UROP Research Mentor Project Submission Portal: Submission #1230
Submission information
Submission Number: 1230
Submission ID: 20746
Submission UUID: 2a143d25-4e18-41d2-8a9b-a42eab6dd312
Submission URI: /urop-research-mentor-project-submission-portal
Submission Update: /urop-research-mentor-project-submission-portal?token=fV29KOISmsP_5X4lcSqP38nsO0bSWXSECt-SWzG74vs
Created: Mon, 08/18/2025 - 12:20 PM
Completed: Mon, 08/18/2025 - 12:43 PM
Changed: Mon, 08/25/2025 - 12:32 PM
Remote IP address: 144.174.27.244
Submitted by: Anonymous
Language: English
Is draft: No
Webform: UROP Project Proposal Portal
Submitted to: UROP Research Mentor Project Submission Portal
Research Mentor Information
Additional Research Mentor(s)
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Overall Project Details
Experiments in Computational Stellar Astrophysics
astronomy physics computer programming data analytics
Yes
1
physics and astrophysics, physics, statistics, computer science, computational science, mathematics, engineering, oceanography, meteorology
On FSU Main Campus
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Partially Remote
10
Flexible schedule (Combination of business and outside of business. TBD between student and research mentor.)
Motivated by observations of supernova remnants such as SN 1987A or Tycho, we are investigating links between the supernova progenitor structure, instabilities developing during the explosion process, and characteristics of emerging young supernova remnants. The starting point for such investigations are stellar evolution studies of supernova progenitors.
From practical point of view, stellar evolution calculations require solving a set of coupled, nonlinear ordinary or partial differential equations. In this project, we will be using the MESA code,
http://mesa.sourceforge.net/
to solve the required evolutionary equations. In recent years, MESA had become a tool of choice for studying variety of astrophysical systems such as stars, binary stars, planets, and basic physics problems in dedicated settings. In this project, we study the evolution of thermonuclear flames powering Type Ia supernovae explosions, and assess sensitivity of their properties, such as speed and width, on the fuel parameters. The results of this study will subsequently be used as input to supernova explosion codes such as Agile-IDSA,
http://www.physik.unibas.ch/~liebend/download/index.html
or FLASH,
https://flash.rochester.edu/site/flashcode/
More advanced students may participate in and contribute to the analysis of multiphysics simulation results, such as computing nucleosynthetic yields and obtaining specific characteristics of explosion models.
This project is strongly computationally-oriented and requires practical user knowledge of Linux or MacOS operating system. In addition, a broader range of topics is available to students fluent with programming languages such as C, C++, Fortran, or Python. Familiarity with simulation data analysis and visualization tools (e.g. Excel, gnuplot, matplotlib) is a plus.
Applications of students who do not have programming skills or do not plan taking a programming class during the first semester of this project are strongly discouraged.
Additional information related to the project can be obtained at
http://people.sc.fsu.edu/~tplewa/Research/index.html
From practical point of view, stellar evolution calculations require solving a set of coupled, nonlinear ordinary or partial differential equations. In this project, we will be using the MESA code,
http://mesa.sourceforge.net/
to solve the required evolutionary equations. In recent years, MESA had become a tool of choice for studying variety of astrophysical systems such as stars, binary stars, planets, and basic physics problems in dedicated settings. In this project, we study the evolution of thermonuclear flames powering Type Ia supernovae explosions, and assess sensitivity of their properties, such as speed and width, on the fuel parameters. The results of this study will subsequently be used as input to supernova explosion codes such as Agile-IDSA,
http://www.physik.unibas.ch/~liebend/download/index.html
or FLASH,
https://flash.rochester.edu/site/flashcode/
More advanced students may participate in and contribute to the analysis of multiphysics simulation results, such as computing nucleosynthetic yields and obtaining specific characteristics of explosion models.
This project is strongly computationally-oriented and requires practical user knowledge of Linux or MacOS operating system. In addition, a broader range of topics is available to students fluent with programming languages such as C, C++, Fortran, or Python. Familiarity with simulation data analysis and visualization tools (e.g. Excel, gnuplot, matplotlib) is a plus.
Applications of students who do not have programming skills or do not plan taking a programming class during the first semester of this project are strongly discouraged.
Additional information related to the project can be obtained at
http://people.sc.fsu.edu/~tplewa/Research/index.html
All the required work will be done on desktop computers provided by the Department of Scientific Computing or with student's laptop computers serving as front ends to departmental computers (connecting via Remote Desktop/Anydesk software), and in person or Zoom for weekly communications.
The project tasks involve,
(1) Review text book information about mathematics and physics relevant to problems in stellar evolution.
(2) Familiarize with the Linux operating system. Download, install, and familiarize with the MESA stellar evolution code.
(3) Construct a series of stellar evolution tracks for various stellar masses (Hertzsprung-Russel Diagram).
(4) Present evolution of stellar structure using Kippenhahn's diagrams (see, e.g., https://github.com/orlox/mkipp ).
(5) Study sensitivity of stellar progenitors characteristics or stellar physics phenomena to problem parameters.
(6) Obtain a series of stellar evolution or relevant multiphysics simulations.
(7) Analyze obtained results.
(8) Prepare a poster presenting the project findings.
The project tasks involve,
(1) Review text book information about mathematics and physics relevant to problems in stellar evolution.
(2) Familiarize with the Linux operating system. Download, install, and familiarize with the MESA stellar evolution code.
(3) Construct a series of stellar evolution tracks for various stellar masses (Hertzsprung-Russel Diagram).
(4) Present evolution of stellar structure using Kippenhahn's diagrams (see, e.g., https://github.com/orlox/mkipp ).
(5) Study sensitivity of stellar progenitors characteristics or stellar physics phenomena to problem parameters.
(6) Obtain a series of stellar evolution or relevant multiphysics simulations.
(7) Analyze obtained results.
(8) Prepare a poster presenting the project findings.
Recommended: practical knowledge of a Linux/MacOS-type operating system.
Required: practical knowledge of MATLAB, Python, or Fortran/C/C++.
Required: strong interest in nature of physics phenomena and good preparation in the areas of mathematics, physics, or statistics.
Required: practical knowledge of MATLAB, Python, or Fortran/C/C++.
Required: strong interest in nature of physics phenomena and good preparation in the areas of mathematics, physics, or statistics.
Promoting learning through inquiry -- the Socratic method.
Sharing own research experience.
Creating a safe environment in which mentees feel that is acceptable to fail and learn from their mistakes.
Sharing own research experience.
Creating a safe environment in which mentees feel that is acceptable to fail and learn from their mistakes.
https://news.fsu.edu/news/science-technology/2020/12/17/fsu-computational-scientist-demonstrates-how-supernovae-detonate/
https://arxiv.org/abs/2505.18482
https://doi.org/10.1093/mnrasl/slaa141
https://arxiv.org/abs/2401.16674
https://doi.org/10.1093/mnrasl/slaa141
https://arxiv.org/abs/2401.16674
No
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UROP Program Elements
Yes
Yes
Yes
Yes
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2025
https://cre.fsu.edu/urop-research-mentor-project-submission-portal?element_parents=elements/research_mentor_information/headshot_optional_&ajax_form=1&_wrapper_format=drupal_ajax&token=fV29KOISmsP_5X4lcSqP38nsO0bSWXSECt-SWzG74vs