The Gravettian burial known as the Prince (‘Il Principe’): new evidence for his age and diet

The famous upper Palaeolithic (Gravettian) burial with shell ornaments known as "Il Principe" was discovered in Italy sixty years ago. Here the authors present recent scientific research on his skeleton, leading to new assessments of the date of the burial and indications of diet

Performance assessment of a distributed intrusion detection system in a real network scenario

The heterogeneity and complexity of modern networks and services urge the requirement for flexible and scalable security systems, which can be dynamically configured to suit the everchanging nature of security threats and user behavior patterns. In this paper we present a distributed architecture for an Intrusion Detection System, allowing for traffic analysis at different granularity levels, performed by using the best available techniques. Such architecture leverages the principle of separation of concerns, and hence proposes to build up a system comprising entities specialized in performing different tasks, appropriately orchestrated by a broker entity playing the crucial role of the mediator. This paper stresses the point that a distributed system, besides being inherently more scalable than a centralized one, allows for better detection capabilities thanks to the effective exploitation of the inner heterogeneity of the involved detection engines. In order to support our findings, we will describe the design, implementation and deployment of the proposed solution in the framework of the INTERSECTION FP7 European Project

New insights on final Epigravettian funerary behavior at Arene Candide cave (Western Liguria, Italy)

We gained new insights on Epigravettian funerary behavior at the Arene Candide cave through the osteological and spatial analysis of the burials and human bone accumulations found in the cave during past excavations. Archaeothanathological information on the human skeletal remains was recovered from diaries, field pictures and notes, and data from recent excavations was integrated. The secondary deposits have traditionally been interpreted as older burials that were disturbed to make space for new inhumations. Our results suggest that those disturbances were not casual: older burials were intentionally displaced to bury younger inhumations. Subsequently, some skeletal elements, especially crania, were arranged around the new burial; these were often placed within stone niches. Based on the composition of some clusters, which contain the bones of two individuals displaced together, it is possible that a double burial composed of two adults was originally present at the site. This would be a burial type that had not been recognized at Arene Candide until now. Strikingly, this potential double burial contained an individual showing pathological bowing of the limbs, a finding which is not infrequent in skeletons from Gravettian and Epigravettian multiple burials. In addition, the crania and other skeletal elements derived from this burial were intentionally placed around a new inhumation, whose skeleton possibly shows a milder form of the same disease (possibly hereditary rickets). This and other observations suggest that the five individuals belonging to the second phase of this “cemetery” (AMS dates spanning 12,030 – 11,180 cal BP) might have been buried over a relatively brief time span. Our study demonstrated similar behaviors in the first phase of mortuary use of the cave (12,820 – 12,420 cal BP), indicating a remarkable persistence in Final Epigravettian funerary models despite their archaeologically apparent rarity and intermittent nature

Feasibility of low energy radiative capture experiments at the LUNA underground accelerator facility

The LUNA (Laboratory Underground for Nuclear Astrophysics) facility has been designed to study nuclear reactions of astrophysical interest. It is located deep underground in the Gran Sasso National Laboratory, Italy. Two electrostatic accelerators, with 50 and 400 kV maximum voltage, in combination with solid and gas target setups allowed to measure the total cross sections of the radiative capture reactions $^2$H(p,$\gamma$)3He and $^{14}$N(p,$\gamma$)$^{15}$O within their relevant Gamow peaks. We report on the gamma background in the Gran Sasso laboratory measured by germanium and bismuth germanate detectors, with and without an incident proton beam. A method to localize the sources of beam induced background using the Doppler shift of emitted gamma rays is presented. The feasibility of radiative capture studies at energies of astrophysical interest is discussed for several experimental scenarios.Comment: Submitted to Eur. Phys. J.

