Demonstrating Agreement between Radio and Fluorescence Measurements of the Depth of Maximum of Extensive Air Showers at the Pierre Auger Observatory

We show, for the first time, radio measurements of the depth of shower maximum (X_{max}) of air showers induced by cosmic rays that are compared to measurements of the established fluorescence method at the same location. Using measurements at the Pierre Auger Observatory we show full compatibility between our radio and the previously published fluorescence dataset, and between a subset of air showers observed simultaneously with both radio and fluorescence techniques, a measurement setup unique to the Pierre Auger Observatory. Furthermore, we show radio X_{max} resolution as a function of energy and demonstrate the ability to make competitive high-resolution X_{max} measurements with even a sparse radio array. With this, we show that the radio technique is capable of cosmic-ray mass composition studies, both at Auger and at other experiments.

Limits to Gauge Coupling in the Dark Sector Set by the Nonobservation of Instanton-Induced Decay of Super-Heavy Dark Matter in the Pierre Auger Observatory Data

Instantons, which are nonperturbative solutions to Yang-Mills equations, provide a signal for the occurrence of quantum tunneling between distinct classes of vacua. They can give rise to decays of particles otherwise forbidden. Using data collected at the Pierre Auger Observatory, we search for signatures of such instanton-induced processes that would be suggestive of super-heavy particles decaying in the Galactic halo. These particles could have been produced during the post-inflationary epoch and match the relic abundance of dark matter inferred today. The nonobservation of the signatures searched for allows us to derive a bound on the reduced coupling constant of gauge interactions in the dark sector: α_{X}≲0.09, for 10^{9}≲M_{X}/GeV<10^{19}. Conversely, we obtain that, for instance, a reduced coupling constant α_{X}=0.09 excludes masses M_{X}≳3×10^{13}  GeV. In the context of dark matter production from gravitational interactions alone, we illustrate how these bounds are complementary to those obtained on the Hubble rate at the end of inflation from the nonobservation of tensor modes in the cosmological microwave background.

Measurement of the Fluctuations in the Number of Muons in Extensive Air Showers with the Pierre Auger Observatory

We present the first measurement of the fluctuations in the number of muons in extensive air showers produced by ultrahigh energy cosmic rays. We find that the measured fluctuations are in good agreement with predictions from air shower simulations. This observation provides new insights into the origin of the previously reported deficit of muons in air shower simulations and constrains models of hadronic interactions at ultrahigh energies. Our measurement is compatible with the muon deficit originating from small deviations in the predictions from hadronic interaction models of particle production that accumulate as the showers develop.

Features of the Energy Spectrum of Cosmic Rays above 2.5×10^{18} eV Using the Pierre Auger Observatory

We report a measurement of the energy spectrum of cosmic rays above 2.5×10^{18}  eV based on 215 030 events. New results are presented: at about 1.3×10^{19}  eV, the spectral index changes from 2.51±0.03(stat)±0.05(syst) to 3.05±0.05(stat)±0.10(syst), evolving to 5.1±0.3(stat)±0.1(syst) beyond 5×10^{19}  eV, while no significant dependence of spectral features on the declination is seen in the accessible range. These features of the spectrum can be reproduced in models with energy-dependent mass composition. The energy density in cosmic rays above 5×10^{18}  eV is [5.66±0.03(stat)±1.40(syst)]×10^{53}  erg Mpc^{-3}.

Testing Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory

Ultrahigh energy cosmic ray air showers probe particle physics at energies beyond the reach of accelerators. Here we introduce a new method to test hadronic interaction models without relying on the absolute energy calibration, and apply it to events with primary energy 6-16 EeV (E_{CM}=110-170  TeV), whose longitudinal development and lateral distribution were simultaneously measured by the Pierre Auger Observatory. The average hadronic shower is 1.33±0.16 (1.61±0.21) times larger than predicted using the leading LHC-tuned models EPOS-LHC (QGSJetII-04), with a corresponding excess of muons.

Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy

We measure the energy emitted by extensive air showers in the form of radio emission in the frequency range from 30 to 80 MHz. Exploiting the accurate energy scale of the Pierre Auger Observatory, we obtain a radiation energy of 15.8±0.7(stat)±6.7(syst)  MeV for cosmic rays with an energy of 1 EeV arriving perpendicularly to a geomagnetic field of 0.24 G, scaling quadratically with the cosmic-ray energy. A comparison with predictions from state-of-the-art first-principles calculations shows agreement with our measurement. The radiation energy provides direct access to the calorimetric energy in the electromagnetic cascade of extensive air showers. Comparison with our result thus allows the direct calibration of any cosmic-ray radio detector against the well-established energy scale of the Pierre Auger Observatory.

Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory

Energy-dependent patterns in the arrival directions of cosmic rays are searched for using data of the Pierre Auger Observatory. We investigate local regions around the highest-energy cosmic rays with [Formula: see text] eV by analyzing cosmic rays with energies above [Formula: see text] eV arriving within an angular separation of approximately 15[Formula: see text]. We characterize the energy distributions inside these regions by two independent methods, one searching for angular dependence of energy-energy correlations and one searching for collimation of energy along the local system of principal axes of the energy distribution. No significant patterns are found with this analysis. The comparison of these measurements with astrophysical scenarios can therefore be used to obtain constraints on related model parameters such as strength of cosmic-ray deflection and density of point sources.

Measurement of the proton-air cross section at √s=57 TeV with the Pierre Auger Observatory

We report a measurement of the proton-air cross section for particle production at the center-of-mass energy per nucleon of 57 TeV. This is derived from the distribution of the depths of shower maxima observed with the Pierre Auger Observatory: systematic uncertainties are studied in detail. Analyzing the tail of the distribution of the shower maxima, a proton-air cross section of [505±22(stat)(-36)(+28)(syst)] mb is found.

Measurement of the depth of maximum of extensive air showers above 10{18} eV

We describe the measurement of the depth of maximum, X{max}, of the longitudinal development of air showers induced by cosmic rays. Almost 4000 events above 10;{18} eV observed by the fluorescence detector of the Pierre Auger Observatory in coincidence with at least one surface detector station are selected for the analysis. The average shower maximum was found to evolve with energy at a rate of (106{-21}{+35}) g/cm{2}/decade below 10{18.24+/-0.05} eV, and (24+/-3) g/cm{2}/decade above this energy. The measured shower-to-shower fluctuations decrease from about 55 to 26 g/cm{2}. The interpretation of these results in terms of the cosmic ray mass composition is briefly discussed.

Observation of the suppression of the flux of cosmic rays above 4 x 10 (19) eV

The energy spectrum of cosmic rays above 2.5 x 10;{18} eV, derived from 20,000 events recorded at the Pierre Auger Observatory, is described. The spectral index gamma of the particle flux, J proportional, variantE;{-gamma}, at energies between 4 x 10;{18} eV and 4 x 10;{19} eV is 2.69+/-0.02(stat)+/-0.06(syst), steepening to 4.2+/-0.4(stat)+/-0.06(syst) at higher energies. The hypothesis of a single power law is rejected with a significance greater than 6 standard deviations. The data are consistent with the prediction by Greisen and by Zatsepin and Kuz'min.

Upper limit on the diffuse flux of ultrahigh energy tau neutrinos from the Pierre Auger Observatory

The surface detector array of the Pierre Auger Observatory is sensitive to Earth-skimming tau neutrinos that interact in Earth's crust. Tau leptons from nu(tau) charged-current interactions can emerge and decay in the atmosphere to produce a nearly horizontal shower with a significant electromagnetic component. The data collected between 1 January 2004 and 31 August 2007 are used to place an upper limit on the diffuse flux of nu(tau) at EeV energies. Assuming an E(nu)(-2) differential energy spectrum the limit set at 90% C.L. is E(nu)(2)dN(nu)(tau)/dE(nu)<1.3 x 10(-7) GeV cm(-2) s(-1) sr(-1) in the energy range 2 x 10(17) eV< E(nu)< 2 x 10(19) eV.

