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Die Nutzung der natürlichen Ressourcen ist zur Sicherung gesellschaftlichen Aktivitäten unverzichtbar, gleichwohl stehen ihrer nachhaltigen Bewirtschaftung immer neue Veränderungsprozesse und damit einhergehende Herausforderungen gegenüber. In Anbetracht von wirtschaftlichen Konzentrationsprozessen, sozio-strukturellen und demographischen Entwicklungen, technischen Innovationen, globalem Wandel und neuen Erkenntnissen zu Risiken stoßen etablierte klassische Verfahren des Planungsdenkens zunehmend an ihre Grenzen. Vor diesem Hintergrund wurden neue und innovative Ansätze zur Ressourcensicherung entwickelt, die vereinzelt auch bereits in der Praxis realisiert wurden. Sie greifen die Herausforderung gegenwärtiger Veränderungsprozesse konzeptionell auf und überführen sie in angepasste Strukturen und Verfahren. Die vorliegende Arbeit beschreibt diesen Übergang zu einem neuen, angepassten Planungsdenken. In seinem Mittelpunkt steht der Begriff der „sozial-ökologischen Ressourcenregulation“. Am Beispiel der Bewirtschaftung der Wasserressourcen werden aktuelle Entwicklungen vorgestellt und exemplarisch anhand von zwei Fallbeispielen vertieft: dem Fuhrberger Feld und dem Hessische Ried unter den spezifischen Gesichtspunkten von Wassergüte und Wassermenge. Die Entwicklungen in beiden Regionen werden zunächst anhand der Anforderungen an eine sozial-ökologische Regulation bewertet. In einem weiteren Schritt werden verallgemeinerte Schlussfolgerungen für eine verbesserte Ressourcenbewirtschaftung und deren Regulation sowohl hinsichtlich der Wassergüte als auch der Wassermenge gezogen. Es zeigt sich hierbei die große Bedeutung der Entstehung adaptiver Strukturen durch Rückkopplungen und den Einbezug der relevanten gesellschaftlichen Akteure; so ist langfristig auch eine Koexistenz von tendenziell konfligierenden Ressourcennutzungen und deren nachhaltige Entwicklung möglich.
This assessment concept paper provides a methodological approach for the formative assessment and summative assessment of GIZ’s International Water Stewardship Programme (IWaSP) and its component partnerships. IWaSP promotes partnerships between the private sector (corporations and SMEs), the public sector and the society to tackle shared water risks and to manage water equitably to meet competing demands. This evaluative assessment concept describes the generic approach of the assessment, the cycle for the assessment of partnerships, the country coordination and the programme.
The overall goal of the assessment is to provide evidence for taxpayers in the donor countries and for citizens in the partnership countries. It also aims to examine the relevance of the programme’s approach, its underlying assumptions, and the heterogeneity of stakeholders and their specific interests. Since the assessment is also formative feedback to GIZ and IWaSP stakeholders, it aims to guide the future implementation of the partnerships and the programme.
The assessment is guided by several generic principles: assessing for learning (formative assessment); assessment of learning (summative assessment); iteration; structuring complex problems; unblocking results; and conformity with other assessment criteria set out by the OECD the Development Assistance Committee (DAC) and GIZ’s Capacity Works success factors (GTZ 2010).
These generic criteria are adapted to the three levels of the IWaSP structure. First, the assessment cycle for partnerships includes the validation of stakeholders (mapping), the analysis of secondary literature, face-to-face interviews and a process for feeding back the findings. Generic tools are provided to guide the assessment, such as a list of key documents and an interview guide. Partnerships will undergo a baseline, interim assessment and final assessment. As progress varies across individual IWaSP partnerships, the steps taken by each partnership to assess shared water risks, prioritise and agree interventions, are expected to differ slightly. In response to these differences the sequencing and content of the assessment may need to be adapted for the different partnerships.
Second, the country-level assessment considers issues such as the coordination of partnerships within a country, scoping strategies, and interaction between partnership and the programme. Information gathered during the partnership assessment feeds into the country-level assessment.
Third, the assessment cycle for the programme involves a document and monitoring plan analysis, reflection on the different perspectives of the programme staff, country staff and external stakeholders.
The final section is concerned with reporting. Several annexes are provided relating to the organisation and preparation of the assessment, including question guidelines and analysis procedures.
This work presents an effective model for strongly interacting matter and the QCD equation of state (EoS). The model includes both hadron and quark degrees of freedom and takes into account the transition of chiral symmetry restoration as well as the deconfinement phase transition. At low temperatures T and baryonic densities ρB a hadron resonance gas is described using a SU(3)-flavor sigma-omega model and a quark phase is introduced in analogy to PNJL models for higher T and ρB. In this way, the correct asymptotic degrees of freedom are used in a wide range of T and ρB. Here, results of this model concerning the chiral and deconfinement phase transitions and thermodynamic model properties are presented. Large hadron resonance multiplicities in the transition region emphasize the importance of heavy-mass resonance states in this region and their impact on the chiral transition behavior. The resulting phase diagram of QCD matter at small chemical potentials is in line with latest lattice QCD and thermal model results.
