24 research outputs found
New results on catalyzed BBN with a long-lived negatively-charged massive particle
It has been proposed that the apparent discrepancies between the inferred
primordial abundances of 6Li and 7Li and the predictions of big bang
nucleosynthesis (BBN) can be resolved by the existence of a negatively-charged
massive unstable supersymmetric particle (X-) during the BBN epoch. Here, we
present new BBN calculations with an X- particle utilizing an improved nuclear
reaction network including captures of nuclei by the particle, nuclear
reactions and beta-decays of normal nuclei and nuclei bound to the X- particles
(X-nuclei), and new reaction rates derived from recent rigorous quantum
many-body dynamical calculations. We find that this is still a viable model to
explain the observed 6Li and 7Li abundances. However, contrary to previous
results, neutral X-nuclei cannot significantly affect the BBN light-element
abundances. We also show that with the new rates the production of heavier
nuclei is suppressed and there is no signature on abundances of nuclei heavier
than Be in the X--particle catalyzed BBN model as has been previously proposed.
We also consider the version of this model whereby the X- particle decays into
the present cold dark matter. We analyze the this paradigm in light of the
recent constraints on the dark-matter mass deduced from the possible detected
events in the CDMS-II experiment. We conclude that based upon the inferred
range for the dark-matter mass, only X- decay via the weak interaction can
achieve the desired 7Li destruction while also reproducing the observed 6Li
abundance.Comment: 6 pages, 2 figure
Effect of Long-lived Strongly Interacting Relic Particles on Big Bang Nucleosynthesis
It has been suggested that relic long-lived strongly interacting massive
particles (SIMPs, or particles) existed in the early universe. We study
effects of such long-lived unstable SIMPs on big bang nucleosynthesis (BBN)
assuming that such particles existed during the BBN epoch, but then decayed
long before they could be detected. The interaction strength between an
particle and a nucleon is assumed to be similar to that between nucleons. We
then calculate BBN in the presence of the unstable neutral charged
particles taking into account the capture of particles by nuclei to form
-nuclei. We also study the nuclear reactions and beta decays of -nuclei.
We find that SIMPs form bound states with normal nuclei during a relatively
early epoch of BBN. This leads to the production of heavy elements which remain
attached to them. Constraints on the abundance of particles during BBN
are derived from observationally inferred limits on the primordial light
element abundances. Particle models which predict long-lived colored particles
with lifetimes longer than 200 s are rejected based upon these
constraints.Comment: 19 pages, 4 figure
Big Bang Nucleosynthesis Constraints on Hadronically and Electromagnetically Decaying Relic Neutral Particles
Big Bang nucleosynthesis in the presence of decaying relic neutral particles
is examined in detail. All non-thermal processes important for the
determination of light-element abundance yields of 2H, 3H, 3He, 4He, 6Li, and
7Li are coupled to the thermonuclear fusion reactions to obtain comparatively
accurate results. Predicted light-element yields are compared to
observationally inferred limits on primordial light-element abundances to infer
constraints on the abundances and properties of relic decaying particles with
decay times in the interval 0.01 sec < tau < 10^(12) sec. Decaying particles
are typically constrained at early times by 4He or 2H, at intermediate times by
6Li, and at large times by the 3He/2H ratio. Constraints are shown for a large
number of hadronic branching ratios and decaying particle masses and may be
applied to constrain the evolution of the early Universe.Comment: 24 pages (revtex), 11 figures, title changed, matches published
versio
Big Bang Nucleosynthesis with Bound States of Long-lived Charged Particles
Charged particles (X) decaying after primordial nucleosynthesis are
constrained by the requirement that their decay products should not change the
light element abundances drastically. If the decaying particle is negatively
charged (X-) then it will bind to the nuclei. We consider the effects of the
decay of X when bound to Helium-4 and show that this will modify the Lithium
abundances.Comment: 5 pages; v2: references added, figure caption corrected; v3:
references adde
Strong Interactive Massive Particles from a Strong Coupled Theory
Minimal walking technicolor models can provide a nontrivial solution for
cosmological dark matter, if the lightest technibaryon is doubly charged.