Career success after flexible training in psychiatry: a survey of former flexible trainees in the Thames regions

This article outlines the findings of a study which indicate that flexible training in psychiatry was considered adequate to prepare doctors for both full-time and part-time work and that those wishing to work part time had no difficulty in finding jobs after accreditation. However, there was evidence to suggest that part-time consultants experienced more problems and less job satisfaction and that part-time training and working may restrict opportunities for an academic career.

The role of unrecognized ambivalence: the mirroring of family conflicts within the professional and legal network

This paper raises some questions about the deleterious effects of unrecognized (unconscious) ambivalence running through child care systems, the Children Act and the adversarial legal system. It is postulated that unrecognized ambivalence may become one of the powerful unconscious dynamics contributing to the mirroring of the family conflicts within the professional network. A detailed clinical example, in which we acted as expert witnesses within a child psychiatry hospital team, is used to illustrate how the denial of ambivalence in a highly complex case, that of a large family involved in care proceedings, led to a state of polarization between the family and a team of professionals which was replicated and amplified within the wider welfare and legal system. It is our view that a state of polarization is likely to produce 'all or nothing decisions' which may not be in the best interest of both children and parents. It is argued that the adversarial nature of the legal process and some underlying assumptions in the Children Act, may contribute to ambivalence being unrecognized. Then it is suggested that ambivalence is inevitable both for professionals and families, particularly in highly complex cases, but with its recognition, a resolution may take place. The conclusions contain some suggestions to promote this process.

Latency--a reappraisal

This paper discusses the specific metapsychology and developmental tasks of the latency period. It offers a Kleinian view of the phase and compares it with other current psychoanalytic theories. The emphasis is on the importance of ego and superego growth and integration during latency resulting in better contact with both external and internal reality. Character formation, social integration and learning are discussed as the specific developmental tasks of the period. Freud's original formulation that the latency period is a consequence of the resolution of the Oedipus complex is evaluated in the light of contemporary developments. I draw on the ideas of Klein and others such as Loewald, Burgner, Holder, Tyson to describe it as a process of progressive and more complex elaboration throughout latency, interconnected with superego development. This process of gradual working through is considered to be a fundamental feature of the period. This model of progressive maturation is illustrated with clinical material. The clinical concept of pseudo-latency is used to distinguish between the developmental achievement represented by the establishment of the latency organisation in contrast to a defensive structure (pseudo-latency) which hides pathology.

The analyst's pregnancy and its consequences on her work

In this paper I discuss with clinical examples how the analyst's pregnancy may affect the analysis in unique, subtle and at times unexpected ways to which the analyst must be alert. Like any major psychosocial crisis in the life cycle, pregnancy challenges the analyst's ability to hold on to the psychoanalytic attitude. It also confronts her with specific issues (primitive anxieties about the inside of the body, fears of loss of identity, of damage to the foetus etc.) which have to be acknowledged and which require consistent and at times painful working through. Overall, my experience was that by and large positive emotional growth took place, both in the patients and myself, during the pregnancy. I would suggest that the possible changes were not only due to the pregnancy per se but to the careful analysis of its effects which allowed for the psychoanalytic situation to be maintained.

The psychodynamics of the STD clinic: secrecy, splitting and isolation

We introduce the idea of a professionally isolated and apparently disconnected agency. We describe how health professionals working in settings with good multi-agency links may not recognize the effect of the isolated agency system on the presentation of problems. In particular, we describe the setting of the Sexually Transmitted Diseases clinic (STD) in which confidentiality can be turned into secrecy by the patients at the service of their denial of the seriousness of their problems. The isolation of the STD clinic as an agency resonates with the patients' isolation from their own feelings and emotional contact with people. It also isolates the professional and the therapeutic network. By way of clinical examples, we describe how this may deskill the staff and lead to dangerous situations.