Closing the loop of SIEM analysis to Secure Critical Infrastructures

Critical Infrastructure Protection is one of the main challenges of last years. Security Information and Event Management (SIEM) systems are widely used for coping with this challenge. However, they currently present several limitations that have to be overcome. In this paper we propose an enhanced SIEM system in which we have introduced novel components to i) enable multiple layer data analysis; ii) resolve conflicts among security policies, and discover unauthorized data paths in such a way to be able to reconfigure network devices. Furthermore, the system is enriched by a Resilient Event Storage that ensures integrity and unforgeability of events stored

First measurement of the 14N(p,gamma)15O cross section down to 70 keV

In stars with temperatures above 20*10^6 K, hydrogen burning is dominated by the CNO cycle. Its rate is determined by the slowest process, the 14N(p,gamma)15O reaction. Deep underground in Italy's Gran Sasso laboratory, at the LUNA 400 kV accelerator, the cross section of this reaction has been measured at energies much lower than ever achieved before. Using a windowless gas target and a 4pi BGO summing detector, direct cross section data has been obtained down to 70 keV, reaching a value of 0.24 picobarn. The Gamow peak has been covered by experimental data for several scenarios of stable and explosive hydrogen burning. In addition, the strength of the 259 keV resonance has been remeasured. The thermonuclear reaction rate has been calculated for temperatures 90 - 300 *10^6 K, for the first time with negligible impact from extrapolations

Activation measurement of the 3He(alpha,gamma)7Be cross section at low energy

The nuclear physics input from the 3He(alpha,gamma)7Be cross section is a major uncertainty in the fluxes of 7Be and 8B neutrinos from the Sun predicted by solar models and in the 7Li abundance obtained in big-bang nucleosynthesis calculations. The present work reports on a new precision experiment using the activation technique at energies directly relevant to big-bang nucleosynthesis. Previously such low energies had been reached experimentally only by the prompt-gamma technique and with inferior precision. Using a windowless gas target, high beam intensity and low background gamma-counting facilities, the 3He(alpha,gamma)7Be cross section has been determined at 127, 148 and 169 keV center-of-mass energy with a total uncertainty of 4%. The sources of systematic uncertainty are discussed in detail. The present data can be used in big-bang nucleosynthesis calculations and to constrain the extrapolation of the 3He(alpha,gamma)7Be astrophysical S-factor to solar energies

Comparison of the LUNA 3He(alpha,gamma)7Be activation results with earlier measurements and model calculations

Recently, the LUNA collaboration has carried out a high precision measurement on the 3He(alpha,gamma)7Be reaction cross section with both activation and on-line gamma-detection methods at unprecedented low energies. In this paper the results obtained with the activation method are summarized. The results are compared with previous activation experiments and the zero energy extrapolated astrophysical S factor is determined using different theoretical models.Comment: Accepted for publication in Journal of Physics

First Direct Measurement of the ^{17}O(p,\gamma)^{18}F Reaction Cross-Section at Gamow Energies for Classical Novae

Classical novae are important contributors to the abundances of key isotopes, such as the radioactive ^{18}F, whose observation by satellite missions could provide constraints on nucleosynthesis models in novae. The ^{17}O(p,\gamma)^{18}F reaction plays a critical role in the synthesis of both oxygen and fluorine isotopes but its reaction rate is not well determined because of the lack of experimental data at energies relevant to novae explosions. In this study, the reaction cross section has been measured directly for the first time in a wide energy range Ecm = 200 - 370 keV appropriate to hydrogen burning in classical novae. In addition, the E=183 keV resonance strength, \omega \gamma=1.67\pm0.12 \mueV, has been measured with the highest precision to date. The uncertainty on the ^{17}O(p,\gamma)^{18}F reaction rate has been reduced by a factor of 4, thus leading to firmer constraints on accurate models of novae nucleosynthesis.Comment: accepted by Phys. Rev. Let

The 3He(alpha,gamma)7Be S-factor at solar energies: the prompt gamma experiment at LUNA

The 3He(alpha,gamma)7Be process is a key reaction in both Big-Bang nucleosynthesis and p-p chain of Hydrogen Burning in Stars. A new measurement of the 3He(alpha,gamma)7Be cross section has been performed at the INFN Gran Sasso underground laboratory by both the activation and the prompt gamma detection methods. The present work reports full details of the prompt gamma detection experiment, focusing on the determination of the systematic uncertainty. The final data, including activation measurements at LUNA, are compared with the results of the last generation experiments and two different theoretical models are used to obtain the S-factor at solar energies.Comment: Accepted for publication in Nucl. Phys.