Technibaryon asymmetry generated in the early Universe is related to baryon
asymmetry and it is possible to create excess of techniparticles with charge
(-2). These excessive techniparticles are all captured by , creating
\emph{techni-O-helium} ``atoms'', as soon as is formed in Big
Bang Nucleosynthesis. The interaction of techni-O-helium with nuclei opens new
paths to the creation of heavy nuclei in Big Bang Nucleosynthesis. Due to the
large mass of technibaryons, the ``atomic'' gas decouples from the
baryonic matter and plays the role of dark matter in large scale structure
formation, while structures in small scales are suppressed. Nuclear
interactions with matter slow down cosmic techni-O-helium in Earth below the
threshold of underground dark matter detectors, thus escaping severe CDMS
constraints. On the other hand, these nuclear interactions are not sufficiently
strong to exclude this form of Strongly Interactive Massive Particles by
constraints from the XQC experiment. Experimental tests of this hypothesis are
possible in search for in balloon-borne experiments (or on the ground)
and for its charged techniparticle constituents in cosmic rays and
accelerators. The ``atoms'' can cause cold nuclear transformations in
matter and might form anomalous isotopes, offering possible ways to exclude (or
prove?) their existence.Comment: 41 pages, 4 figure
A Cosmological Model with Dark Spinor Source
In this paper, we discuss the system of Friedman-Robertson-Walker metric
coupling with massive nonlinear dark spinors in detail, where the thermodynamic
movement of spinors is also taken into account. The results show that, the
nonlinear potential of the spinor field can provide a tiny negative pressure,
which resists the Universe to become singular. The solution is oscillating in
time and closed in space, which approximately takes the following form
g_{\mu\nu}=\bar R^2(1-\delta\cos t)^2\diag(1,-1,-\sin^2r ,-\sin^2r
\sin^2\theta), with light year, and
. The present time is about .Comment: 13 pages, no figure, to appear in IJMP
Dark matter with invisible light from heavy double charged leptons of almost-commutative geometry?
A new candidate of cold dark matter arises by a novel elementary particle
model: the almostcommutative AC-geometrical framework. Two heavy leptons are
added to the Standard Model, each one sharing a double opposite electric charge
and an own lepton flavor number The novel mathematical theory of
almost-commutative geometry [1] wishes to unify gauge models with gravity. In
this scenario two new heavy (m_L>100GeV), oppositely double charged leptons
(A,C),(A with charge -2 and C with charge +2), are born with no twin quark
companions. The model naturally involves a new U(1) gauge interaction,
possessed only by the AC-leptons and providing a Coulomblike attraction between
them. AC-leptons posses electro-magnetic as well as Z-boson interaction and,
according to the charge chosen for the new U(1) gauge interaction, a new
"invisible light" interaction. Their final cosmic relics are bounded into
"neutral" stable atoms (AC) forming the mysterious cold dark matter, in the
spirit of the Glashow's Sinister model. An (AC) state is reached in the early
Universe along a tail of a few secondary frozen exotic components. They should
be now here somehow hidden in the surrounding matter. The two main secondary
manifest relics are C (mostly hidden in a neutral (Cee) "anomalous helium"
atom, at a 10-8 ratio) and a corresponding "ion" A bounded with an ordinary
helium ion (4He); indeed the positive helium ions are able to attract and
capture the free A fixing them into a neutral relic cage that has nuclear
interaction (4HeA).Comment: This paper has been merged with [astro-ph/0603187] for publication in
Classical and Quantum Gravit
Improvement of microwave equipment excitation efficiency using methods of focused arrays
The problem of multielement excitation of exposed-type microwave equipment is studied. Optimization problem is formulated as amplitudes, phases and elements location definition to maximize the special efficiency criteria. Both coherent and noncoherent multielement excitation are considered. Substantial improvement of microwave field excitation can be achieved by proposed approach. A number of particular optimization procedures advantageous for practical use is presented