The impacts of dust size distribution on the head-on collision of quantum dust-acoustic solitary waves in ultradense astrophysical objects

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Head-On Collision, Quantum Dust-Acoustic Solitary Waves, The Extended Poincaré-Lighthill-Kuo, Ultradense Astrophysical Objects, The Dust Size Distribution

Scientific paper

The head-on collision between two quantum dust-acoustic solitary waves (QDASWs) in ultradense astrophysical objects has been investigated theoretically using the extended Poincaré-Lighthill-Kuo (PLK) method. The Korteweg-de Vries equations and the analytical phase shifts after the head-on collision of the two QDASWs in quantum dusty plasmas are obtained. Numerically, the obtained results demonstrate that the dust size distribution, the quantum corrections of diffraction and the temperatures of electrons and ions have strong effects on the nature of the phase shifts and the trajectories of the two QDASWs after collision.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

The impacts of dust size distribution on the head-on collision of quantum dust-acoustic solitary waves in ultradense astrophysical objects 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 impacts of dust size distribution on the head-on collision of quantum dust-acoustic solitary waves in ultradense astrophysical objects, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The impacts of dust size distribution on the head-on collision of quantum dust-acoustic solitary waves in ultradense astrophysical objects will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1285295

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.