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Aim: Replicate the analysis conducted by Prof. Dr. Alexander W. Schmidt-Catran (Goethe University Frankfurt), Prof. Dr. Malcolm Fairbrother (Umea University), and Prof. Dr. Hans-Jürgen Andreß (University of Cologne) that was published in a special issue on Cross-National Comparative Research in the German academic journal Kölner Zeitschrift für Soziologie und Sozialpsychologie in 2019. Result: Almost all calculations, tables and graphs from Schmidt-Catran et al. (2019) could be replicated sufficiently well in R.
The equation of state (EoS) of matter at extremely high temperatures and densities is currently not fully understood, and remains a major challenge in the field of nuclear physics. Neutron stars harbor such extreme conditions and therefore serve as celestial laboratories for constraining the dense matter EoS. In this thesis, we present a novel algorithm that utilizes the idea of Bayesian analysis and the computational efficiency of neural networks to reconstruct the dense matter equation of state from mass-radius observations of neutron stars. We show that the results are compatible with those from earlier works based on conventional methods, and are in agreement with the limits on tidal deformabilities obtained from the gravitational wave event, GW170817. We also observe that the resulting squared speed of sound from the reconstructed EoS features a peak, indicating a likely convergence to the conformal limit at asymptotic densities, as expected from quantum chromodynamics. The novel algorithm can also be applied across various fields faced with computational challenges in solving inverse problems. We further examine the efficiency of deep learning methods for analyzing gravitational waves from compact binary coalescences in this thesis. In particular, we develop a deep learning classifier to segregate simulated gravitational wave data into three classes: signals from binary black hole mergers, signals from binary neutron star mergers, or white noise without any signals. A second deep learning algorithm allows for the regression of chirp mass and combined tidal deformability from simulated binary neutron star mergers. An accurate estimation of these parameters is crucial to constrain the underlying EoS. Lastly, we explore the effects of finite temperatures on the binary neutron star merger remnant from GW170817. Isentropic EoSs are used to infer the frequencies of the rigidly rotating remnant and are noted to be significantly lower compared to previous estimates from zero temperature EoSs. Overall, this thesis presents novel deep learning methods to constrain the neutron star EoS, which will prove useful in future, as more observational data is expected in the upcoming years.
After myocardial infarction in the adult heart the remaining, non-infarcted tissue adapts to compensate the loss of functional tissue. This adaptation requires changes in gene expression networks, which are mostly controlled by transcription regulating proteins. Long non-coding transcripts (lncRNAs) are taking part in fine-tuning such gene programs. We describe and characterize the cardiomyocyte specific lncRNA Sweetheart RNA (Swhtr), an approximately 10 kb long transcript divergently expressed from the cardiac core transcription factor coding gene Nkx2-5. We show that Swhtr is dispensable for normal heart development and function but becomes essential for the tissue adaptation process after myocardial infarction in murine males. Re-expressing Swhtr from an exogenous locus rescues the Swhtr null phenotype. Genes that depend on Swhtr after cardiac stress are significantly occupied and therefore most likely regulated by NKX2-5. The Swhtr transcript interacts with NKX2-5 and disperses upon hypoxic stress in cardiomyocytes, indicating an auxiliary role of Swhtr for NKX2-5 function in tissue adaptation after myocardial injury.
Diese Versuchsreihe beschäftigte sich mit der Fragestellung, ob günstige Handelsmarken- Zigaretten mehr Feinstaub als teure Markenzigaretten emittieren. Dabei wurde der Passivrauch untersucht, welcher durch das Verrauchen verschiedener Zigarettenmarken entstand. Feinstaub stellt heutzutage den wichtigsten einzelnen gesundheitsschädlichen Faktor in Innenräumen dar. Das Augenmerk liegt dabei hauptsächlich auf den feinen Partikeln (PM2,5, PM1). Tumore, chronische Atemwegserkrankungen und eine erhöhte Mortalität stellen nur einen Teil der massiven gesundheitlichen Folgen durch Feinstaub dar. Vulnerable Bevölkerungsgruppen wie Kinder und alte Personen sind besonders durch Passivrauch gefährdet. Die Ergebnisse der Versuchsreihe dienen als Grundlage, um den gesundheitsschädlichen Einfluss des Passivrauchs zu interpretieren. Günstige Handelsmarken-Zigaretten weisen, unter anderem wegen des beständig ansteigenden Zigarettenpreises als auch der anhaltenden Inflation in Deutschland, einen wachsenden Marktanteil auf. Daher müssen sie auch weiterhin in wissenschaftlichen Untersuchungen mit einbezogen werden.
