Norbert Wex
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View article: The double neutron star PSR J1946+2052
The double neutron star PSR J1946+2052 Open
Aims. Double neutron star (DNS) systems are superb laboratories for testing theories of gravity and constraining the equation of state of ultra-dense matter. PSR J1946+2052 is a particularly intriguing DNS system due to its orbital period …
View article: The double neutron star PSR J1946+2052 I. Masses and tests of general relativity
The double neutron star PSR J1946+2052 I. Masses and tests of general relativity Open
We conducted high-precision timing of PSR J1946+2052 to determine the masses of the two neutron stars in the system, test general relativity (GR) and assessed the system's potential for future measurement of the moment of inertia of the pu…
View article: NGC 1851A: Revealing an ongoing three-body encounter in a dense globular cluster
NGC 1851A: Revealing an ongoing three-body encounter in a dense globular cluster Open
PSR J0514−4002A is a binary millisecond pulsar located in the globular cluster NGC 1851. The pulsar has a spin period of 4.99 ms, an orbital period of 18.8 days, and is in a very eccentric ( e = 0.89) orbit around a massive companion. In t…
View article: Demographics of black holes at $<$100 R$_{\rm g}$ scales: accretion flows, jets, and shadows
Demographics of black holes at $<$100 R$_{\rm g}$ scales: accretion flows, jets, and shadows Open
Using the Event Horizon Telescope (EHT), the gravitationally lensed rings around the supermassive black holes (SMBHs) in Messier 87 (M87) and Sagittarius A* (Sgr A*) have now been successfully imaged at a resolution under 10 gravitational …
View article: Explanation of the exceptionally strong timing noise of PSR J0337+1715 by a circum-ternary planet and consequences for gravity tests
Explanation of the exceptionally strong timing noise of PSR J0337+1715 by a circum-ternary planet and consequences for gravity tests Open
Context. Timing of pulsar PSR J0337+1715 provides a unique opportunity to test the strong equivalence principle (SEP) with a strongly self-gravitating object. This is due to its unique situation in a triple stellar system with two white dw…
View article: Explanation of the exceptionally strong timing noise of PSR J0337+1715 by a circum-ternary planet and consequences for gravity tests
Explanation of the exceptionally strong timing noise of PSR J0337+1715 by a circum-ternary planet and consequences for gravity tests Open
Context: Timing of pulsar PSR J0337+1715 provides a unique opportunity to test the strong equivalence principle (SEP) with a strongly self-gravitating object. This is due to its unique situation in a triple stellar system with two white dw…
View article: MeerKAT observations of pair-plasma induced birefringence in the double pulsar eclipses
MeerKAT observations of pair-plasma induced birefringence in the double pulsar eclipses Open
PSR J0737−3039A/B is unique among double neutron star systems. Its near-perfect edge-on orbit causes the fast spinning pulsar A to be eclipsed by the magnetic field of the slow spinning pulsar B. Using high-sensitivity MeerKAT radio observ…
View article: Gravity experiments with radio pulsars
Gravity experiments with radio pulsars Open
The discovery of the first pulsar in a binary star system, the Hulse–Taylor pulsar, 50 years ago opened up an entirely new field of experimental gravity. For the first time it was possible to investigate strong-field and radiative aspects …
View article: A pulsar in a binary with a compact object in the mass gap between neutron stars and black holes
A pulsar in a binary with a compact object in the mass gap between neutron stars and black holes Open
Some compact objects observed in gravitational wave events have masses in the gap between known neutron stars (NSs) and black holes (BHs). The nature of these mass gap objects is unknown, as is the formation of their host binary systems. W…
View article: A MeerKAT view of the double pulsar eclipses
A MeerKAT view of the double pulsar eclipses Open
The double pulsar system, PSR J0737−3039A/B, consists of two neutron stars bound together in a highly relativistic orbit that is viewed nearly edge-on from the Earth. This alignment results in brief radio eclipses of the fast-rotating puls…
View article: A MeerKAT view of the double pulsar eclipses -- Geodetic precession of pulsar B and system geometry
A MeerKAT view of the double pulsar eclipses -- Geodetic precession of pulsar B and system geometry Open
The double pulsar system, PSR J0737$-$3039A/B, consists of two neutron stars bound together in a highly relativistic orbit that is viewed nearly edge-on from the Earth. This alignment results in brief radio eclipses of the fast-rotating pu…
View article: New constraints on the kinematic, relativistic, and evolutionary properties of the PSR J1757−1854 double neutron star system
New constraints on the kinematic, relativistic, and evolutionary properties of the PSR J1757−1854 double neutron star system Open
PSR J1757−1854 is one of the most relativistic double neutron star binary systems known in our Galaxy, with an orbital period of $P_\text{b}=4.4\, \text{h}$ and an orbital eccentricity of e = 0.61. As such, it has promised to be an outstan…
View article: New constraints on the kinematic, relativistic and evolutionary properties of the PSR J1757$-$1854 double neutron star system
New constraints on the kinematic, relativistic and evolutionary properties of the PSR J1757$-$1854 double neutron star system Open
PSR J1757$-$1854 is one of the most relativistic double neutron star binary systems known in our Galaxy, with an orbital period of $P_\text{b}=4.4\,\text{hr}$ and an orbital eccentricity of $e=0.61$. As such, it has promised to be an outst…
View article: A new pulsar timing model for scalar-tensor gravity with applications to PSR J2222-0137 and pulsar-black hole binaries
A new pulsar timing model for scalar-tensor gravity with applications to PSR J2222-0137 and pulsar-black hole binaries Open
Context . Scalar-tensor gravity (STG) theories are well-motivated alternatives to general relativity (GR). One class of STG theories, Damour–Esposito–Farèse (DEF) gravity, has a massless scalar field with two arbitrary coupling parameters.…
