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The focus of his prize-winning thesis is on observations and
modeling of binary millisecond pulsars. But in addition, John
Antoniadis covers a wide range of observational measurements of
binary compact stars systems and tests of General Relativity, like
indirect measurements of gravitational wave emission and posing the
most stringent constraints on Scalar-Tensor gravity theories. Among
others, he presents a system that hosts the most massive neutron
star known to date, which has important ramifications for
strong-field gravity and nuclear physics. This impressive work was
awarded the Otto-Hahn Medal of the Max-Planck Society and the Best
PhD in Gravity, Particle and Atomic physics award by the German
Physics Society (DPG).
The focus of his prize-winning thesis is on observations and
modeling of binary millisecond pulsars. But in addition, John
Antoniadis covers a wide range of observational measurements of
binary compact stars systems and tests of General Relativity, like
indirect measurements of gravitational wave emission and
posing the most stringent constraints on Scalar-Tensor gravity
theories. Among others, he presents a system that hosts the most
massive neutron star known to date, which has important
ramifications for strong-field gravity and nuclear
physics. This impressive work was awarded the Otto-Hahn Medal
of the Max-Planck Society and the Best PhD in Gravity, Particle and
Atomic physics award by the German Physics Society (DPG).
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