Drei teure sowie drei günstige Zigarettenmarken wurden miteinander und mit der Referenzzigarette 3R4F der Universität Kentucky verglichen. Zu den teuren Marken zählten Marlboro, Camel und Nil. Die günstigeren Handelsmarken-Zigaretten waren Giants, Goldfield und Jakordia. Die Rauchpumpe „Automatic environmental tobacco smoke emitter“ (AETSE) ermöglichte in einem definierten Raum der abgeschlossenen Rauchkammer, Passivrauch zu erzeugen, ohne die menschliche Gesundheit zu gefährden. Ein standardisiertes Rauchprotokoll garantierte dabei reproduzierbare und vergleichbare Ergebnisse. Das Laser Aerosolspektrometer (LAS) Modell 1.109 der Firma Grimm wies eine Messspanne von 0,25 μm bis 32 μm auf. So konnte der Feinstaub gemessen und gruppiert werden. Obwohl der Versuchsaufbau nicht vollkommen realitätsgetreu war, entstand ein adäquater Vergleich der Feinstaubemissionen von (Handels-)Markenzigaretten.
PM10 und PM2,5 wurden erhoben, weil sie die von der EU und WHO standardisierten Messwerte für die Luftverschmutzung durch Feinstaub sind. Die Messung von PM1 rechtfertigt sich durch die stärker gesundheitsschädigende Komponente von Partikeln dieser Größenordnung. Für diese drei Größenfraktionen wurden die mittlere Konzentration Cmean sowie die Area Under The Curve (AUC) ermittelt. Die AUC stellt dabei die Höhe der Gesamtexposition durch Feinstaub dar.
Die Ergebnisse dieser Versuchsreihe zeigen, dass PM1 den größten Anteil der Feinstaubemission der getesteten Zigaretten ausmachte. Alle Zigarettenmarken haben in einem abgeschlossenen Raum Feinstaubmengen in gesundheitsgefährdender Menge produziert. Die Handelsmarke Jakordia emittierte beim Verrauchen generell weniger Feinstaub als alle anderen Zigarettenmarken. Im Allgemeinen konnte kein Unterschied zwischen den günstigen Handels- und den teuren Markenzigaretten festgestellt werden. Es ist wissenschaftlich belegt, dass sich jede Feinstaubkonzentration negativ auf die Gesundheit auswirkt. Die Ergebnisse können dementsprechend in Gänze unter dem Gesichtspunkt der Gesundheitsschädlichkeit eingestuft werden.
Aufgrund veralteter und unspezifischer, beziehungsweise fehlender Angaben zu den Inhaltsstoffen der einzelnen Zigarettensorten, konnte die Ursache der Unterschiede zwischen Jakordia und den anderen Marken nicht geklärt werden. Die Zigarettenhersteller müssen verpflichtet werden, die detaillierten Zusammensetzungen der Tabakprodukte den Behörden wie dem BMEL oder dem Bundesgesundheitsministerium zugänglich zu machen. Dies wäre ein wichtiger Bestandteil für die zukünftige Forschung und Risikobewertung der verschiedenen Inhalts- und Zusatzstoffe.
Generating predictions about environmental regularities, relying on these predictions, and updating these predictions when there is a violation from incoming sensory evidence are considered crucial functions of our cognitive system for being adaptive in the future. The violation of a prediction can result in a prediction error (PE) which affects subsequent memory processing. In our preregistered studies, we examined the effects of different levels of PE on episodic memory. Participants were asked to generate predictions about the associations between sequentially presented cue-target pairs, which were violated later with individual items in three PE levels, namely low, medium, and high PE. Hereafter, participants were asked to provide old/new judgments on the items with confidence ratings, and to retrieve the paired cues. Our results indicated a better recognition memory for low PE than medium and high PE levels, suggesting a memory congruency effect. On the other hand, there was no evidence of memory benefit for high PE level. Together, these novel and coherent findings strongly suggest that high PE does not guarantee better memory.
