Speaker
Description
Our aims to study the quark-gluon plasma (QGP), theorised to
have been present during the early and expanding stages of our universe. Through the equations of state (EoS) of temperature, pressure and energy density, we can understand more about the evolution of the early universe QGP. The Friedmann equations (derived from the Einstein field equations) are solved by utilising a phenomenological quasi-particle model, where we take into consideration the effective quark mass incorporating the current mass and the thermal mass of the quasi-particles, which are the thermal excitations generated due to the interactions between the quarks and gluons. The results are interesting and significant in the early universe of quark gluon plasma.
Details
Yogesh Kumar, Dr., Deshbandhu College, University of Delhi, Kalkaji, New Delhi, India
| Is this abstract from experiment? | No |
|---|---|
| Name of experiment and experimental site | N/A |
| Is the speaker for that presentation defined? | Yes |
| Internet talk | Yes |