View article: A new pulsar timing model for scalar-tensor gravity with applications to PSR J2222-0137 and pulsar-black hole binaries
A new pulsar timing model for scalar-tensor gravity with applications to PSR J2222-0137 and pulsar-black hole binaries Open
Context. Scalar-tensor gravity (STG) theories are well-motivated alternatives to general relativity (GR). One class of STG theories, the Damour-Esposito-Farese (DEF) gravity, has a massless scalar field with two arbitrary coupling paramete…
View article: News and views regarding PSR J1757–1854, a highly-relativistic binary pulsar
News and views regarding PSR J1757–1854, a highly-relativistic binary pulsar Open
View article: Gravitational signal propagation in the double pulsar studied with the MeerKAT telescope
Gravitational signal propagation in the double pulsar studied with the MeerKAT telescope Open
The double pulsar PSR J0737−3039A/B has offered a wealth of gravitational experiments in the strong-field regime, all of which general relativity has passed with flying colours. In particular, among current gravity experiments that test ph…
View article: Closing a spontaneous-scalarization window with binary pulsars
Closing a spontaneous-scalarization window with binary pulsars Open
Benefitting from the unequaled precision of the pulsar timing technique, binary pulsars are important testbeds of gravity theories, providing some of the tightest bounds on alternative theories of gravity. One class of well-motivated alter…
View article: Strong-Field Gravity Tests with the Double Pulsar
Strong-Field Gravity Tests with the Double Pulsar Open
Continued observations of the Double Pulsar, PSR J0737-3039A/B, consisting of\ntwo radio pulsars (A and B) that orbit each other with a period of 2.45hr in a\nmildly eccentric (e=0.088) binary system, have led to large improvements in the\…
View article: The Variability of the Black-Hole Image in M87 at the Dynamical Time Scale
The Variability of the Black-Hole Image in M87 at the Dynamical Time Scale Open
The black-hole images obtained with the Event Horizon Telescope (EHT) are expected to be variable at the dynamical timescale near their horizons. For the black hole at the center of the M87 galaxy, this timescale (5-61 days) is comparable …
View article: PSR J2222−0137
PSR J2222−0137 Open
Context. The PSR J2222−0137 binary system has a set of features that make it a unique laboratory for tests of gravity theories. Aims. To fully exploit the system’s potential for these tests, we aim to improve the measurements of its physic…
View article: An 86 GHz Search for Pulsars in the Galactic Center with the Atacama Large Millimeter / submillimeter Array
An 86 GHz Search for Pulsars in the Galactic Center with the Atacama Large Millimeter / submillimeter Array Open
We report on the first pulsar and transient survey of the Galactic Center (GC) with the Atacama Large Millimeter/submillimeter Array (ALMA). The observations were conducted during the Global Millimeter VLBI Array campaign in 2017 and 2018.…
View article: The relativistic binary programme on MeerKAT: science objectives and first results
The relativistic binary programme on MeerKAT: science objectives and first results Open
We describe the ongoing Relativistic Binary programme (RelBin), a part of the MeerTime large survey project with the MeerKAT radio telescope. RelBin is primarily focused on observations of relativistic effects in binary pulsars to enable m…
View article: Parkes observations for project P1054 semester 2021APRS_04
Parkes observations for project P1054 semester 2021APRS_04 Open
With this proposal we ask time for a timing follow-up campaign of the first 5 mllisecond pulsars discovered in the TRAPUM (TRAnsients and PUlsars with Meerkat) survey. The sources have been detected in targeted observations of Fermi uniden…
View article: Understanding and improving the timing of PSR J0737−3039B
Understanding and improving the timing of PSR J0737−3039B Open
\nThe double pulsar (PSR J0737−3039A/B) provides some of the most stringent tests of general relativity (GR) and its alternatives. The success of this system in tests of GR is largely due to the high-precision, long-term timing of its recy…
View article: A revisit of PSR J1909−3744 with 15-yr high-precision timing
A revisit of PSR J1909−3744 with 15-yr high-precision timing Open
We report on a high-precision timing analysis and an astrophysical study of the binary millisecond pulsar, PSR J1909−3744, motivated by the accumulation of data with well improved quality over the past decade. Using 15 yr of observations w…
View article: Gravity Tests with Radio Pulsars
Gravity Tests with Radio Pulsars Open
The discovery of the first binary pulsar in 1974 has opened up a completely new field of experimental gravity. In numerous important ways, pulsars have taken precision gravity tests quantitatively and qualitatively beyond the weak-field sl…
View article: New graviton mass bound from binary pulsars
New graviton mass bound from binary pulsars Open
In Einstein's general relativity, gravity is mediated by a massless metric field. The extension of general relativity to consistently include a mass for the graviton has profound implications for gravitation and cosmology. Salient features…
View article: Constraining the dense matter equation-of-state with radio pulsars
Constraining the dense matter equation-of-state with radio pulsars Open
Radio pulsars provide some of the most important constraints for our understanding of matter at supranuclear densities. So far, these constraints are mostly given by precision mass measurements of neutron stars (NS). By combining single me…
View article: An improved test of the strong equivalence principle with the pulsar in a triple star system
An improved test of the strong equivalence principle with the pulsar in a triple star system Open
This repository contains the source code of the Nutimo software, the dataset and results of the article "An improved test of the strong equivalence principle with the pulsar in a triple star system", Voisin, Cognard, Freire, Wex, Guillemot…