246 research outputs found
F-theory and the Witten Index
We connect the fermionic fields, localized on the intersection curve
of two D7-branes with zero background flux, to a N=2 supersymmetric quantum
mechanics algebra, within the theoretical framework of F-theory
F-theory Yukawa Couplings and Supersymmetric Quantum Mechanics
The localized fermions on the intersection curve of D7-branes, are
connected to a N=2 supersymmetric quantum mechanics algebra. Due to this
algebra the fields obey a global U(1) symmetry. This symmetry restricts the
proton decay operators and the neutrino mass terms. Particularly, we find that
several proton decay operators are forbidden and the Majorana mass term is the
only one allowed in the theory. A special SUSY QM algebra is studied at the end
of the paper. In addition we study the impact of a non-trivial holomorphic
metric perturbation on the localized solutions along each matter curve.
Moreover, we study the connection of the localized solutions to an N=2
supersymmetric quantum mechanics algebra when background fluxes are turned on.Comment: References added, New Material Added, Published versio
Excitation spectrum of vortex lattices in rotating Bose-Einstein condensates
Using the coarse grain averaged hydrodynamic approach, we calculate the
excitation spectrum of vortex lattices sustained in rotating Bose-Einstein
condensates. The spectrum gives the frequencies of the common-mode longitudinal
waves in the hydrodynamic regime, including those of the higher-order
compressional modes. Reasonable agreement with the measurements taken in a
recent JILA experiment is found, suggesting that one of the longitudinal modes
reported in the experiment is likely to be the , mode.Comment: 2 figures. Submitted to Physical Review A. v2 contains more
references. No change in the main resul
Upper critical field in dirty two-band superconductors: breakdown of the anisotropic Ginzburg-Landau theory
We investigate the upper critical field in a dirty two-band superconductor
within quasiclassical Usadel equations. The regime of very high anisotropy in
the quasi-2D band, relevant for MgB, is considered. We show that strong
disparities in pairing interactions and diffusion constant anisotropies for two
bands influence the in-plane in a different way at high and low
temperatures. This causes temperature-dependent anisotropy, in
accordance with recent experimental data in MgB. The three-dimensional
band most strongly influences the in-plane near , in the
Ginzburg-Landau (GL) region. However, due to a very large difference between
the c-axis coherence lengths in the two bands, the GL theory is applicable only
in an extremely narrow temperature range near . The angular dependence of
deviates from a simple effective-mass law even near .Comment: 12 pages, 5 figures, submitted to Phys.Rev.
Ecological and cultural factors underlying the global distribution of prejudice
Prejudiced attitudes and political nationalism vary widely around the world, but there has
been little research on what predicts this variation. Here we examine the ecological and cultural factors underlying the worldwide distribution of prejudice. We suggest that cultures
grow more prejudiced when they tighten cultural norms in response to destabilizing ecological threats. A set of seven archival analyses, surveys, and experiments (âN = 3,986,402)
find that nations, American states, and pre-industrial societies with tighter cultural norms
show the most prejudice based on skin color, religion, nationality, and sexuality, and that
tightness predicts why prejudice is often highest in areas of the world with histories of ecological threat. Peopleâs support for cultural tightness also mediates the link between perceived ecological threat and intentions to vote for nationalist politicians. Results replicate
when controlling for economic development, inequality, conservatism, residential mobility,
and shared cultural heritage. These findings offer a cultural evolutionary perspective on prejudice, with implications for immigration, intercultural conflict, and radicalization.publishedVersio
Dimerization and Fusion of two C60 Molecules
We investigate the dimerization and fusion of C60 molecules to form various
C60 dimers when pushed against each other at several inter-molecular distances.
We study the stability of this dimerized C60 molecule based on its binding
strength provided by intramolecular interactions. Tersoff potential, which is
considered to represent intramolecular interactions well, has been used to
calculate potential energy at these distances of separation and for all
possible orientations of the molecules. We observe that several minimum energy
configurations exist at various distances between the C60 molecules. Our
calculation shows that apart from the dumbbell structures, many interesting
composite phases also result, such as fused, peanut and carbon nanotubes of
geometry (5,5) and (10,0) of certain specific length.Comment: 18 pages and 8 figure
Aveiro discretization method in mathematics: a new discretization principle
We found a very general discretization method for solving wide classes of mathematical problems by applying the theory of reproducing kernels. An illustration of the generality of the method is here performed by considering several distinct classes of problems to which the method is applied. In fact, one of the advantages of the present method -- in comparison to other well-known and well established methods -- is its global nature and no need of special or very particular data conditions. Numerical experiments have been made, and consequent results are here exhibited.
Due to the powerful results which arise from the application of the present method, we consider that this method has everything to become one of the next generation methods of solving general analytical problems by using computers. In particular, we would like to point out that we will be able to solve very global linear partial differential equations satisfying very general boundary conditions or initial values (and in a somehow independent way of the boundary and domain). Furthermore, we will be able to give an ultimate sampling theory and an ultimate realization of the consequent general reproducing kernel Hilbert spaces. The general theory is here presented in a constructive way, and containing some related historical and concrete examples
Doing synthetic biology with photosynthetic microorganisms
The use of photosynthetic microbes as synthetic biology hosts for the sustainable production of commodity chemicals and even fuels has received increasing attention over the last decade. The number of studies published, tools implemented, and resources made available for microalgae have increased beyond expectations during the last few years. However, the tools available for genetic engineering in these organisms still lag those available for the more commonly used heterotrophic host organisms. In this mini-review, we provide an overview of the photosynthetic microbes most commonly used in synthetic biology studies, namely cyanobacteria, chlorophytes, eustigmatophytes and diatoms. We provide basic information on the techniques and tools available for each model group of organisms, we outline the state-of-the-art, and we list the synthetic biology tools that have been successfully used. We specifically focus on the latest CRISPR developments, as we believe that precision editing and advanced genetic engineering tools will be pivotal to the advancement of the field. Finally, we discuss the relative strengths and weaknesses of each group of organisms and examine the challenges that need to be overcome to achieve their synthetic biology potential.Peer reviewe
Galaxy Clusters Associated with Short GRBs. II. Predictions for the Rate of Short GRBs in Field and Cluster Early-Type Galaxies
We determine the relative rates of short GRBs in cluster and field early-type
galaxies as a function of the age probability distribution of their
progenitors, P(\tau) \propto \tau^n. This analysis takes advantage of the
difference in the growth of stellar mass in clusters and in the field, which
arises from the combined effects of the galaxy stellar mass function, the
early-type fraction, and the dependence of star formation history on mass and
environment. This approach complements the use of the early- to late-type host
galaxy ratio, with the added benefit that the star formation histories of
early-type galaxies are simpler than those of late-type galaxies, and any
systematic differences between progenitors in early- and late-type galaxies are
removed. We find that the ratio varies from R(cluster)/R(field) ~ 0.5 for n =
-2 to ~ 3 for n = 2. Current observations indicate a ratio of about 2,
corresponding to n ~ 0 - 1. This is similar to the value inferred from the
ratio of short GRBs in early- and late-type hosts, but it differs from the
value of n ~ -1 for NS binaries in the Milky Way. We stress that this general
approach can be easily modified with improved knowledge of the effects of
environment and mass on the build-up of stellar mass, as well as the effect of
globular clusters on the short GRB rate. It can also be used to assess the age
distribution of Type Ia supernova progenitors.Comment: ApJ accepted versio
- âŠ