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Instructions

Student presentations must have a faculty sponsor.

Abstracts must include a title and a description of the research, scholarship, or creative work. The description should be 150-225 words in length and constructed in a format or style appropriate for the presenter’s discipline.

The following points should be addressed within the selected format or style for the abstract:

  • A clear statement of the problem or question you pursued, or the scholarly goal or creative theme achieved in your work.
  • A brief comment about the significance or uniqueness of the work.
  • A clear description of the methods used to achieve the purpose or goals for the work.
  • A statement of the conclusions, results, outcomes, or recommendations, or if the work is still in progress, the results you expect to report at the event.

Presenter photographs should be head and shoulder shots comparable to passport photos.

Additional Information

More information is available at carthage.edu/celebration-scholars/. The following are members of the Research, Scholarship, and Creativity Committee who are eager to listen to ideas and answer questions:

  • Jun Wang
  • Kim Instenes
  • John Kirk
  • Nora Nickels
  • Andrew Pustina
  • James Ripley

#11: Modeling Binary Compact Object Merger Events Detected by the LIGO and Virgo Gravitational Wave Observatories

Name: Andrew Jocham
Major: Physics
Hometown: Colgate, WI
Faculty Sponsor: Jean Quashnock
Other Sponsors:  
Type of research: Independent research

Name: Chance Hoskinson
Major: Physics
Hometown: NA
Faculty Sponsor: Jean Quashnock
Other Sponsors:  
Type of research: Independent research

Name: Jean Quashnock
Department: Natural Science
Type of research: Independent research

Name: William Schuster
Major: Physics
Hometown: Rockford, IL
Faculty Sponsor: Jean Quashnock
Other Sponsors:  
Type of research: Independent research

Name: Andrew Valentini
Major: Physics
Hometown: NA
Faculty Sponsor: Jean Quashnock
Other Sponsors:  
Type of research: Independent research

Abstract

In this investigation, we model multiple neutron star and black hole merger events detected in the LIGO-Virgo Collaboration. We use Kepler’s Laws and Newtonian mechanics to model an infalling system of two objects with equal masses. We predict the expected increase in frequency or “chirp” of the infalling binary and compare that to what is found in the LIGO-Virgo database (presented in an adjacent poster). In the initial period during which the Newtonian approximation is valid, we find reasonable agreement between our model and the results from the LIGO-Virgo Collaboration, thus verifying the basic physics of the infall. We also estimate the amount of gravitational wave energy emitted during the entire process. This provides a better understanding of the nature of these merger events and why gravitational waves are emitted by these merging compact objects.

Poster file

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