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Background: Panic disorder is common (5% prevalence) and females are twice as likely to be affected as males. The heritable component of panic disorder is estimated at 48%. Glutamic acid dehydrogenase GAD1, the key enzyme for the synthesis of the inhibitory and anxiolytic neurotransmitter GABA, is supposed to influence various mental disorders, including mood and anxiety disorders. In a recent association study in depression, which is highly comorbid with panic disorder, GAD1 risk allele associations were restricted to females.
Methodology/Principal Findings: Nineteen single nucleotide polymorphisms (SNPs) tagging the common variation in GAD1 were genotyped in two independent gender and age matched case-control samples (discovery sample n = 478; replication sample n = 584). Thirteen SNPs passed quality control and were examined for gender-specific enrichment of risk alleles associated with panic disorder by using logistic regression including a genotype×gender interaction term. The latter was found to be nominally significant for four SNPs (rs1978340, rs3762555, rs3749034, rs2241165) in the discovery sample; of note, the respective minor/risk alleles were associated with panic disorder only in females. These findings were not confirmed in the replication sample; however, the genotype×gender interaction of rs3749034 remained significant in the combined sample. Furthermore, this polymorphism showed a nominally significant association with the Agoraphobic Cognitions Questionnaire sum score.
Conclusions/Significance: The present study represents the first systematic evaluation of gender-specific enrichment of risk alleles of the common SNP variation in the panic disorder candidate gene GAD1. Our tentative results provide a possible explanation for the higher susceptibility of females to panic disorder.
Der langsame Neutronen-Einfangprozess (s-Prozess) ist weitgehend verstanden und erforscht. Dies liegt vor allem daran, dass er im Gegensatz zu r- und p- Prozess hauptsächlich an stabilen Nukliden abläuft. Auch ist die Anzahl relevanter Reaktionen (Netzwerk) vergleichsweise klein.
Dennoch gibt es im s-Prozess viele ungeklärte Fragen. Eine dieser Fragen ist die Häufigkeitsverteilung von 86Kr in Staubkörnern von Meteoriten. Mit bisherigen Berechnungen und Simulationen dieser Szenarien konnte die Häufigkeitsverteilung von 86Kr jedoch nicht erklärt werden.
In dieser Arbeit werden die besonderen Eigenschaften von 85Kr, insbesondere sein Isomerzustand, vorgestellt und genauer untersucht. Die Häufigkeitsverteilung von 86Kr im s-Prozess wird entscheidend durch die Eigenschaften 85Kr beeinflusst. Mit den gewonnenen Daten aus dieser Arbeit wurde eine erste Simulation erstellt, die einen möglichenWeg aufzeigt, das Rätsel um die Häufigkeitsverteilung zu lösen.
XIII Nuclei in the Cosmos, 7-11 July, 2014 Debrecen, Hungary.
As an alternative production scenario to the so-called g process, the most abundant p nucleus 92Mo may be produced by a chain of proton-capture reactions in supernovae type Ia. The reactions 90Zr(p,g) and 91Nb(p,g) are the most important reactions in this chain. We have measured the first reaction using high-resolution in-beam g-spectroscopy at HORUS, Cologne, Germany, to contribute to the existing experimental data base. So far, we only investigated the high-energy part of the Gamow window and the analysis is still in progress. We plan to study the second reaction in standard kinematics at the FRANZ facility, Frankfurt, Germany. Current developments at FRANZ will be explained in detail.
p-process nucleosynthesis via proton-capture reactions in thermonuclear supernovae explosions
(2015)
Model calculations within the framework of the so-called γ process show an underproduction of the p nucleus with the highest isotopic abundace 92Mo. This discrepancy can be narrowed by taking into account the alternative production site of a type Ia supernova explosion. Here, the nucleus 92Mo can be produced by a sequence of proton-capture reactions. The amount of 92Mo nuclei produced via this reaction chain is most sensitive to the reactions 90Zr(p,γ) and 91Nb(p,γ). Both rates have to be investigated experimentally to study the impact of this nucleosynthesis aspect on the long-standing 92Mo-problem. We have already measured the proton-capture reaction on 90Zr using high-resolution in-beam γ-ray spectroscopy. In this contribution, we will present our preliminary results of the total cross sections as well as the partial cross sections. Furthermore, we plan to measure the 91Nb(p,γ) reaction soon. Due to the radioactive target material, the 91Nb nuclei have to be produced prior to the experiment. The current status of this production will be presented in this contribution.
The p nucleus 92Mo is believed to be mainly produced through photodisintegration reactions in type II supernovae. However, this production scenario cannot solely account for the observed solar relative isotopic abundance of 92Mo. Additional production scenarios have been suggested to explain this discrepancy. One of these scenarios could be the production of 92Mo in type Ia supernovae via a chain of proton-capture reactions. To verify this scenario, an accurate knowledge of the involved reaction rates is important. We measured the cross section of 90Zr(p,γ) reaction using an enriched 90Zr target by means of in-beam γ-ray spectroscopy in the energy range between 3.6MeV and 5.1MeV. Since the reactions 90Zr(p,γ) and 91Zr(p,n) produce the same nucleus, the contributions of both reactions have to be disentangled. This procedure is explained in this contribution in detail.
