From cba732925ae67bdec704db8924bf4ec42165b222 Mon Sep 17 00:00:00 2001
From: duetosymmetry <679461+duetosymmetry@users.noreply.github.com>
Date: Tue, 14 Jan 2025 11:03:43 +0000
Subject: [PATCH] Auto paper update

---
 _papers/Mroue:2008fu.md | 43 ++++++++++++++++++++---------------------
 1 file changed, 21 insertions(+), 22 deletions(-)

diff --git a/_papers/Mroue:2008fu.md b/_papers/Mroue:2008fu.md
index 5002434..d8ee99c 100644
--- a/_papers/Mroue:2008fu.md
+++ b/_papers/Mroue:2008fu.md
@@ -1,36 +1,35 @@
 ---
 title: "Ineffectiveness of Padé resummation techniques in post-Newtonian approximations"
 authors:
-  - "Abdul H. Mroué"
-  - "Lawrence E. Kidder"
-  - "Saul A. Teukolsky"
-jref: "Phys. Rev. D 78, 044004 (2008)"
+  - "Mroue, Abdul H."
+  - "Kidder, Lawrence E."
+  - "Teukolsky, Saul A."
+jref: "Phys.Rev.D 78, 044004 (2008)"
 doi: "10.1103/PhysRevD.78.044004"
 date: 2008-05-15
 arxiv: "0805.2390"
-used_spec: true
 abstract: |
   We test the resummation techniques used in developing Padé and
-  Effective One Body (EOB) waveforms for gravitational wave
-  detection. Convergence tests show that Padé approximants of the
-  gravitational wave energy flux do not accelerate the convergence of
-  the standard Taylor approximants even in the test mass limit, and
-  there is no reason why Padé transformations should help in
-  estimating parameters better in data analysis. Moreover, adding a
-  pole to the flux seems unnecessary in the construction of these
-  Padé-approximated flux formulas. Padé approximants may be useful in
-  suggesting the form of fitting formulas. We compare a 15-orbit
+  Effective One Body (EOB) waveforms for gravitational wave detection.
+  Convergence tests show that Padé approximants of the gravitational
+  wave energy flux do not accelerate the convergence of the standard
+  Taylor approximants even in the test mass limit, and there is no
+  reason why Padé transformations should help in estimating
+  parameters better in data analysis. Moreover, adding a pole to the
+  flux seems unnecessary in the construction of these
+  Padé-approximated flux formulas. Padé approximants may be useful
+  in suggesting the form of fitting formulas. We compare a 15-orbit
   numerical waveform of the Caltech-Cornell group to the suggested
   Padé waveforms of Damour et al. in the equal mass, nonspinning
-  quasi-circular case. The comparison suggests that the Padé waveforms
-  do not agree better with the numerical waveform than the standard
-  Taylor based waveforms. Based on this result, we design a simple EOB
-  model by modifiying the ET EOB model of Buonanno et al., using the
-  Taylor series of the flux with an unknown parameter at the fourth
-  post-Newtonian order that we fit for. This simple EOB model
+  quasi-circular case. The comparison suggests that the Padé
+  waveforms do not agree better with the numerical waveform than the
+  standard Taylor based waveforms. Based on this result, we design a
+  simple EOB model by modifiying the ET EOB model of Buonanno et al.,
+  using the Taylor series of the flux with an unknown parameter at the
+  fourth post-Newtonian order that we fit for. This simple EOB model
   generates a waveform having a phase difference of only 0.002 radians
   with the numerical waveform, much smaller than 0.04 radians the
   phase uncertainty in the numerical data itself. An EOB Hamiltonian
-  can make use of a Padé transformation in its construction, but this
-  is the only place Padé transformations seem useful.
+  can make use of a Padé transformation in its construction, but
+  this is the only place Padé transformations seem useful.
 ---