eprint = {2009.11865},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.GA},
  doi = {10.3847/1538-4357/ac01c5},
  journal = {Astrophys. J.},
  volume = {915},
  number = {2},
  pages = {97},
  year = {2021},
  dimensions = {true}
}

Precision Timing of PSR J0437–4715 with the IAR Observatory and Implications for Low-frequency Gravitational Wave Source Sensitivity

M. T. Lam, and J. S. Hazboun

Astrophys. J., Apr 2021

arXiv Bib

@article{Lam:2020niv,
  author = {Lam, M. T. and Hazboun, J. S.},
  title = {{Precision Timing of PSR J0437\textendash{}4715 with the IAR Observatory and Implications for Low-frequency Gravitational Wave Source Sensitivity}},
  eprint = {2007.00260},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.HE},
  doi = {10.3847/1538-4357/abeb64},
  journal = {Astrophys. J.},
  volume = {911},
  number = {2},
  pages = {137},
  year = {2021},
  dimensions = {true}
}

The NANOGrav 12.5 yr Data Set: Wideband Timing of 47 Millisecond Pulsars

Md F. Alam, and others

Astrophys. J. Suppl., Apr 2021

arXiv Bib

@article{NANOGrav:2020qll,
  author = {Alam, Md F. and others},
  collaboration = {NANOGrav},
  title = {{The NANOGrav 12.5 yr Data Set: Wideband Timing of 47 Millisecond Pulsars}},
  eprint = {2005.06495},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.HE},
  doi = {10.3847/1538-4365/abc6a1},
  journal = {Astrophys. J. Suppl.},
  volume = {252},
  number = {1},
  pages = {5},
  year = {2021},
  dimensions = {true}
}

The NANOGrav 12.5 yr Data Set: Observations and Narrowband Timing of 47 Millisecond Pulsars

Md F. Alam, and others

Astrophys. J. Suppl., Apr 2021

arXiv Bib

@article{NANOGrav:2020gpb,
  author = {Alam, Md F. and others},
  collaboration = {NANOGrav},
  title = {{The NANOGrav 12.5 yr Data Set: Observations and Narrowband Timing of 47 Millisecond Pulsars}},
  eprint = {2005.06490},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.HE},
  doi = {10.3847/1538-4365/abc6a0},
  journal = {Astrophys. J. Suppl.},
  volume = {252},
  number = {1},
  pages = {4},
  year = {2021},
  dimensions = {true}
}

2020

Model Dependence of Bayesian Gravitational-Wave Background Statistics for Pulsar Timing Arrays

Jeffrey S. Hazboun, Joseph Simon, Xavier Siemens, and 1 more author

Astrophys. J. Lett., Apr 2020

arXiv Bib

@article{Hazboun:2020kzd,
  author = {Hazboun, Jeffrey S. and Simon, Joseph and Siemens, Xavier and Romano, Joseph D.},
  title = {{Model Dependence of Bayesian Gravitational-Wave Background Statistics for Pulsar Timing Arrays}},
  eprint = {2009.05143},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.IM},
  doi = {10.3847/2041-8213/abca92},
  journal = {Astrophys. J. Lett.},
  volume = {905},
  number = {1},
  pages = {L6},
  year = {2020},
  dimensions = {true}
}

The NANOGrav 12.5 yr Data Set: Search for an Isotropic Stochastic Gravitational-wave Background

Zaven Arzoumanian, and others

Astrophys. J. Lett., Apr 2020

arXiv Bib

@article{NANOGrav:2020bcs,
  author = {Arzoumanian, Zaven and others},
  collaboration = {NANOGrav},
  title = {{The NANOGrav 12.5 yr Data Set: Search for an Isotropic Stochastic Gravitational-wave Background}},
  eprint = {2009.04496},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.HE},
  doi = {10.3847/2041-8213/abd401},
  journal = {Astrophys. J. Lett.},
  volume = {905},
  number = {2},
  pages = {L34},
  year = {2020},
  dimensions = {true}
}

