834 research outputs found
Anomalous Hall effect in dense QCD matter
In this letter, we investigate the anomalous Hall effect in dense QCD matter.
When the dual chiral density wave which is the spatially modulated chiral
condensate appears in the medium, it gives rise to two Weyl points to the
single-particle energy-spectrum and then the anomalous Hall conductivity
becomes nonzero. Then, dense QCD matter is analogous to the Weyl semimetal. The
direct calculation of the Hall conductivity by way of Kubo's linear response
theory gives the term proportional to the distance between the Weyl points.
Unlike the Weyl semimetal, there appears the additional contribution induced by
axial anomaly.Comment: 5 pages, 2 figure
Magnetic properties in the inhomogeneous chiral phase
We investigate the magnetic properties of quark matter in the inhomogeneous
chiral phase, where both scalar and pseudoscalar condensates spatially
modulate. The energy spectrum of the lowest Landau level becomes asymmetric
about zero in the external magnetic field, and gives rise to the remarkably
magnetic properties: quark matter has a spontaneous magnetization, while the
magnetic susceptibility does not diverge on the critical point.Comment: 6 pages, 3 figures, talk given in Excited QCD 2016, Mar. 6-12, 2016,
Costa da Caparica, Portuga
The Supernova Remnant W44: confirmations and challenges for cosmic-ray acceleration
The middle-aged supernova remnant (SNR) W44 has recently attracted attention
because of its relevance regarding the origin of Galactic cosmic-rays. The
gamma-ray missions AGILE and Fermi have established, for the first time for a
SNR, the spectral continuum below 200 MeV which can be attributed to neutral
pion emission. Confirming the hadronic origin of the gamma-ray emission near
100 MeV is then of the greatest importance. Our paper is focused on a global
re-assessment of all available data and models of particle acceleration in W44,
with the goal of determining on a firm ground the hadronic and leptonic
contributions to the overall spectrum. We also present new gamma-ray and CO
NANTEN2 data on W44, and compare them with recently published AGILE and Fermi
data. Our analysis strengthens previous studies and observations of the W44
complex environment and provides new information for a more detailed modeling.
In particular, we determine that the average gas density of the regions
emitting 100 MeV - 10 GeV gamma-rays is relatively high (n= 250 - 300 cm^-3).
The hadronic interpretation of the gamma-ray spectrum of W44 is viable, and
supported by strong evidence. It implies a relatively large value for the
average magnetic field (B > 10^2 microG) in the SNR surroundings, sign of field
amplification by shock-driven turbulence. Our new analysis establishes that the
spectral index of the proton energy distribution function is p1 = 2.2 +/- 0.1
at low energies and p2 = 3.2 +/- 0.1 at high energies. We critically discuss
hadronic versus leptonic-only models of emission taking into account
simultaneously radio and gamma-ray data. We find that the leptonic models are
disfavored by the combination of radio and gamma-ray data. Having determined
the hadronic nature of the gamma-ray emission on firm ground, a number of
theoretical challenges remains to be addressed.Comment: 13 pages, 11 figures, accepted by A&
Recombining Plasma and Hard X-ray Filament in the Mixed-Morphology Supernova Remnant W44
We report new features of the typical mixed-morphology (MM) supernova remnant
(SNR) W44. In the X-ray spectra obtained with Suzaku, radiative recombination
continua (RRCs) of highly ionized atoms are detected for the first time. The
spectra are well reproduced by a thermal plasma in a recombining phase. The
best-fit parameters suggest that the electron temperature of the shock-heated
matters cooled down rapidly from ,keV to ,keV, possibly due to
adiabatic expansion (rarefaction) occurred years ago. We also
discover hard X-ray emission which shows an arc-like structure
spatially-correlated with a radio continuum filament. The surface brightness
distribution shows a clear anti-correlation with CO (J=2-1) emission
from a molecular cloud observed with NANTEN2. While the hard X-ray is most
likely due to a synchrotron enhancement in the vicinity of the cloud, no
current model can quantitatively predict the observed flux.Comment: 10 pages, 5 figures, accepted for publication in PAS
Changes in body mass index by birth cohort in Japanese adults: results from the National Nutrition Survey of Japan 1956–2005
Background The National Nutrition Survey, Japan (NNS-J) provides annual anthropometric information for a whole nation over 50 years. Based on this survey, the mean body mass index (BMI) of Japanese men and elderly women has increased in recent decades, but that of young women has decreased. We examined the effect of birth cohort on this phenomenon
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