Share
Rapidly Rotating Axisymmetric Neutron Stars and Quark Matter
Partha Roy Chowdhury
(Author)
·
LAP Lambert Academic Publishing
· Paperback
Rapidly Rotating Axisymmetric Neutron Stars and Quark Matter - Roy Chowdhury, Partha
Choose the list to add your product or create one New List
✓ Product added successfully to the Wishlist.
Go to My Wishlists
Origin: U.S.A.
(Import costs included in the price)
It will be shipped from our warehouse between
Wednesday, August 14 and
Wednesday, August 21.
You will receive it anywhere in United Kingdom between 1 and 3 business days after shipment.
Synopsis "Rapidly Rotating Axisymmetric Neutron Stars and Quark Matter"
Neutron stars (NSs) are ideal astrophysical laboratories for testing theories of dense matter and provide connections among astrophysics, nuclear and particle physics. The recent discoveries of the binary millisecond pulsars PSR J0952-0607, PSR J0740+6620, PSR J0348+0432 and PSR J1614-2230 suggest that the maximum mass Mmax lie within 2.35 0.17M⊙, 2.08 0.07 M⊙, 2.01 0.04 M⊙ and 1.97 0.04 M⊙ respectively, where M⊙ is the solar mass. The largest mass measurements are powerfully influencing the behavior of nuclear symmetry energy near the nuclear saturation density and the high-density equation of state (EoS) because of the existence of the maximum mass. The properties of pure hadronic and hybrid compact stars using a suitable realistic nuclear equation of state for β-equilibrated neutron star matter are discussed here. We have employed the pure hadronic EoS and the EoS combined with quark for the ultra-dense inner core to determine the mass of NS. The significant reduction of maximum mass has been found with the inclusion of quark core.
- 0% (0)
- 0% (0)
- 0% (0)
- 0% (0)
- 0% (0)
All books in our catalog are Original.
The book is written in English.
The binding of this edition is Paperback.
✓ Producto agregado correctamente al carro, Ir a Pagar.