29,156 research outputs found
Coupling vector and pseudoscalar mesons to study baryon resonances
A study of meson-baryon systems with total strangeness -1 is made within a
framework based on the chiral and hidden local symmetries. These systems
consist of octet baryons, pseudoscalar and vector mesons. The pseudoscalar
meson-baryon (PB) dynamics has been earlier found determinant for the existence
of some strangeness -1 resonances, for example, ,
, etc. The motivation of the present work is to study the effect
of coupling the closed vector meson-baryon (VB) channels to these resonances.
To do this, we obtain the and
amplitudes from the t-channel diagrams and the
amplitudes are calculated using the Kroll-Ruddermann term where, considering
the vector meson dominance phenomena, the photon is replaced by a vector meson.
The calculations done within this formalism reveal a very strong coupling of
the VB channels to the and . In the isospin 1
case, we find an evidence for a double pole structure of the
which, like the isospin 0 resonances, is also found to couple strongly to the
VB channels. The strong coupling of these low-lying resonances to the VB
channels can have important implications on certain reactions producing them.Comment: Minor typos corrected (in Eq.(22) and axis-labels of some figures
Plausible explanation of the puzzle
From a Faddeev calculation for the
system we show the plausible existence of three dynamically generated
baryon states below 2.3 GeV whereas only two
resonances, and
are cataloged in the Particle Data Book
Review. Our results give theoretical support to data analyses extracting two
distinctive resonances, and
from which the mass of
is estimated. We propose that these two
resonances should be cataloged instead of This
proposal gets further support from the possible assignment of the other baryon
states found in the approach in the with
sectors to known baryonic resonances. In
particular, is naturally interpreted as a bound state.Comment: 13 pages, 7 figure
Mass-radius relation for magnetized strange quark stars
We review the stability of magnetized strange quark matter (MSQM) within the
phenomenological MIT bag model, taking into account the variation of the
relevant input parameters, namely, the strange quark mass, baryon density,
magnetic field and bag parameter. A comparison with magnetized asymmetric quark
matter in -equilibrium as well as with strange quark matter (SQM) is
presented. We obtain that the energy per baryon for MSQM decreases as the
magnetic field increases, and its minimum value at vanishing pressure is lower
than the value found for SQM, which implies that MSQM is more stable than
non-magnetized SQM. The mass-radius relation for magnetized strange quark stars
is also obtained in this framework.Comment: 7 pages, 6 figures. To be published in the Proceedings of 4th
International Workshop on Relativistic Astrophysical and Astronomy IWARA0
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