Multimessenger Gravitational-wave Searches with Pulsar Timing Arrays: Application to 3C 66B Using the NANOGrav 11-year Data Set

Zaven Arzoumanian, and others

Astrophys. J., Apr 2020

arXiv Bib

@article{NANOGrav:2020lwu,
  author = {Arzoumanian, Zaven and others},
  collaboration = {NANOGrav},
  title = {{Multimessenger Gravitational-wave Searches with Pulsar Timing Arrays: Application to 3C 66B Using the NANOGrav 11-year Data Set}},
  eprint = {2005.07123},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.GA},
  doi = {10.3847/1538-4357/ababa1},
  journal = {Astrophys. J.},
  volume = {900},
  number = {2},
  pages = {102},
  year = {2020},
  dimensions = {true}
}

Modeling the uncertainties of solar-system ephemerides for robust gravitational-wave searches with pulsar timing arrays

M. Vallisneri, and others

Jan 2020

arXiv Bib

@article{NANOGrav:2020tig,
  author = {Vallisneri, M. and others},
  collaboration = {NANOGrav},
  title = {{Modeling the uncertainties of solar-system ephemerides for robust gravitational-wave searches with pulsar timing arrays}},
  eprint = {2001.00595},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.HE},
  doi = {10.3847/1538-4357/ab7b67},
  month = jan,
  year = {2020},
  dimensions = {true}
}

The NANOGrav 11 yr Data Set: Limits on Gravitational Wave Memory

K. Aggarwal, and others

Astrophys. J., Jan 2020

arXiv Bib

@article{NANOGrav:2019vto,
  author = {Aggarwal, K. and others},
  collaboration = {NANOGrav},
  title = {{The NANOGrav 11 yr Data Set: Limits on Gravitational Wave Memory}},
  eprint = {1911.08488},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.HE},
  doi = {10.3847/1538-4357/ab6083},
  journal = {Astrophys. J.},
  volume = {889},
  pages = {38},
  year = {2020},
  dimensions = {true}
}

2019

Hasasia: A Python package for Pulsar Timing Array Sensitivity Curves

Jeffrey Hazboun, Joseph Romano, and Tristan Smith

J. Open Source Softw., Jan 2019

Bib

@article{Hazboun:2019nqt,
  author = {Hazboun, Jeffrey and Romano, Joseph and Smith, Tristan},
  title = {{Hasasia: A Python package for Pulsar Timing Array Sensitivity Curves}},
  doi = {10.21105/joss.01775},
  journal = {J. Open Source Softw.},
  volume = {4},
  number = {42},
  pages = {1775},
  year = {2019},
  dimensions = {true}
}

The NANOGrav 11-Year Data Set: Evolution of Gravitational Wave Background Statistics

J. S. Hazboun, and others

Sep 2019

arXiv Bib

@article{NANOGrav:2019ydy,
  author = {Hazboun, J. S. and others},
  collaboration = {NANOGrav},
  title = {{The NANOGrav 11-Year Data Set: Evolution of Gravitational Wave Background Statistics}},
  eprint = {1909.08644},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.HE},
  doi = {10.3847/1538-4357/ab68db},
  month = sep,
  year = {2019},
  dimensions = {true}
}

The International Pulsar Timing Array: Second data release

B. B. P. Perera, and others

Mon. Not. Roy. Astron. Soc., Sep 2019

arXiv Bib

@article{Perera:2019sca,
  author = {Perera, B. B. P. and others},
  title = {{The International Pulsar Timing Array: Second data release}},
  eprint = {1909.04534},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.HE},
  doi = {10.1093/mnras/stz2857},
  journal = {Mon. Not. Roy. Astron. Soc.},
  volume = {490},
  number = {4},
  pages = {4666--4687},
  year = {2019},
  dimensions = {true}
}

The NANOGrav Program for Gravitational Waves and Fundamental Physics

A. Brazier, and others

Aug 2019

arXiv Bib

@article{Brazier:2019mmu,
  author = {Brazier, A. and others},
  title = {{The NANOGrav Program for Gravitational Waves and Fundamental Physics}},
  eprint = {1908.05356},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.IM},
  month = aug,
  year = {2019},
}

