Even though statistics cannot draw a comprehensive picture of the reality of poverty or the feelings and suffering of the people affected and even less of how they cope with their situation and ...deprivations, some initial figures can illustrate how child poverty spreads. What is important is not only the poverty rate, or how child poverty spreads, but rather the individual case, the single child unable to seize opportunities in life due to economic poverty. Because each of these children is one too many and our efforts are necessary to support their well-being, the consequences of child poverty will be presented in specific fields such as health or education.
A statewide cohort study on the occurrence of second primary neoplasms was conducted among 9678 women first diagnosed with breast cancer in Saarland, Germany between 1968 and 1987. A total number of ...409 second primary neoplasms was observed compared to 328 cases that would have been expected based on the incidence rates of the general population (standardised incidence ratio, SIR = 1.25). This elevation in incidence of second neoplasms was primarily due to increased occurrence of cancer of the opposite breast (SIR = 2.48), which was most pronounced for patients below the age of 50 (SIR = 4.20) and within the first 5 years after diagnosis (SIR = 2.91). There was a moderate elevation in incidence of malignant tumours of the ovaries (SIR = 1.46), while the incidence of most other malignancies was lower than in the general population. Our results, which are in agreement with previous findings from Northern Europe, the U.S.A. and Japan provide valuable background information for aetiological research, as well as for surveillance of breast cancer patients.
Nanowires with helical surface states represent key prerequisites for observing and exploiting phase-coherent topological conductance phenomena, such as spin-momentum locked quantum transport or ...topological superconductivity. We demonstrate in a joint experimental and theoretical study that gated nanowires fabricated from high-mobility strained HgTe, known as a bulk topological insulator, indeed preserve the topological nature of the surface states, that moreover extend phase-coherently across the entire wire geometry. The phase-coherence lengths are enhanced up to 5 \(\mu\)m when tuning the wires into the bulk gap, so as to single out topological transport. The nanowires exhibit distinct conductance oscillations, both as a function of the flux due to an axial magnetic field, and of a gate voltage. The observed \(h/e\)-periodic Aharonov-Bohm-type modulations indicate surface-mediated quasi-ballistic transport. Furthermore, an in-depth analysis of the scaling of the observed gate-dependent conductance oscillations reveals the topological nature of these surface states. To this end we combined numerical tight-binding calculations of the quantum magneto-conductance with simulations of the electrostatics, accounting for the gate-induced inhomogenous charge carrier densities around the wires. We find that helical transport prevails even for strongly inhomogenous gating and is governed by flux-sensitive high-angular momentum surface states that extend around the entire wire circumference.
The occurrence of second primary malignancies was assessed among 2922 women with cervical cancer, 2721 women with endometrial cancer and 1745 women with malignant neoplasms of the ovaries, who were ...notified to the cancer registry of Saarland, Germany, between 1968 and 1987. Analyses are presented for second primary malignancies at any site and at the most important single sites. Among women with cervical cancer, 98 second primary malignancies were observed, slightly fewer than the 99.3 cases that would have been expected on the basis of the incidence rates of the general population (standardized incidence ratio, SIR = 0.99). More second malignancies were observed than expected in the urinary bladder (SIR = 3.51) while the opposite applied to second neoplasms in the breast (SIR = 0.56). Among women with endometrial and ovarian cancer, the numbers of observed cases slightly exceeded the expected numbers for second primary neoplasms at any site (SIR = 1.19 and 1.41 respectively). More second primary neoplasms were observed than expected in the colon, breast, urinary bladder and kidneys among these women. We discuss our results, which are in agreement with findings among North European and North American populations, from clinical and etiological points of view.
We derive rotation curves from optical emission lines of 182 disk galaxies (96 in the cluster and 86 in the field) in the region of Abell 901/902 located at \(z\sim 0.165\). We focus on the analysis ...of B-band and stellar-mass Tully-Fisher relations. We examine possible environmental dependencies and differences between normal spirals and "dusty red" galaxies, i.e. disk galaxies that have red colors due to relatively low star formation rates. We find no significant differences between the best-fit TF slope of cluster and field galaxies. At fixed slope, the field population with high-quality rotation curves (57 objects) is brighter by \(\Delta M_{B}=-0\fm42\pm0\fm15\) than the cluster population (55 objects). We show that this slight difference is at least in part an environmental effect. The scatter of the cluster TFR increases for galaxies closer to the core region, also indicating an environmental effect. Interestingly, dusty red galaxies become fainter towards the core at given rotation velocity (i.e. total mass). This indicates that the star formation in these galaxies is in the process of being quenched. The luminosities of normal spiral galaxies are slightly higher at fixed rotation velocity for smaller cluster-centric radii. Probably these galaxies are gas-rich (compared to the dusty red population) and the onset of ram-pressure stripping increases their star-formation rates. The results from the TF analysis are consistent with and complement our previous findings. Dusty red galaxies might be an intermediate stage in the transformation of infalling field spiral galaxies into cluster S0s, and this might explain the well-known increase of the S0 fraction in galaxy clusters with cosmic time.
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