Neutron star pulse profile observations as extreme gravity probes

Abstract

The x-ray emission of hot spots on the surface of neutron stars is the prime target of the Neutron star Interior Composition Explorer (NICER). These x-ray pulse profiles not only encode information of the bulk properties of these stars, which teaches us about matter at supranuclear densities, but also about the spacetime curvature around them which teaches us about relativistic gravity. We explore the possibility of performing strong-gravity tests with NICER observations using a recently developed pulse profile model beyond general relativity. Our results suggest that NICER can place constraints on deviations from general relativity due to an additional scalar degree of freedom which are independent and competitive relative to constraints with binary pulsar observations.

arXiv comment7 pages, 3 figures. v2: updated title and new appendix

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• Astrophysical and theoretical physics implications from multimessenger neutron star observations
• Spontaneous scalarization
• The surface of rapidly-rotating neutron stars: implications to neutron star parameter estimation
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