Results 1 to 10 of about 235,480 (181)
Light- and strange-quark mass dependence of the ρ(770) meson revisited [PDF]
Recent lattice data on ππ-scattering phase shifts in the vector-isovector channel, pseudoscalar meson masses and decay constants for strange-quark masses smaller or equal to the physical value allow us to study the strangeness dependence of these ...
R. Molina, J. Ruiz de Elvira
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Properties of strange quark matter and strange quark stars
A Polyakov chiral $$\text {SU(3)}$$ SU(3) quark mean-field (PCQMF) model is applied to study the properties of strange quark matter (SQM) and strange quark star (SQS) in $$\beta $$ β -equilibrium.
Manisha Kumari, Arvind Kumar
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Solitonic effect on relativistic string cloud spacetime attached with strange quark matter
In this research paper, we discussed some geometric axioms of a relativistic string cloud spacetime attached with strange quark matter. We determined the conformal $ \eta $-Ricci soliton on a relativistic string cloud spacetime attached with strange ...
Yanlin Li +4 more
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CLS 2+1 flavor simulations at physical light-and strange-quark masses [PDF]
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
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Chiral perturbation theory: Expansions in the mass of the strange quark [PDF]
J. Gasser, H. Leutwyler
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Strange quark as a probe for new physics in the Higgs sector [PDF]
This paper describes a novel algorithm for tagging jets originating from the hadronisation of strange quarks (strange-tagging) with the future International Large Detector (ILD) at the International Linear Collider (ILC).
A. Albert+27 more
semanticscholar +1 more source
Effects of Anisotropy on Strongly Magnetized Neutron and Strange Quark Stars in General Relativity [PDF]
We investigate the properties of anisotropic, spherically symmetric compact stars, especially neutron stars (NSs) and strange quark stars (SQSs), made of strongly magnetized matter. The NSs are described by the SLy equation of state (EOS) and the SQSs by
D. Deb, B. Mukhopadhyay, F. Weber
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Was GW190814 a Black Hole-Strange Quark Star System? [PDF]
We investigate the possibility that the low mass companion of the black hole in the source of GW190814 was a strange quark star. This possibility is viable within the so-called two-families scenario in which neutron stars and strange quark stars coexist.
I. Bombaci+4 more
semanticscholar +1 more source
Gravitational Waves from Strange Star Core–Crust Oscillation
According to the strange quark matter hypothesis, pulsars may actually be strange stars composed of self-bound strange quark matter. The normal matter crust of a strange star, unlike that of a normal neutron star, is supported by a strong electric field.
Ze-Cheng Zou+2 more
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Strange Quark Stars in 4D Einstein–Gauss–Bonnet Gravity [PDF]
The existence of strange matter in compact stars may give rise to striking outcomes of the various physical phenomena. As an alternative to neutron stars, a new class of compact stars called strange stars should exist if the strange matter hypothesis is ...
A. Banerjee+2 more
semanticscholar +1 more source