NANOGrav Education and Outreach: Growing a Diverse and Inclusive Collaboration for Low-Frequency Gravitational Wave Astronomy

P. T. Baker, and others

Jul 2019

arXiv Bib

@article{NANOGrav:2019yfi,
  author = {Baker, P. T. and others},
  collaboration = {NANOGrav},
  title = {{NANOGrav Education and Outreach: Growing a Diverse and Inclusive Collaboration for Low-Frequency Gravitational Wave Astronomy}},
  eprint = {1907.07348},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.IM},
  month = jul,
  year = {2019},
}

Physics Beyond the Standard Model With Pulsar Timing Arrays

Xavier Siemens, Jeffrey S. Hazboun, Paul T. Baker, and 5 more authors

Jul 2019

arXiv Bib

@article{Siemens:2019xkk,
  author = {Siemens, Xavier and Hazboun, Jeffrey S. and Baker, Paul T. and Burke-Spolaor, Sarah and Madison, Dustin and Mingarelli, Chiara and Simon, Joseph and Smith, Tristan},
  title = {{Physics Beyond the Standard Model With Pulsar Timing Arrays}},
  eprint = {1907.04960},
  archiveprefix = {arXiv},
  primaryclass = {gr-qc},
  month = jul,
  year = {2019}
}

Realistic sensitivity curves for pulsar timing arrays

Jeffrey S. Hazboun, Joseph D. Romano, and Tristan L. Smith

Phys. Rev. D, Jul 2019

arXiv Bib

@article{Hazboun:2019vhv,
  author = {Hazboun, Jeffrey S. and Romano, Joseph D. and Smith, Tristan L.},
  title = {{Realistic sensitivity curves for pulsar timing arrays}},
  eprint = {1907.04341},
  archiveprefix = {arXiv},
  primaryclass = {gr-qc},
  doi = {10.1103/PhysRevD.100.104028},
  journal = {Phys. Rev. D},
  volume = {100},
  number = {10},
  pages = {104028},
  year = {2019},
  dimensions = {true}
}

Astro2020 science white paper: The gravitational wave view of massive black holes

Monica Colpi, and others

Mar 2019

arXiv Bib

@article{Colpi:2019yzd,
  author = {Colpi, Monica and others},
  title = {{Astro2020 science white paper: The gravitational wave view of massive black holes}},
  eprint = {1903.06867},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.GA},
  month = mar,
  year = {2019}
}

The NANOGrav 11-Year Data Set: Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries

K. Aggarwal, and others

Astrophys. J., Mar 2019

arXiv Bib

@article{Aggarwal:2018mgp,
  author = {Aggarwal, K. and others},
  title = {{The NANOGrav 11-Year Data Set: Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries}},
  eprint = {1812.11585},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.GA},
  doi = {10.3847/1538-4357/ab2236},
  journal = {Astrophys. J.},
  volume = {880},
  pages = {2},
  year = {2019},
  dimensions = {true}
}

The Astrophysics of Nanohertz Gravitational Waves

Sarah Burke-Spolaor, and others

Astron. Astrophys. Rev., Mar 2019

arXiv Bib

@article{Burke-Spolaor:2018bvk,
  author = {Burke-Spolaor, Sarah and others},
  title = {{The Astrophysics of Nanohertz Gravitational Waves}},
  eprint = {1811.08826},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.HE},
  doi = {10.1007/s00159-019-0115-7},
  journal = {Astron. Astrophys. Rev.},
  volume = {27},
  number = {1},
  pages = {5},
  year = {2019},
  dimensions = {true}
}