The production of 77,79,85,85mKr and 77Br via the reaction Se(a, x) was investigated between Ea = 11 and 15 MeV using the activation technique. The irradiation of natural selenium targets on aluminum backings was conducted at the Physikalisch-Technische Bundesanstalt (PTB) in Braunschweig, Germany. The spectroscopic analysis of the reaction products was performed using a high-purity germanium detector located at PTB and a low energy photon spectrometer detector at the Goethe University Frankfurt, Germany. Thicktarget yields were determined. The corresponding energy-dependent production cross sections of 77,79,85,85mKr and 77Br were calculated from the thicktarget yields. Good agreement between experimental data and theoretical predictions using the TALYS-1.6 code was found.
Based on neurofeedback (NF) training as a neurocognitive treatment in attention-deficit/hyperactivity disorder (ADHD), we designed a randomized, controlled functional near-infrared spectroscopy (fNIRS) NF intervention embedded in an immersive virtual reality classroom in which participants learned to control overhead lighting with their dorsolateral prefrontal brain activation. We tested the efficacy of the intervention on healthy adults displaying high impulsivity as a sub-clinical population sharing common features with ADHD. Twenty participants, 10 in an experimental and 10 in a shoulder muscle-based electromyography control group, underwent eight training sessions across 2 weeks. Training was bookended by a pre- and post-test including go/no-go, n-back, and stop-signal tasks (SST). Results indicated a significant reduction in commission errors on the no-go task with a simultaneous increase in prefrontal oxygenated hemoglobin concentration for the experimental group, but not for the control group. Furthermore, the ability of the subjects to gain control over the feedback parameter correlated strongly with the reduction in commission errors for the experimental, but not for the control group, indicating the potential importance of learning feedback control in moderating behavioral outcomes. In addition, participants of the fNIRS group showed a reduction in reaction time variability on the SST. Results indicate a clear effect of our NF intervention in reducing impulsive behavior possibly via a strengthening of frontal lobe functioning. Virtual reality additions to conventional NF may be one way to improve the ecological validity and symptom-relevance of the training situation, hence positively affecting transfer of acquired skills to real life.
The 124Xe(p,γ) reaction has been measured for the first time at energies around the Gamow window by using stored ions at the ESR facility. The desired beam energies below 10 MeV/u introduce new experimental challenges like windowless ions detection under UHV conditions, extremely short beam lifetimes and efficient beam deceleration and cooling, all of which have been successfully met.
Most of the elements in the universe are produced via charged-particle fusion reactions during the primordial nucleosynthesis and different stellar burning stages, as well as via neutron-capture reactions. Around 35 heavy, proton-rich isotopes are bypassed by those reaction paths, the p nuclei. A series of photo-disintegration reactions occurring in supernovae, called the γ process, was suggested as a mechanisms to produce the p nuclei. Numerical simulations of the γ process have been unable to reproduce the observed abundances of the light p isotopes. Recent models showed that a series of proton capture reactions could provide the observed abundances. Hence, the cross sections of the crucial capture reactions have to be measured in order to test those assumptions.
Radiative proton captures in addition to the γ-process could reproduce the observed abundance pattern. This thesis presents preparations of a proton capture measurement on the radioactive 91Nb in standard kinematics with a calorimetric 4π setup. The 91Nb(p,γ)92Mo reaction might be the key to explain the production of one of the most abundant p-nuclei, 92Mo. So far, no experimental data for this reaction is available.
We produced a sample of 91Nb, with a half-life of 680 yr, at the Physikalisch Technische Bundesanstalt in Braunschweig, Germany, by irradiating 92Mo with protons in the energy range of 12 – 20MeV. 91Nb was produced via the reaction 92Mo(p,2p)91Nb and via 92Mo(p,pn)91Mo, where 91Mo decays to 91Nb with a half-life of 15.5min. To predict the amount of produced 91Nb the cross section of 92Mo(p, 2p) was measured. It was found to be higher than the value given by theoretical calculations with TALYS. Finally, 91Nb was chemically separated from the molybdenum carried at Paul-Scherrer- Institut, Villigen, Switzerland.
In-beam total absorption cross-section measurement of the reaction 91Nb(p,γ)92Mo with 2 MeV protons at FRANZ is planed with the produced 91Nb. A 4π BaF2 detector consisting of 41 crystals will be used. During this experiment we will measure the sum energy and the multiplicity of each event. The freshly produced 91Nb constitutes only a minor component of the sample material. The sum energy and multiplicity are crucial to distinguish the desired 91Nb(p,γ) from all the other more dominant reactions. The expected multiplicity and the efficiency of the setup were carefully simulated with DICEBOX and GEANT4. It was possible to show that background reactions can be effectively suppressed. The most important background contributions could be identified and result from 92Mo(p,γ), 19F(p,γ), and 19F(p,α).
Background: Bidirectional promoters (BPs) are prevalent in eukaryotic genomes. However, it is poorly understood how the cell integrates different epigenomic information, such as transcription factor (TF) binding and chromatin marks, to drive gene expression at BPs. Single-cell sequencing technologies are revolutionizing the field of genome biology. Therefore, this study focuses on the integration of single-cell RNA-seq data with bulk ChIP-seq and other epigenetics data, for which single-cell technologies are not yet established, in the context of BPs.
Results: We performed integrative analyses of novel human single-cell RNA-seq (scRNA-seq) data with bulk ChIP-seq and other epigenetics data. scRNA-seq data revealed distinct transcription states of BPs that were previously not recognized. We find associations between these transcription states to distinct patterns in structural gene features, DNA accessibility, histone modification, DNA methylation and TF binding profiles.
Conclusions: Our results suggest that a complex interplay of all of these elements is required to achieve BP-specific transcriptional output in this specialized promoter configuration. Further, our study implies that novel statistical methods can be developed to deconvolute masked subpopulations of cells measured with different bulk epigenomic assays using scRNA-seq data.