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AMReX-Astro · Sep 30, 2024 · d859fa1 · d859fa1
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diff --git a/paper-parser/papers.bib b/paper-parser/papers.bib
@@ -478,12 +478,43 @@ @article{Boyd_2024
 author = {B Boyd and A Smith Clark and A C Calder and D M Townsley and M Zingale},
 title = {Sensitivity of 3D Convective Urca Simulations to Changes in Urca Reactions},
 journal = {Journal of Physics: Conference Series},
-abstract = {A proposed setting for thermonuclear (Type Ia) supernovae is a white dwarf that has gained mass from a companion to the point of carbon ignit
-ion in the core. There is a simmering phase in the early stages of burning that involves the formation and growth of a core convection zone. One aspect o
-f this phase is the convective Urca process, a linking of weak nuclear reactions to convection that may alter the composition and structure of the white 
-dwarf. Convective Urca is not well understood and requires 3D fluid simulations to realistically model. Additionally, the convection is relatively slow (
-Mach number less than 0.005) so a low-Mach method is needed to make simulating computationally feasible. Using the MAESTROeX low-Mach hydrodynamics code,
- we investigate recent changes to how the weak reactions are modeled in the convective Urca simulations. We present results that quantify the changes to 
-the reaction rates and their impact on the evolution of the simulation.},
+abstract = {A proposed setting for thermonuclear (Type Ia) supernovae
+                  is a white dwarf that has gained mass from a
+                  companion to the point of carbon ignit ion in the
+                  core. There is a simmering phase in the early stages
+                  of burning that involves the formation and growth of
+                  a core convection zone. One aspect o f this phase is
+                  the convective Urca process, a linking of weak
+                  nuclear reactions to convection that may alter the
+                  composition and structure of the white
+                  dwarf. Convective Urca is not well understood and
+                  requires 3D fluid simulations to realistically
+                  model. Additionally, the convection is relatively
+                  slow ( Mach number less than 0.005) so a low-Mach
+                  method is needed to make simulating computationally
+                  feasible. Using the MAESTROeX low-Mach hydrodynamics
+                  code, we investigate recent changes to how the weak
+                  reactions are modeled in the convective Urca
+                  simulations. We present results that quantify the
+                  changes to the reaction rates and their impact on
+                  the evolution of the simulation.},
   subject = {Type Ia supernovae&mdash;Chandrasekhar mass model}
 }
+
+@ARTICLE{2024arXiv240508952G,
+       author = {{Guichandut}, Simon and {Zingale}, Michael and {Cumming}, Andrew},
+        title = "{Hydrodynamical simulations of proton ingestion flashes in Type I X-ray Bursts}",
+      journal = {arXiv e-prints},
+     keywords = {Astrophysics - High Energy Astrophysical Phenomena},
+         year = 2024,
+        month = {may},
+          eid = {arXiv:2405.08952},
+        pages = {arXiv:2405.08952},
+          doi = {10.48550/arXiv.2405.08952},
+archivePrefix = {arXiv},
+       eprint = {2405.08952},
+ primaryClass = {astro-ph.HE},
+       adsurl = {https://ui.adsabs.harvard.edu/abs/2024arXiv240508952G},
+      adsnote = {Provided by the SAO/NASA Astrophysics Data System},
+  subject = {X-ray bursts}
+}
diff --git a/paper-parser/papers.html b/paper-parser/papers.html
@@ -67,6 +67,7 @@ <h1><a href="index.html">MAESTROeX</a></h1>
                     <li>Adam Jacobs (Stony Brook, 2016)</li>
                     <li>Don Willcox (Stony Brook, 2018)</li>
                     <li>Xinlong Li (Stony Brook, 2021)</li>
+                    <li>Simon Guichandut (McGill, 2024)</li>
                   </ul>
                 </li>
 
@@ -160,6 +161,8 @@ <h3>X-ray bursts</h3>
 </header>
 <div class='table-wrapper'>
   <table>
+<tr><td><a href='https://ui.adsabs.harvard.edu/abs/2024arXiv240508952G'>Hydrodynamical simulations of proton ingestion flashes in Type I X-ray Bursts</a><br>
+Guichandut, Simon, Zingale, Michael, &amp; Cumming, Andrew 2024, arXiv e-prints, p. arXiv:2405.08952</td></tr>
 <tr><td><a href='http://adsabs.harvard.edu/abs/2015ApJ...807...60Z'>Comparisons of Two- and Three-Dimensional Convection in Type I X-Ray Bursts</a><br>
 Zingale, M., Malone, C. M., Nonaka, A., Almgren, A. S., &amp; Bell, J. B. 2015, ApJ, 807, p. 60</td></tr>
 <tr><td><a href='http://adsabs.harvard.edu/abs/2014ApJ...788..115M'>Multidimensional Modeling of Type I X-Ray Bursts. II. Two-dimensional Convection in a Mixed H/He Accretor</a><br>

diff --git a/paper-parser/papers.template b/paper-parser/papers.template
@@ -67,6 +67,7 @@
                     <li>Adam Jacobs (Stony Brook, 2016)</li>
                     <li>Don Willcox (Stony Brook, 2018)</li>
                     <li>Xinlong Li (Stony Brook, 2021)</li>
+                    <li>Simon Guichandut (McGill, 2024)</li>
                   </ul>
                 </li>
 

diff --git a/papers.html b/papers.html
@@ -67,6 +67,7 @@ <h1><a href="index.html">MAESTROeX</a></h1>
                     <li>Adam Jacobs (Stony Brook, 2016)</li>
                     <li>Don Willcox (Stony Brook, 2018)</li>
                     <li>Xinlong Li (Stony Brook, 2021)</li>
+                    <li>Simon Guichandut (McGill, 2024)</li>
                   </ul>
                 </li>
 
@@ -160,6 +161,8 @@ <h3>X-ray bursts</h3>
 </header>
 <div class='table-wrapper'>
   <table>
+<tr><td><a href='https://ui.adsabs.harvard.edu/abs/2024arXiv240508952G'>Hydrodynamical simulations of proton ingestion flashes in Type I X-ray Bursts</a><br>
+Guichandut, Simon, Zingale, Michael, &amp; Cumming, Andrew 2024, arXiv e-prints, p. arXiv:2405.08952</td></tr>
 <tr><td><a href='http://adsabs.harvard.edu/abs/2015ApJ...807...60Z'>Comparisons of Two- and Three-Dimensional Convection in Type I X-Ray Bursts</a><br>
 Zingale, M., Malone, C. M., Nonaka, A., Almgren, A. S., &amp; Bell, J. B. 2015, ApJ, 807, p. 60</td></tr>
 <tr><td><a href='http://adsabs.harvard.edu/abs/2014ApJ...788..115M'>Multidimensional Modeling of Type I X-Ray Bursts. II. Two-dimensional Convection in a Mixed H/He Accretor</a><br>