Results 91 to 100 of about 112,649 (235)
Strange matter and its stability in presence of magnetic field [PDF]
arXiv, 1995 We study the effect of a magnetic field on the interacting quark matter and apply to strange star. We considere the low temperature approximation to strange matter. We find that the interacting strange quark matter is more stable compare to free quark gas in presence of strong external magnetic field with zero and finite temperature.
arxiv
Gravitational Wave Emission from Close-in Strange Quark Planets Around Strange Stars with Magnetic Interactions [PDF]
Monthly Notices of the Royal Astronomical Society (MNRAS),
531:3905, 2024According to the strange quark matter hypothesis, strange planets may exist, which are planetary mass objects composed of almost equal numbers of up, down and strange quarks. A strange planet can revolve around its host strange star in a very close-in orbit.
arxiv +1 more source
Modified F(R,T)-Gravity Model Coupled with Magnetized Strange Quark Matter Fluid
MathematicsThis research note presents the properties of the F(R,T)-gravity model in combination with magnetized strange quark matter. We obtain the equation of state for the magnetized strange quark matter in the F(R,T)-gravity model endowed with the Lagrangian ...
Mohd Danish Siddiqi +2 more
doaj +1 more source
Phase diagram of dense neutral three-flavor quark matter [PDF]
, 2007 We study the phase diagram of dense, locally neutral three-flavor quark matter as a function of the strange quark mass, the quark chemical potential, and the temperature, employing a general nine-parameter ansatz for the gap matrix.
Rischke, Dirk-Hermann +2 more
core
Reading Wolfgang Herrndorf's Tschick (2010)
Die Unterrichtspraxis/Teaching German, Volume 57, Issue 1, Page 71-86, Spring 2024.Abstract This article highlights how Wolfgang Herrndorf's bestselling novel Tschick (2010) is particularly well suited for advanced courses focused on cultural and linguistic enrichment. Herrndorf's Tschick, I argue, facilitates interaction, engagement, and individual interpretation; is linguistically accessible because of its use of high‐frequency ...
Brigitte Rossbacher
wiley +1 more source
Torsional oscillations of strange stars
EPJ Web of Conferences, 2014 Strange stars are one of the hypothetical compact stellar objects that can be formed after a supernova explosion. The existence of these objects relies on the absolute stability of strange collapsed quark matter with respect to standard nuclear matter ...
Mannarelli Massimo
doaj +1 more source
Differential rotation in compact objects with hyperons and delta isobars
Astronomische Nachrichten, Volume 345, Issue 2-3, February-March 2024.Abstract Neutron stars may experience differential rotation on short, dynamical timescales following extreme astrophysical events like binary neutron star mergers. In this work, the masses and radii of differentially rotating neutron star models are computed.
Delaney Farrell +3 more
wiley +1 more source
Strangeness Content of the Nucleon in the \chiCQM_{config} [PDF]
arXiv, 2007 Several parameters characterizing the strangeness content of the nucleon have been calculated in the chiral constituent quark model with configuration mixing (\chiCQM_{config}) which is known to provide a satisfactory explanation of the ``proton spin problem'' and related issues. In particular, we have calculated the strange spin polarization \Delta s,
arxiv
CLS 2+1 flavor simulations at physical light-and strange-quark masses
EPJ Web of Conferences, 2018 We report recent efforts by CLS to generate an ensemble with physical lightand strange-quark masses in a lattice volume of 192 × 963 at β = 3:55 corresponding to a lattice spacing of 0:064 fm.
Mohler Daniel +2 more
doaj +1 more source
Phase diagram of dense neutral three-flavor quark matter
, 2004 We study the phase diagram of dense, locally neutral three-flavor quark matter as a function of the strange quark mass, the quark chemical potential, and the temperature, employing a general nine-parameter ansatz for the gap matrix.
Alford +78 more
core +1 more source