2018

The Second International Pulsar Timing Array Mock Data Challenge

Jeffrey S. Hazboun, Chiara M. F. Mingarelli, and Kejia Lee

Oct 2018

arXiv Bib

@article{Hazboun:2018wpv,
  author = {Hazboun, Jeffrey S. and Mingarelli, Chiara M. F. and Lee, Kejia},
  title = {{The Second International Pulsar Timing Array Mock Data Challenge}},
  eprint = {1810.10527},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.IM},
  month = oct,
  year = {2018}
}

An Acoustical Analogue of a Galactic-scale Gravitational-Wave Detector

Michael T. Lam, Joseph D. Romano, Joey S. Key, and 2 more authors

Am. J. Phys., Oct 2018

arXiv Bib

@article{Lam:2018wbx,
  author = {Lam, Michael T. and Romano, Joseph D. and Key, Joey S. and Normandin, Marc and Hazboun, Jeffrey S.},
  title = {{An Acoustical Analogue of a Galactic-scale Gravitational-Wave Detector}},
  eprint = {1803.05285},
  archiveprefix = {arXiv},
  primaryclass = {physics.ed-ph},
  doi = {10.1119/1.5050190},
  journal = {Am. J. Phys.},
  volume = {86},
  number = {10},
  pages = {755},
  year = {2018},
  dimensions = {true}
}

Constructing an explicit AdS/CFT correspondence with Cartan geometry

Jeffrey S. Hazboun

Nucl. Phys. B, Oct 2018

arXiv Bib

@article{Hazboun:2018dbl,
  author = {Hazboun, Jeffrey S.},
  title = {{Constructing an explicit AdS/CFT correspondence with Cartan geometry}},
  eprint = {1802.09561},
  archiveprefix = {arXiv},
  primaryclass = {gr-qc},
  doi = {10.1016/j.nuclphysb.2018.02.006},
  journal = {Nucl. Phys. B},
  volume = {929},
  pages = {254--265},
  year = {2018},
  dimensions = {true}
}

The NANOGrav 11-year Data Set: Pulsar-timing Constraints On The Stochastic Gravitational-wave Background

Z. Arzoumanian, and others

Astrophys. J., Oct 2018

arXiv Bib

@article{NANOGRAV:2018hou,
  author = {Arzoumanian, Z. and others},
  collaboration = {NANOGRAV},
  title = {{The NANOGrav 11-year Data Set: Pulsar-timing Constraints On The Stochastic Gravitational-wave Background}},
  eprint = {1801.02617},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.HE},
  doi = {10.3847/1538-4357/aabd3b},
  journal = {Astrophys. J.},
  volume = {859},
  number = {1},
  pages = {47},
  year = {2018},
  dimensions = {true}
}

A Second Chromatic Timing Event of Interstellar Origin toward PSR J1713+0747

M. T. Lam, and others

Astrophys. J., Oct 2018

arXiv Bib

@article{Lam:2017duo,
  author = {Lam, M. T. and others},
  title = {{A Second Chromatic Timing Event of Interstellar Origin toward PSR J1713+0747}},
  eprint = {1712.03651},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.HE},
  doi = {10.3847/1538-4357/aac770},
  journal = {Astrophys. J.},
  volume = {861},
  number = {2},
  pages = {132},
  year = {2018},
  dimensions = {true}
}

2017

Power radiated by a binary system in a de Sitter Universe

Béatrice Bonga, and Jeffrey S. Hazboun

Phys. Rev. D, Oct 2017

arXiv Bib

@article{Bonga:2017dlx,
  author = {Bonga, B\'eatrice and Hazboun, Jeffrey S.},
  title = {{Power radiated by a binary system in a de Sitter Universe}},
  eprint = {1708.05621},
  archiveprefix = {arXiv},
  primaryclass = {gr-qc},
  doi = {10.1103/PhysRevD.96.064018},
  journal = {Phys. Rev. D},
  volume = {96},
  number = {6},
  pages = {064018},
  year = {2017},
  dimensions = {true}
}

