Anna Heffernan

ORCID: 0000-0003-3355-9671
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About
Contact & Profiles
Research Areas
  • Pulsars and Gravitational Waves Research
  • Gamma-ray bursts and supernovae
  • Geophysics and Gravity Measurements
  • Astrophysical Phenomena and Observations
  • Geophysics and Sensor Technology
  • High-pressure geophysics and materials
  • Cosmology and Gravitation Theories
  • COVID-19 Pandemic Impacts
  • COVID-19 epidemiological studies
  • History and Developments in Astronomy
  • Radio Astronomy Observations and Technology
  • Particle Accelerators and Free-Electron Lasers
  • Astronomy and Astrophysical Research
  • Dark Matter and Cosmic Phenomena
  • Relativity and Gravitational Theory
  • Atomic and Subatomic Physics Research
  • Space Satellite Systems and Control
  • COVID-19 Clinical Research Studies
  • earthquake and tectonic studies
  • Cognitive Abilities and Testing
  • Astro and Planetary Science
  • Structural Health Monitoring Techniques
  • COVID-19 diagnosis using AI
  • Superconducting Materials and Applications
  • Acoustic Wave Phenomena Research

Universitat de les Illes Balears
2022-2025

Fundació Universitat-Empresa de les Illes Balears
2024

Laboratoire AstroParticule et Cosmologie
2024

Perimeter Institute
2021-2023

University of Guelph
2020-2022

University of Florida
2018-2022

University College Dublin
2012-2022

Florida Museum of Natural History
2018-2022

European Space Research and Technology Centre
2014-2018

Tulane University
1983

The self-field of a charged particle has singular component which diverges at the particle. We use both coordinate and covariant approaches to compute an expansion this field for particles in generic geodesic orbits about Schwarzschild black hole scalar, electromagnetic gravitational cases. check that yield identical results give, as application, calculation previously unknown mode-sum regularization parameters. In so-called approach self-force calculations, each mode retarded is finite,...

10.1103/physrevd.86.104023 article EN Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology 2012-11-07

The inspiral of a stellar-mass compact object into massive ($\sim 10^{4}$-$10^{7} M_{\odot}$) black hole produces an intricate gravitational-wave signal. Due to the extreme-mass ratios involved, these systems complete $\sim 10^{4}$-$10^{5}$ orbits, most them in strong-field region hole, emitting frequency range $\sim10^{-4}-1~$Hz. This makes prime sources for space-based observatory LISA (Laser Interferometer Space Antenna). observations will enable high-precision measurements physical...

10.48550/arxiv.1903.03686 preprint EN other-oa arXiv (Cornell University) 2019-01-01
LISA Consortium Waveform Working Group Niayesh Afshordi Sarp Akçay Pau Amaro‐Seoane Andrea Antonelli and 95 more Josu C. Aurrekoetxea Leor Barack Enrico Barausse Robert Benkel Laura Bernard Sebastiano Bernuzzi Emanuele Berti Matteo Bonetti Béatrice Bonga Gabriele Bozzola Richard Brito Alessandra Buonanno Alejandro Cárdenas-Avendaño Marc Casals David Chernoff Alvin J. K. Chua Katy Clough M. Colleoni Mekhi Dhesi Adrien Druart Leanne Durkan Guillaume Faye D. L. Ferguson Scott E. Field W. Gabella J. García-Bellido Miguel Gracia-Linares Davide Gerosa Stephen Green M. Haney Mark Hannam Anna Heffernan Tanja Hinderer Thomas Helfer Scott A. Hughes S. Husa Soichiro Isoyama Michael L. Katz Chris Kavanagh Gaurav Khanna Larry Kidder Valeriya Korol Lorenzo Küchler Pablo Laguna François Larrouturou Alexandre Le Tiec Benjamin Leather Eugene A. Lim Hyun Lim T. B. Littenberg Oliver Long Carlos O. Lousto Geoffrey Lovelace Georgios Lukes-Gerakopoulos Philip Lynch Rodrigo Panosso Macedo C. Markakis Elisa Maggio Ilya Mandel Andrea Maselli Josh Mathews Pierre Mourier David Neilsen Alessandro Nagar David A. Nichols Jan Novák Maria Okounkova R. O’Shaughnessy Naritaka Oshita Conor O’Toole Zhen Pan Paolo Pani George Pappas Vasileios Paschalidis Harald Pfeiffer Lorenzo Pompili Adam Pound G. Pratten Hannes R. Rüter Milton Ruiz Zeyd Sam Laura Sberna Stuart L. Shapiro Deirdre Shoemaker Carlos F. Sopuerta Andrew Spiers Hari Sundar Nicola Tamanini Jonathan E. Thompson Alexandre Toubiana Antonios Tsokaros Samuel D. Upton Maarten van de Meent Daniele Vernieri Jeremy M. Wachter

LISA, the Laser Interferometer Space Antenna, will usher in a new era gravitational-wave astronomy. As first anticipated space-based detector, it expand our view to millihertz sky, where spectacular variety of interesting sources abound: from millions ultra-compact binaries Galaxy, mergers massive black holes at cosmological distances; beginnings inspirals that venture into ground-based detectors' death spiral compact objects holes, and many between. Central realising LISA's discovery...

10.48550/arxiv.2311.01300 preprint EN cc-by arXiv (Cornell University) 2023-01-01

Abstract On the 29th of May 2023, LIGO–Virgo–KAGRA Collaboration observed a compact binary coalescence event consistent with neutron star – black hole merger, though heavier object mass 2.5 − 4.5 M⊙ would fall into purported lower gap. An alternative explanation for apparent observations events in this range has been suggested as strongly gravitationally lensed stars. In scenario, magnification lead to source appearing closer and than it really is. Here, we investigate chances possible...