We study the phase diagram of a generalized chiral SU(3)-flavor model in mean-field approxi- mation. In particular, the influence of the baryon resonances, and their couplings to the scalar and vector fields, on the characteristics of the chiral phase transition as a function of temperature and baryon-chemical potential is investigated. Present and future finite-density lattice calculations might constrain the couplings of the fields to the baryons. The results are compared to recent lattice QCD calculations and it is shown that it is non-trivial to obtain, simultaneously, stable cold nuclear matter.
Abstract: The measured particle ratios in central heavy-ion collisions at RHIC-BNL are investigated within a chemical and thermal equilibrium chiral SU(3) Ã É approach. The commonly adopted non-interacting gas calculations yield temperatures close to or above the critical temperature for the chiral phase transition, but without taking into account any interactions. In contrast, the chiral SU(3) model predicts temperature and density dependent effective hadron masses and effective chemical potentials in the medium and a transition to a chirally restored phase at high temperatures or chemical potentials. Three different parametrizations of the model, which show different types of phase transition behaviour, are investigated. We show that if a chiral phase transition occured in those collisions, freezing of the relative hadron abundances in the symmetric phase is excluded by the data. Therefore, either very rapid chemical equilibration must occur in the broken phase, or the measured hadron ratios are the outcome of the dynamical symmetry breaking. Furthermore, the extracted chemical freeze-out parameters differ considerably from those obtained in simple non-interacting gas calculations. In particular, the three models yield up to 35 MeV lower temperatures than the free gas approximation. The inmedium masses turn out to differ up to 150 MeV from their vacuum values.
In this work the baryon number and strange susceptibility of second and fourth order are presented. The results at zero baryon-chemical potential are obtained using a well tested chiral effective model including all known hadron degrees of freedom and additionally implementing quarks and gluons in a PNJL-like approach. Quark and baryon number susceptibilities are sensitive to the fundamental degrees of freedom in the model and signal the shift from massive hadrons to light quarks at the deconfinement transition by a sharp rise at the critical temperature. Furthermore, all susceptibilities are found to be largely suppressed by repulsive vector field interactions of the particles. In the hadronic sector vector repulsion of baryon resonances restrains fluctuations to a large amount and in the quark sector above Tc even small vector field interactions of quarks quench all fluctuations unreasonably strong. For this reason, vector field interactions for quarks have to vanish in the deconfinement limit.
A unified chiral mean field approach is presented for QCD thermodynamics in a wide range of temperatures and densities. The model simultaneously gives a satisfactory description of lattice QCD thermodynamics and fulfills nuclear matter and astrophysical constraints. The resulting equation of state can be incorporated in relativistic fluid-dynamical simulations of heavy-ion collisions and neutron stars mergers. Access to different regions of the QCD phase diagram can be obtained in simulations of heavy-ion data and observations of neutron star mergers.
The measured particle ratios in central heavy-ion collisions at RHIC-BNL are investigated within a chemical and thermal equilibrium chiral SU(3) σ–ω approach. The commonly adopted noninteracting gas calculations yield temperatures close to or above the critical temperature for the chiral phase transition, but without taking into account any interactions. Contrary, the chiral SU(3) model predicts temperature and density dependent effective hadron masses and effective chemical potentials in the medium and a transition to a chirally restored phase at high temperatures or chemical potentials. Three different parametrizations of the model, which show different types of phase transition behaviour, are investigated. We show that if a chiral phase transition occured in those collisions, “freezing” of the relative hadron abundances in the symmetric phase is excluded by the data. Therefore, either very rapid chemical equilibration must occur in the broken phase, or the measured hadron ratios are the outcome of the dynamical symmetry breaking. Furthermore, the extracted chemical freeze-out parameters differ considerably from those obtained in simple noninteracting gas calculations. In particular, the three models yield up to 35 MeV lower temperatures than the free gas approximation. The in-medium masses turn out to differ up to 150 MeV from their vacuum values.
We show how repulsive interactions of deconfined quarks as well as confined hadrons have an influence on the baryon number susceptibilities and the curvature of the chiral pseudo-critical line in effective models of QCD. We discuss implications and constraints for the vector interaction strength from comparisons to lattice QCD and comment on earlier constraints, extracted from the curvature of the transition line of QCD and compact star observables. Our results clearly point to a strong vector repulsion in the hadronic phase and near-zero repulsion in the deconfined phase.
Gravitational waves, electromagnetic radiation, and the emission of high energy particles probe the phase structure of the equation of state of dense matter produced at the crossroad of the closely related relativistic collisions of heavy ions and of binary neutron stars mergers. 3 + 1 dimensional special- and general relativistic hydrodynamic simulation studies reveal a unique window of opportunity to observe phase transitions in compressed baryon matter by laboratory based experiments and by astrophysical multimessenger observations. The astrophysical consequences of a hadron-quark phase transition in the interior of a compact star will be focused within this article. Especially with a future detection of the post-merger gravitational wave emission emanated from a binary neutron star merger event, it would be possible to explore the phase structure of quantum chromodynamics. The astrophysical observables of a hadron-quark phase transition in a single compact star system and binary hybrid star merger scenario will be summarized within this article. The FAIR facility at GSI Helmholtzzentrum allows one to study the universe in the laboratory, and several astrophysical signatures of the quark-gluon plasma have been found in relativistic collisions of heavy ions and will be explored in future experiments.