2016

Null-stream pointing with pulsar timing arrays

Jeffrey S. Hazboun, and Shane L. Larson

Jul 2016

arXiv Bib

@article{Hazboun:2016glx,
  author = {Hazboun, Jeffrey S. and Larson, Shane L.},
  title = {{Null-stream pointing with pulsar timing arrays}},
  eprint = {1607.03459},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.IM},
  month = jul,
  year = {2016}
}

2014

C7 multi-messenger astronomy of GW sources

M. Branchesi, and others

Gen. Rel. Grav., Jul 2014

Bib

@article{Branchesi:2014vsa,
  author = {Branchesi, M. and others},
  title = {{C7 multi-messenger astronomy of GW sources}},
  doi = {10.1007/s10714-014-1771-6},
  journal = {Gen. Rel. Grav.},
  volume = {46},
  pages = {1771},
  year = {2014},
  dimensions = {true}
}

Time and dark matter from the conformal symmetries of Euclidean space

Jeffrey S Hazboun, and James T Wheeler

Class. Quant. Grav., Jul 2014

arXiv Bib

@article{Hazboun:2013lra,
  author = {Hazboun, Jeffrey S and Wheeler, James T},
  title = {{Time and dark matter from the conformal symmetries of Euclidean space}},
  eprint = {1305.6972},
  archiveprefix = {arXiv},
  primaryclass = {gr-qc},
  doi = {10.1088/0264-9381/31/21/215001},
  journal = {Class. Quant. Grav.},
  volume = {31},
  number = {21},
  pages = {215001},
  year = {2014},
  dimensions = {true}
}

2013

Limiting alternative theories of gravity using gravitational wave observations across the spectrum

Jeffrey S. Hazboun, Manuel Pichardo Marcano, and Shane L. Larson

Nov 2013

arXiv Bib

@article{Hazboun:2013pea,
  author = {Hazboun, Jeffrey S. and Marcano, Manuel Pichardo and Larson, Shane L.},
  title = {{Limiting alternative theories of gravity using gravitational wave observations across the spectrum}},
  eprint = {1311.3153},
  archiveprefix = {arXiv},
  primaryclass = {gr-qc},
  month = nov,
  year = {2013}
}

2012

A systematic construction of curved phase space: A gravitational gauge theory with symplectic form

Jeffrey S. Hazboun, and James T. Wheeler

J. Phys. Conf. Ser., Nov 2012

Bib

@article{Hazboun:2012zz,
  author = {Hazboun, Jeffrey S. and Wheeler, James T.},
  editor = {Mena Marugan, Guillermo A. and Barbero, J. Fernando G. and Garay, Luis J. and Villasenor, Eduardo J. S. and Olmedo, Javier},
  title = {{A systematic construction of curved phase space: A gravitational gauge theory with symplectic form}},
  doi = {10.1088/1742-6596/360/1/012013},
  journal = {J. Phys. Conf. Ser.},
  volume = {360},
  pages = {012013},
  year = {2012},
  dimensions = {true}
}

2010

The Effect of Negative-Energy Shells on the Schwarzschild Black Hole

Jeffrey S Hazboun, and Tevian Dray

Gen. Rel. Grav., Nov 2010

arXiv Bib

@article{Hazboun:2009zs,
  author = {Hazboun, Jeffrey S and Dray, Tevian},
  title = {{The Effect of Negative-Energy Shells on the Schwarzschild Black Hole}},
  eprint = {0907.0696},
  archiveprefix = {arXiv},
  primaryclass = {gr-qc},
  doi = {10.1007/s10714-009-0916-5},
  journal = {Gen. Rel. Grav.},
  volume = {42},
  pages = {1457--1467},
  year = {2010},
  dimensions = {true}
}

1967

Vision

Letters on wave mechanics

Albert Einstein, Erwin Schrödinger, Max Planck, and 2 more authors

Nov 1967

Bib

@book{przibram1967letters,
  title = {Letters on wave mechanics},
  author = {Einstein, Albert and Schrödinger, Erwin and Planck, Max and Lorentz, Hendrik Antoon and Przibram, Karl},
  year = {1967},
  publisher = {Vision},
}

1956

Investigations on the Theory of the Brownian Movement

Albert Einstein

Nov 1956

Bib

1950

AJP

The meaning of relativity

Albert Einstein, and AH Taub

American Journal of Physics, Nov 1950

Bib

@article{einstein1950meaning,
  title = {The meaning of relativity},
  author = {Einstein, Albert and Taub, AH},
  journal = {American Journal of Physics},
  volume = {18},
  number = {6},
  pages = {403--404},
  year = {1950},
  publisher = {American Association of Physics Teachers}
}

1935

PhysRev
Can Quantum-Mechanical Description of Physical Reality Be Considered Complete?

