923 research outputs found
Development of portable NMR polarimeter system for polarized HD target
A portable NMR polarimeter system has been developed to measure the
polarization of a polarized Hydrogen-Deuteride (HD) target for hadron
photoproduction experiments at SPring-8. The polarized HD target is produced at
the Research Center for Nuclear Physics (RCNP), Osaka university and is
transported to SPring-8. The HD polarization should be monitored at both
places. We have constructed the portable NMR polarimeter system by replacing
the devices in the conventional system with the software system with PCI
eXtensions for Instrumentation (PXI). The weight of the NMR system is downsized
from 80 kg to 7 kg, and the cost is reduced to 25%. We check the performance of
the portable NMR polarimeter system. The signal-to-noise (S/N) ratio of the NMR
signal for the portable system is about 50% of that for the conventional NMR
system. This performance of the portable NMR system is proved to be compatible
with the conventional NMR system for the polarization measurement.Comment: 6 page, 8 figures, 2011/Mar/9 Replace Author
Massive Decaying Tau Neutrino and Big Bang Nucleosynthesis
Comparing Big Bang Nucleosynthesis predictions with the light element
abundances inferred from observational data, we can obtain the strong
constraints on some neutrino properties, e.g. number of neutrino species, mass,
lifetime. Recently the deuterium abundances were measured in high red-shift QSO
absorption systems. It is expected that they are close to the primordial
values, however, two groups have reported inconsistent values which are
different in one order of magnitude. In this paper we show how we can constrain
on neutrino mass and its lifetime in each case when we adopt either high
or low deuterium data. We find that if 0.01 \sec
\lesssim \tau_{\nutau} \lesssim 1 \sec and 10\mev \lesssim m_{\nutau}
\lesssim 24\mev, the theoretical predictions agree with the low D/H
abundances. On the other hand if we adopt the high D/H abundances, we obtain
the upper bound of neutrino mass, m_{\nutau}\lesssim 20 \mev.Comment: 11 pages, using LATEX and four postscript figure
Possible solution to the Li problem by the long lived stau
Modification of standard big-bang nucleosynthesis is considered in the
minimal supersymmetric standard model to resolve the excessive theoretical
prediction of the abundance of primordial lithium 7. We focus on the stau as a
next-lightest superparticle, which is long lived due to its small mass
difference with the lightest superparticle. It provides a number of additional
decay processes of and . A particularly
important process is the internal conversion in the stau-nucleus bound state,
which destroys the and effectively. We show
that the modification can lead to a prediction consistent with the observed
abundance of .Comment: 6 pages, 5 figure
Big-Bang Nucleosynthesis with Unstable Gravitino and Upper Bound on the Reheating Temperature
We study the effects of the unstable gravitino on the big-bang
nucleosynthesis. If the gravitino mass is smaller than \sim 10 TeV, primordial
gravitinos produced after the inflation are likely to decay after the big-bang
nucleosynthesis starts, and the light element abundances may be significantly
affected by the hadro- and photo-dissociation processes as well as by the p n
conversion process. We calculate the light element abundances and derived upper
bound on the reheating temperature after the inflation. In our analysis, we
calculate the decay parameters of the gravitino (i.e., lifetime and branching
ratios) in detail. In addition, we performed a systematic study of the hadron
spectrum produced by the gravitino decay, taking account of all the hadrons
produced by the decay products of the gravitino (including the daughter
superparticles). We discuss the model-dependence of the upper bound on the
reheating temperature.Comment: 32 pages, 11 figure
Neutralino Dark Matter from Heavy Gravitino Decay
We propose a new scenario of non-thermal production of neutralino cold dark
matter, in which the overproduction problem of lightest supersymmetric
particles (LSPs) in the standard thermal history is naturally solved. The
mechanism requires a heavy modulus field which decays mainly to ordinary
particles releasing large entropy to dilute gravitinos produced just after
inflation and thermal relics of LSPs. Significant amount of gravitinos are also
pair-produced at the decay, which subsequently decay into the neutralinos. We
identify the regions of the parameter space in which the requisite abundance of
the neutralino dark matter is obtained without spoiling the big-bang
nucleosynthesis by injection of hadronic showers from gravitino decay. The
neutralino abundance obtained in this mechanism is insensitive to the details
of the superparticle mass spectrum, unlike the standard thermal abundance. We
also briefly mention the testability of the scenario in future experiments.Comment: 19 pages, 5 figures, to appear in Phys. Rev.
Solving the cosmic lithium problems with primordial late-decaying particles
We investigate the modifications to predictions for the abundances of light
elements from standard Big-Bang nucleosynthesis when exotic late-decaying
particles with lifetimes exceeding ~1 sec are prominent in the early Universe.
Utilising a model-independent analysis of the properties of these long-lived
particles, we identify the parameter space associated with models that are
consistent with all observational data and hence resolve the much discussed
discrepancies between observations and theoretical predictions for the
abundances of Li^7 and Li^6.Comment: 6 pages, 3 figures, submitted to Physical Review D; minor changes to
reference
Big Bang Nucleosynthesis with Long Lived Charged Massive Particles
We consider Big Bang Nucleosynthesis (BBN) with long lived charged massive
particles. Before decaying, the long lived charged particle recombines with a
light element to form a bound state like a hydrogen atom. This effect modifies
the nuclear reaction rates during the BBN epoch through the modifications of
the Coulomb field and the kinematics of the captured light elements, which can
change the light element abundances. It is possible that the heavier nuclei
abundances such as Li and Be decrease sizably, while the ratios ,
D/H, and He/H remain unchanged. This may solve the current discrepancy
between the BBN prediction and the observed abundance of Li. If future
collider experiments found signals of a long-lived charged particle inside the
detector, the information of its lifetime and decay properties could provide
insights to understand not only the particle physics models but also the
phenomena in the early universe in turn.Comment: 20 pages, 6 figures, published version in Physical Review
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