Vortices on Higher Genus Surfaces

We consider the topological interactions of vortices on general surfaces. If the genus of the surface is greater than zero, the handles can carry magnetic flux. The classical state of the vortices and the handles can be described by a mapping from the fundamental group to the unbroken gauge group. The allowed configurations must satisfy a relation induced by the fundamental group. Upon quantization, the handles can carry ``Cheshire charge.'' The motion of the vortices can be described by the braid group of the surface. How the motion of the vortices affects the state is analyzed in detail.Comment: 28 pages with 10 figures; uses phyzzx and psfig; Caltech preprint CALT-68-187

Observation of the 0+ 2 and γ bands in 98Ru, and shape coexistence in the Ru isotopes

Excited states in 98Ru were investigated using γ-ray spectroscopy following the β-decay of 98Rh, and via the 100Ru(p,t) reaction. Combining the results from the two experiments, two states were revised to have spin-parity of 4+ and subsequently assigned to the 02+ and “γ” bands, respectively. The observed structures in 98Ru are suggested to be deformed and rotational, rather than spherical and vibrational, and fit well into the systematics of these excitations in the Ru isotopes. The 02+ excitation is suggested as a shape coexisting configuration. This observation eliminates some of the last remaining candidates for nearly harmonic vibrational nuclei in the Z≈50 region. Beyond-mean-field calculations are presented that support shape coexistence throughout the Ru isotopes with N=52–62, and suggest a smooth evolution of the shape

Planck-scale quintessence and the physics of structure formation

In a recent paper we considered the possibility of a scalar field providing an explanation for the cosmic acceleration. Our model had the interesting properties of attractor-like behavior and having its parameters of O(1) in Planck units. Here we discuss the effect of the field on large scale structure and CMB anisotropies. We show how some versions of our model inspired by "brane" physics have novel features due to the fact that the scalar field has a significant role over a wider range of redshifts than for typical "dark energy" models. One of these features is the additional suppression of the formation of large scale structure, as compared with cosmological constant models. In light of the new pressures being placed on cosmological parameters (in particular H_0) by CMB data, this added suppression allows our "brane" models to give excellent fits to both CMB and large scale structure data.Comment: 18 pages, 12 figures, submitted to PR

High resolution 148Nd(3He,nγ) two proton stripping reaction and the structure of the 02 + state in 150Sm

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Study of 0+ States at iThemba LABS

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First application of the Oslo method in inverse kinematics

International audienceThe $\gamma$-ray strength function ($\gamma$SF) and nuclear level density (NLD) have been extracted for the first time from inverse kinematic reactions with the Oslo method. This novel technique allows measurements of these properties across a wide range of previously inaccessible nuclei. Proton–$\gamma$ coincidence events from the $\mathrm {d}(^{86}\mathrm {Kr}, \mathrm {p}\gamma )^{87}\mathrm {Kr}$ reaction were measured at iThemba LABS and the $\gamma$SF and NLD in $^{87}\mathrm {Kr}$ was obtained. The low-energy region of the $\gamma$SF is compared to shell-model calculations, which suggest this region to be dominated by M1 strength. The $\gamma$SF and NLD are used as input parameters to Hauser–Feshbach calculations to constrain $(\mathrm {n},\gamma )$ cross sections of nuclei using the TALYS reaction code. These results are compared to $^{86}\mathrm {Kr}(n,\gamma )$ data from direct measurements

Nuclear level densities and γ\gamma-ray strength functions of 87Kr^{87}\mathrm{Kr} -- First application of the Oslo Method in inverse kinematics

