A Double-Pulsar System - A Rare Laboratory for Relativistic Gravity and Plasma Physics
arXiv:astro-ph/0401086 · doi:10.1126/science.1094645
Abstract
The clock-like properties of pulsars moving in the gravitational fields of their unseen neutron-star companions have allowed unique tests of general relativity and provided evidence for gravitational radiation. We report here the detection of the 2.8-sec pulsar J0737-3039B as the companion to the 23-ms pulsar J0737-3039A in a highly-relativistic double-neutron-star system, allowing unprecedented tests of fundamental gravitational physics. We observe a short eclipse of J0737-3039A by J0737-3039B and orbital modulation of the flux density and pulse shape of J0737-3039B, probably due to the influence of J0737-3039A's energy flux upon its magnetosphere. These effects will allow us to probe magneto-ionic properties of a pulsar magnetosphere.
21 pages, 5 figures, Science, in press
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- Orbital variation of the X-ray emission from the double neutron star binary J1537+1155
- Why the mean anomaly at epoch is not used in tests of non-Newtonian gravity?
- Infrared observations of the candidate double neutron star system PSR J1811-1736
- Applicability of Relativistic Point-Coupling Models to Neutron Star Physics
- Dense matter equation of state and neutron star properties from nuclear theory and experiment
- Classical and general relativistic post-Keplerian effects in binary pulsars hosting fast rotating main sequence stars
- Constraining the optical emission from the double pulsar system J0737-3039
- Measuring the De Sitter precession with a new Earth's satellite to the level: a proposal
- On the Unpulsed Radio Emission from J0737-3039
- Quark matter and the astrophysics of neutron stars
- The Effects of Finite Emission Height in Precision Pulsar Timing
- Long Term Study of the Double Pulsar J0737-3039 with XMM-Newton: pulsar timing
- Are the infrared-faint radio sources pulsars?
- The impact of the spin-orbit misalignment and of the spin of B on the Lense-Thrirring orbital precessions of the Double Pulsar PSR J0737-3039A/B
- Black Hole and Neutron Star Binaries: Theoretical Challenges
- On Some Critical Issues of the LAGEOS-Based Tests of the Lense-Thirring Effect
- Tests of Classical Gravity with Radio Pulsars
- Might the 2PN perihelion precession of Mercury become measurable in the next future?
- Members of the double pulsar system PSR J0737-3039 : neutron stars or strange stars ?
- Enhanced particle acceleration in a pulsar wind interacting with a companion
- Long Journey toward the Detection of Gravitational Waves and New Era of Gravitational Wave Astrophysics
- Are we close to put the anomalous perihelion precessions from Verlinde's emergent gravity to the test?
- The hunt for new pulsars with the Green Bank Telescope
- Orbital effects due to gravitational induction
- Theoretical constraints on properties of low-mass neutron stars from EOS of inner crust matters
- The fan beam model for the pulse evolution of PSR J0737-3039B
- Long-term study of the Double Pulsar J0737-3039 with XMM-Newton: spectral analysis
- Quantum Uncertainty Considerations for Gravitational Lens Interferometry
- On the 2PN periastron precession of the Double Pulsar PSR J0737-3039A/B
- Ten years of extreme gravity tests of general theory of relativity with gravitational-wave observations
- A deep search for radio pulsations from the 1.3 M compact-object binary companion of young pulsar PSR J1906+0746
- Some comments on the electrodynamics of binary pulsars
- New frontiers in Numerical Relativity
- Minimum Accretion Rate for Millisecond Pulsar Formation in Binary System
- CXOU J121538.2+361921 in the galaxy NGC 4214: a double neutron star in the making?
- Correlations in the properties of static and rapidly rotating compact stars
- Pulsars as Fantastic Objects and Probes
- Exotica in rotating compact stars
- Influence of hyperon-hyperon interaction on the properties of neutron stars
- Bragg diffraction and the Iron crust of cold Neutron Stars
- Tackling artefacts in the timing of relativistic pulsar binaries: towards the SKA
- The High Time Resolution Universe surveys for pulsars and fast transients
- Strong Field of Binary Systems And Its Effects On Pulsar Arrival Times
- Observations of General Relativity at strong and weak limits
- On the Euler-type gravitomagnetic orbital effects in the field of a precessing body
- Direct Detection of Gravity Waves from Neutron Stars
- And Don't Forget The Black Holes
- Hot Neutron and Quark Star Evolution
- Specific Features of Reflection of Radiation of a Compact Source Rotating about its Axis
- Properties of rapidly rotating hot neutron stars within Brueckner theory
- Constraints on the Neutron Star Equation of State from GW170817
- Gravitational Interstellar Scintillation
- Conducting The Deepest All-Sky Pulsar Survey Ever: The All-Sky High Time Resolution Universe Survey
- Seven Pulsars in Binary Systems above the Spin-up Line
- Nethotrons: exploring the possibility of measuring relativistic spin precessions, from Earth's satellites to the Galactic Centre
- The FAST Galactic Plane Pulsar Snapshot Survey. IX. Timing Three Binary Pulsars with Wide Orbits and Low Orbital Eccentricities
- Kinematic Evidence for Open Cluster Origins of Galactic Binary Neutron Stars
- Bare Collapse, Formation of Neutron Star Binaries and Fast Optical Transients
- Probing fundamental physics with pulsars
- Questions on accreting mass and minimum magnetic field of millisecond pulsars
- The Discovery of the Most Accelerated Binary Pulsar