A. Einstein^*†, B. Podolsky^*, and N. Rosen^*

Phys. Rev., New Jersey. More Information can be found here , May 1935

Abs Bib HTML PDF Video

In a complete theory there is an element corresponding to each element of reality. A sufficient condition for the reality of a physical quantity is the possibility of predicting it with certainty, without disturbing the system. In quantum mechanics in the case of two physical quantities described by non-commuting operators, the knowledge of one precludes the knowledge of the other. Then either (1) the description of reality given by the wave function in quantum mechanics is not complete or (2) these two quantities cannot have simultaneous reality. Consideration of the problem of making predictions concerning a system on the basis of measurements made on another system that had previously interacted with it leads to the result that if (1) is false then (2) is also false. One is thus led to conclude that the description of reality as given by a wave function is not complete.
@article{PhysRev.47.777, title = {Can Quantum-Mechanical Description of Physical Reality Be Considered Complete?}, author = {Einstein, A. and Podolsky, B. and Rosen, N.}, journal = {Phys. Rev.}, location = {New Jersey}, volume = {47}, issue = {10}, pages = {777--780}, numpages = {0}, year = {1935}, month = may, publisher = {American Physical Society,}, doi = {10.1103/PhysRev.47.777}, url = {http://link.aps.org/doi/10.1103/PhysRev.47.777}, dimensions = {true}, }

1920

Relativity: the Special and General Theory

Albert Einstein

May 1920

HTML

1905

Über die von der molekularkinetischen Theorie der Wärme geforderte Bewegung von in ruhenden Flüssigkeiten suspendierten Teilchen

A. Einstein

Annalen der physik, May 1905

Bib

@article{einstein1905molekularkinetischen,
  title = {{\"U}ber die von der molekularkinetischen Theorie der W{\"a}rme geforderte Bewegung von in ruhenden Fl{\"u}ssigkeiten suspendierten Teilchen},
  author = {Einstein, A.},
  journal = {Annalen der physik},
  volume = {322},
  number = {8},
  pages = {549--560},
  year = {1905},
  publisher = {Wiley Online Library}
}

Ann. Phys.

Un the movement of small particles suspended in statiunary liquids required by the molecular-kinetic theory 0f heat

A. Einstein

Ann. Phys., May 1905

Bib

@article{einstein1905movement,
  title = {Un the movement of small particles suspended in statiunary liquids required by the molecular-kinetic theory 0f heat},
  author = {Einstein, A.},
  journal = {Ann. Phys.},
  volume = {17},
  pages = {549--560},
  year = {1905}
}

On the electrodynamics of moving bodies

A. Einstein

May 1905

Bib

Ann. Phys.

Über einen die Erzeugung und Verwandlung des Lichtes betreffenden heuristischen Gesichtspunkt

Albert Einstein

Ann. Phys., May 1905

Nobel Prize Abs Bib

Albert Einstein receveid the Nobel Prize in Physics 1921 for his services to Theoretical Physics, and especially for his discovery of the law of the photoelectric effect

@article{einstein1905photoelectriceffect,
  title = {{{\"U}ber einen die Erzeugung und Verwandlung des Lichtes betreffenden heuristischen Gesichtspunkt}},
  author = {Einstein, Albert},
  journal = {Ann. Phys.},
  volume = {322},
  number = {6},
  pages = {132--148},
  year = {1905},
  doi = {10.1002/andp.19053220607},
}