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_papers/Muhammed:2024zmk.md

@@ -11,11 +11,10 @@ authors:
   - "Kidder, Lawrence E."
   - "Pfeiffer, Harald P."
   - "Scheel, Mark A."
-jref:
-doi:
+jref: "Phys.Rev.D 110, 124063 (2024)"
+doi: "10.1103/PhysRevD.110.124063"
 date: 2024-03-08
 arxiv: "2403.05642"
-used_spec: true
 abstract: |
   Binary neutron star mergers produce massive, hot, rapidly
   differentially rotating neutron star remnants; electromagnetic and
@@ -28,12 +27,12 @@ abstract: |
   a constant angular momentum sequence, the onset of unstable stars is
   found at maximum density less than but close to the density of
   maximum mass. In this paper, we test this turning point criterion
-  for non-monotonic angular velocity profiles and non-isentropic
-  entropy profiles, both chosen to more realistically model post-
-  merger equilibria. Stability is assessed by evolving perturbed
-  equilibria in 2D using the Spectral Einstein Code. We present tests
-  of the code's new capability for axisymmetric metric evolution. We
-  confirm the turning point theorem and determine the region of our
-  rotation law parameter space that provides highest maximum mass for
-  a given angular momentum.
+  for nonmonotonic angular velocity profiles and nonisentropic entropy
+  profiles, both chosen to more realistically model postmerger
+  equilibria. Stability is assessed by evolving perturbed equilibria
+  in 2D using the spectral einstein Code. We present tests of the
+  code’s new capability for axisymmetric metric evolution. We confirm
+  the turning point theorem and determine the region of our rotation
+  law parameter space that provides highest maximum mass for a given
+  angular momentum.
 ---