The Tetrahedral 4-Body Problem with Rotation

Details The Tetrahedral 4-Body Problem with Rotation The Tetrahedral 4-Body Problem with Rotation

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998cemda..71...15v&link_type=abstract

Celestial Mechanics and Dynamical Astronomy, v. 71, Issue 1, p. 15-33 (1998).

Astronomy and Astrophysics

Astronomy

3

Collision Singularities, Blow-Up, Total Collision Manifold, Blow&Hyphen, Up

Scientific paper

We consider four bodies in space with same masses forming two binaries, each one symmetric with respect to a fixed axis and moving under Newtonian gravitation in opposite directions about this axis. It is given a direct proof that all singularities of this model are due to collisions, and it is proved that the singularities due to simultaneous double collisions are regularizable.

Affiliated with

Also associated with

No associations

Rating

The Tetrahedral 4-Body Problem with Rotation does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The Tetrahedral 4-Body Problem with Rotation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Tetrahedral 4-Body Problem with Rotation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1368436