10.1093/mnras/staf049 article EN cc-by Monthly Notices of the Royal Astronomical Society 2025-01-11

In a previous paper, we computed expressions for the Detweiler-Whiting singular field of point scalar, electromagnetic and gravitational charges following geodesic Schwarzschild spacetime. We now extend this to case equatorial orbits in Kerr spacetime, using coordinate covariant approaches compute expansions cases. As an application, give calculation previously unknown mode-sum regularization parameters. also propose new application high-order approximations field, showing how they may be...

10.1103/physrevd.89.024030 article EN Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology 2014-01-22

On 19th March, the World Health Organisation declared a pandemic. Through this global spread, many nations have witnessed exponential growth of confirmed cases brought under control by severe mass quarantine or lockdown measures. However, some have, through different timeline actions, prevented growth. Currently as continue to tackle growth, others attempt safely lift restrictions whilst avoiding resurgence. This study seeks quantify impact government actions in mitigating viral transmission...

10.1109/tetci.2020.3046012 article EN IEEE Transactions on Emerging Topics in Computational Intelligence 2021-01-21

WAIS Digit Span scores of 50 subjects were evaluated to determine the relationship Digits Forward and Backward intellectual functioning in an intellectually subnormal population. The fell into one five levels intelligence, 50—59, 60—69, 70—79, 80—89, 90—99, based upon Full Scale IQ. IQs are significantly more highly correlated all three than Forward. Only (combined forward backward) discriminated across intelligence.

10.2466/pms.1983.56.1.335 article EN Perceptual and Motor Skills 1983-02-01

We provide expansions of the Detweiler–Whiting singular field for a particle with scalar moving along arbitrary, planar accelerated trajectories in Schwarzschild spacetime. transcribe these results into mode-sum regularization parameters, computing previously unknown terms that increase convergence rate mode-sum. test our by self-force variety trajectories. For non-uniformly circular orbits we present from new 1+1D discontinuous Galerkin time-domain code which employs an effective source....

10.1088/1361-6382/aad420 article EN Classical and Quantum Gravity 2018-07-19

The growing reality of gravitational wave astronomy is giving age-old problems a new lease life; one such problem that the self-force. A charged or massive particle moving in curved background space-time produces field affects its motion, pushing it off expected geodesic. This self-field gives rise to so-called self-force acting on particle. In modelling this approach uses perturbative expansion mass ratio. One most interesting sources waves are extreme ratio inspirals - systems perfectly...

10.48550/arxiv.1403.6177 preprint EN other-oa arXiv (Cornell University) 2014-01-01

A scalar charged particle moving in a curved background spacetime will emit field affecting its own motion; the resolving of this resulting motion is often referred to as self-force problem. This also serves toy model for astrophysically interesting compact body binaries, extreme mass ratio inspirals, targets future space-based gravitational wave detector, LISA. In modelling such systems, point-particle assumption leads problematic singularities which need be safely removed solve regardless...

10.1103/physrevd.106.064031 article EN Physical review. D/Physical review. D. 2022-09-15

On 29 May 2023, the LIGO Livingston observatory detected gravitational-wave signal GW230529_181500 from merger of a neutron star with lower mass-gap compact object. Its long inspiral provides unique opportunity to test General Relativity (GR) in parameter space previously unexplored by strong-field tests. In this work, we performed parameterized tests GR GW230529_181500. Specifically, search for deviations frequency-domain GW phase allowing agnostic corrections post-Newtonian coefficients....

10.48550/arxiv.2406.03568 preprint EN arXiv (Cornell University) 2024-06-05

On the 29th of May 2023, LIGO-Virgo-KAGRA Collaboration observed a compact binary coalescence event consistent with neutron star-black hole merger, though heavier object mass 2.5-4.5 $M_\odot$ would fall into purported lower gap. An alternative explanation for apparent observations events in this range has been suggested as strongly gravitationally lensed stars. In scenario, magnification lead to source appearing closer and than it really is. Here, we investigate chances possible...

10.48550/arxiv.2409.07298 preprint EN arXiv (Cornell University) 2024-09-11

The self-force is the leading method in modelling waveforms for extreme mass ratio inspirals, a key target of ESA's future space-based gravitational wave detector LISA. In these systems, one approximates smaller body as point particle to problematic singularities that need be removed. Modelling this singular structure has settled on Detweiler-Whiting field gold standard. As solution governing equation itself, removal, it leaves smooth regular homogeneous equation, much like its well...

10.48550/arxiv.2209.05450 preprint EN other-oa arXiv (Cornell University) 2022-01-01

We consider the interplanetary trajectory design problem posed by 8th edition of Global Trajectory Optimization Competition and present end-to-end strategy developed team ACT-ISAS (a collaboration between European Space Agency's Advanced Concepts Team JAXA's Institute Astronautical Science). The resulting won 1st place in competition, achieving a final mission value $J=146.33$ [Mkm]. Several new algorithms were this context but have an interest that go beyond particular considered, thus,...

10.48550/arxiv.1602.00849 preprint EN other-oa arXiv (Cornell University) 2016-01-01

On 19th March, the World Health Organisation declared a pandemic. Through this global spread, many nations have witnessed exponential growth of confirmed cases brought under control by severe mass quarantine or lockdown measures. However, some have, through different timeline actions, prevented growth. Currently as continue to tackle growth, others attempt safely lift restrictions whilst avoiding resurgence. This study seeks quantify impact government actions in mitigating viral transmission...

10.48550/arxiv.2006.08867 preprint EN other-oa arXiv (Cornell University) 2020-01-01
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