Using data samples with an integrated luminosity of 6.4~fb−1 collected by the BESIII detector operating at the BEPCII storage ring, the process of e+e−→γϕJ/ψ is studied. The processes of e+e−→ϕχc1,c2, χc1,c2→γJ/ψ are observed with a significance of more than 10σ. The s√-dependent cross section of e+e−→ϕχc1,c2 is measured between 4.600 and 4.951~GeV, and evidence of a resonance structure is found for the first time in the ϕχc2 process. We also search for the processes of e+e−→γX(4140), γX(4274) and γX(4500) via the γϕJ/ψ final state, but no obvious structures are found. The upper limits on the production cross section times the branching fraction for these processes at the 90% confidence level are reported.
Using a data sample corresponding to an integrated luminosity of 11.3 fb−1 collected at center-of-mass energies from 4.23 to 4.70 GeV with the BESIII detector, we observe the process e+e− → π0π0ψ2(3823) for the first time with a statistical significance of 6.0 standard deviations. The ratio of average cross sections for e+e− → π0π0ψ2(3823) and π+π−ψ2(3823) is determined to be R = σ[e+e− → π0π0ψ2(3823)] σ[e+e−→π+π−ψ2(3823)] = 0.57 ± 0.14 ± 0.05, which is consistent with expectations from isospin symmetry. Here and below, the first uncertainties are statistical and the second are systematic. The mass of the ψ2(3823) is measured to be M[ψ2(3823)] = 3824.5±2.4±1.0 MeV/c2. Due to the limited data sample, an upper limit of 18.8 MeV at 90% confidence level is set on the intrinsic width of ψ2(3823).
Using an 𝑒+𝑒− collision data sample of (27.08±0.14)×108 𝜓(3686) events collected by the BESIII detector, we report the first observation of 𝜒𝑐𝐽→Ω−¯Ω+ (𝐽=0, 1, 2) decays with significances of 5.6𝜎, 6.4𝜎, and 18𝜎, respectively, where the 𝜒𝑐𝐽 mesons are produced in the radiative 𝜓(3686) decays. The branching fractions are determined to be ℬ(𝜒𝑐0→Ω−¯Ω+) = (3.51±0.54±0.29)×10−5, ℬ(𝜒𝑐1→Ω−¯Ω+)=(1.49±0.23±0.10)×10−5, and ℬ(𝜒𝑐2→Ω−¯Ω+)=(4.52±0.24±0.18)×10−5, where the first and second uncertainties are statistical and systematic, respectively.
The Ξ0 asymmetry parameters are measured using entangled quantum Ξ0 − Ξ¯ 0 pairs from a sample of ð448.1 2.9Þ × 106 ψð3686Þ events collected with the BESIII detector at BEPCII. The relative phase between the transition amplitudes of the Ξ0Ξ¯ 0 helicity states is measured to be ΔΦ ¼ −0.050 0.150 0.020 rad, which implies that there is no obvious polarization at the current level of statistics. The decay parameters of the Ξ0 hyperon ðαΞ0 ; αΞ¯ 0 ; ϕΞ0 ; ϕΞ¯ 0 Þ and the angular distribution parameter ½αψð3686Þ and ΔΦ are measured simultaneously for the first time. In addition, the CP asymmetry observables are determined to be AΞ0 CP ¼ ðαΞ0 þ αΞ¯ 0 Þ=ðαΞ0 − αΞ¯ 0 Þ ¼ −0.007 0.082 0.025 and ΔϕΞ0 CP ¼ ðϕΞ0 þ ϕΞ¯ 0 Þ=2 ¼ −0.079 0.082 0.010 rad, which are consistent with CP conservation.
We present our recent results on antiheavy-antiheavy-light-light tetraquark systems using lattice QCD. Our study of the b¯b¯us four-quark system with quantum numbers JP=1+ and the b¯c¯ud four-quark systems with I(JP)=0(0+) and I(JP)=0(1+) utilizes scattering operators at the sink to improve the extraction of the low-lying energy levels. We found a bound state for b¯b¯us with Ebind,b¯b¯us=(−86±22±10)MeV, but no indication for a bound state in both b¯c¯ud channels. Moreover, we show preliminary results for b¯b¯ud with I(JP)=0(1+), where we used scattering operators both at the sink and the source. We found a bound state and determined its infinite-volume binding energy with a scattering analysis, resulting in Ebind,b¯b¯ud=(−103±8)MeV.