The $\gamma$-ray strength function ($\gamma$SF) and nuclear level density (NLD) have been extracted for the first time from inverse kinematic reactions with the Oslo Method. This novel technique allows measurements of these properties across a wide range of previously inaccessible nuclei. Proton-$\gamma$ coincidence events from the $\mathrm{d}(^{86}\mathrm{Kr}, \mathrm{p}\gamma)^{87}\mathrm{Kr}$ reaction were measured at iThemba LABS and the $\gamma$SF and NLD in $^{87}\mathrm{Kr}$ obtained. The low-energy region of the $\gamma$SF is compared to Shell Model calculations which suggest this region to be dominated by M1 strength. The $\gamma$SF and NLD are used as input parameters to Hauser-Feshbach calculations to constrain $(\mathrm{n},\gamma)$ cross sections of nuclei using the TALYS reaction code. These results are compared to $^{86}\mathrm{Kr}(n,\gamma)$ data from direct measurements

Fruit Distribution in the Canadian West

Transcription factors, by binding to particular DNA sequences termed transcription factor-binding sites, play an important role in regulating gene expression in both prokaryotic and eukaryotic organisms. These binding sites lie within promoters (which are located just upstream of a gene and promote transcription of that gene) and enhancers (short DNA elements enhancing transcription levels of genes in a gene cluster, and which need not be particularly close to the genes they act on, or even located on the same chromosome). Binding of transcription factors in these genomic regulatory regions can influence gene transcription rates either positively or negatively. The binding may also be dependant on the interaction with co-activators and co-repressors, in addition to context (e.g. particular histone modifications in the vicinity of the regulatory element). Identifying all transcription factors and their respective binding sites would be an important step towards a more thorough understanding of gene regulation. Regular expression type patterns, as well as nucleotide distribution matrices, have both been used for describing transcription factor-binding sites, e.g. (Bucher 1990; Ghosh 1990; Chen et al. 1995; Wingender et al. 1996). Here we will discuss some of the computational approaches that are used in binding site identification.SCOPUS: ch.binfo:eu-repo/semantics/publishe

Low-spin states in <math><mmultiscripts><mi>Sn</mi><mprescripts/><none/><mn>118</mn></mmultiscripts></math> populated by the radiative capture of thermal neutrons

International audienceBackground: γ-ray spectroscopy studies of the Sn isotopes provide important information on nuclear structure and shell evolution across the long isotopic chain between the doubly-magic Sn100 and Sn132 nuclei. These studies also offer great value to test and tune nuclear models which can then be applied to other regions of the nuclear chart.Purpose: We aim to expand the level scheme of Sn118 by populating low-spin states in the range of 3–5 MeV and determine their angular momentum for the possible connection of these states to pygmy quadrupole Resonances, a new phenomenon observed in the neighboring Sn112,114,124 isotopes as a resonance-like structure in the 3–5 MeV range.Method: Excited states in Sn118 were populated via the Sn117(n,γ)Sn118 reaction at the Institut Laue-Langevin in Grenoble, France. The FIssion Product Prompt gamma-ray Spectrometer (FIPPS), an array of eight n-type high purity Germanium clover detectors augmented with eight additional clover detectors from IFIN “Horia Hulubei” were used to detect γ rays from excited states in Sn118. The array provides a superior efficiency for γ-ray detection and nearly 4π coverage for the measurements of angular correlations for spin assignment of excited nuclear levels.Results: Through γ-γ coincidences, 112 excited states were identified with 57 being newly placed in the level scheme. From these states, 567 γ-ray transitions were observed with 501 being newly identified. Many levels were identified in the 3–5 MeV region. Further, an indirect measurement of the E0 transition which decays from the 03+ state to the 2p-2h, 02+ state was performed and the qK2(E0/E2) and X(E0/E2) for this transition were determined to be 12.7(11) and 6.3(5), respectively. The 103×ρ2(E0) was determined to be &gt;38 based on a half-life limit of &lt;200 ps of the 2057-keV, 03+ level.Conclusions: The abundant spectroscopic information on Sn118 obtained in the present experiment is an important input to the theoretical description of nuclei in the region and highlights the capabilities of the FIPPS array at ILL in conjunction with neutron capture reactions. Many states identified in the 3–5 MeV region could very likely have J=2+ and contribute to the pygmy quadrupole resonances