The baryon density of the Universe from an improved rate of deuterium burning.

Light elements were produced in the first few minutes of the Universe through a sequence of nuclear reactions known as Big Bang nucleosynthesis (BBN)1,2. Among the light elements produced during BBN1,2, deuterium is an excellent indicator of cosmological parameters because its abundance is highly sensitive to the primordial baryon density and also depends on the number of neutrino species permeating the early Universe. Although astronomical observations of primordial deuterium abundance have reached percent accuracy3, theoretical predictions4-6 based on BBN are hampered by large uncertainties on the cross-section of the deuterium burning D(p,γ)3He reaction. Here we show that our improved cross-sections of this reaction lead to BBN estimates of the baryon density at the 1.6 percent level, in excellent agreement with a recent analysis of the cosmic microwave background7. Improved cross-section data were obtained by exploiting the negligible cosmic-ray background deep underground at the Laboratory for Underground Nuclear Astrophysics (LUNA) of the Laboratori Nazionali del Gran Sasso (Italy)8,9. We bombarded a high-purity deuterium gas target10 with an intense proton beam from the LUNA 400-kilovolt accelerator11 and detected the γ-rays from the nuclear reaction under study with a high-purity germanium detector. Our experimental results settle the most uncertain nuclear physics input to BBN calculations and substantially improve the reliability of using primordial abundances to probe the physics of the early Universe.

Proton-Capture Rates on Carbon Isotopes and Their Impact on the Astrophysical

The ^{12}C/^{13}C ratio is a significant indicator of nucleosynthesis and mixing processes during hydrogen burning in stars. Its value mainly depends on the relative rates of the ^{12}C(p,γ)^{13}N and ^{13}C(p,γ)^{14}N reactions. Both reactions have been studied at the Laboratory for Underground Nuclear Astrophysics (LUNA) in Italy down to the lowest energies to date (E_{c.m.}=60 keV) reaching for the first time the high energy tail of hydrogen burning in the shell of giant stars. Our cross sections, obtained with both prompt γ-ray detection and activation measurements, are the most precise to date with overall systematic uncertainties of 7%-8%. Compared with most of the literature, our results are systematically lower, by 25% for the ^{12}C(p,γ)^{13}N reaction and by 30% for ^{13}C(p,γ)^{14}N. We provide the most precise value up to now of 3.6±0.4 in the 20-140 MK range for the lowest possible ^{12}C/^{13}C ratio that can be produced during H burning in giant stars.

Direct Measurement of the

One of the main neutron sources for the astrophysical s process is the reaction ^{13}C(α,n)^{16}O, taking place in thermally pulsing asymptotic giant branch stars at temperatures around 90 MK. To model the nucleosynthesis during this process the reaction cross section needs to be known in the 150-230 keV energy window (Gamow peak). At these sub-Coulomb energies, cross section direct measurements are severely affected by the low event rate, making us rely on input from indirect methods and extrapolations from higher-energy direct data. This leads to an uncertainty in the cross section at the relevant energies too high to reliably constrain the nuclear physics input to s-process calculations. We present the results from a new deep-underground measurement of ^{13}C(α,n)^{16}O, covering the energy range 230-300 keV, with drastically reduced uncertainties over previous measurements and for the first time providing data directly inside the s-process Gamow peak. Selected stellar models have been computed to estimate the impact of our revised reaction rate. For stars of nearly solar composition, we find sizeable variations of some isotopes, whose production is influenced by the activation of close-by branching points that are sensitive to the neutron density, in particular, the two radioactive nuclei ^{60}Fe and ^{205}Pb, as well as ^{152}Gd.

Erratum: Three New Low-Energy Resonances in the

This corrects the article DOI: 10.1103/PhysRevLett.115.252501.

Direct Capture Cross Section and the E_{p}=71 and 105 keV Resonances in the

The ^{22}Ne(p,γ)^{23}Na reaction, part of the neon-sodium cycle of hydrogen burning, may explain the observed anticorrelation between sodium and oxygen abundances in globular cluster stars. Its rate is controlled by a number of low-energy resonances and a slowly varying nonresonant component. Three new resonances at E_{p}=156.2, 189.5, and 259.7 keV have recently been observed and confirmed. However, significant uncertainty on the reaction rate remains due to the nonresonant process and to two suggested resonances at E_{p}=71 and 105 keV. Here, new ^{22}Ne(p,γ)^{23}Na data with high statistics and low background are reported. Stringent upper limits of 6×10^{-11} and 7×10^{-11} eV (90% confidence level), respectively, are placed on the two suggested resonances. In addition, the off-resonant S factor has been measured at unprecedented low energy, constraining the contributions from a subthreshold resonance and the direct capture process. As a result, at a temperature of 0.1 GK the error bar of the ^{22}Ne(p,γ)^{23}Na rate is now reduced by 3 orders of magnitude.

Final Results of the OPERA Experiment on ν_{τ} Appearance in the CNGS Neutrino Beam.

The OPERA experiment was designed to study ν_{µ}→ν_{τ} oscillations in the appearance mode in the CERN to Gran Sasso Neutrino beam (CNGS). In this Letter, we report the final analysis of the full data sample collected between 2008 and 2012, corresponding to 17.97×10^{19} protons on target. Selection criteria looser than in previous analyses have produced ten ν_{τ} candidate events, thus reducing the statistical uncertainty in the measurement of the oscillation parameters and of ν_{τ} properties. A multivariate approach for event identification has been applied to the candidate events and the discovery of ν_{τ} appearance is confirmed with an improved significance level of 6.1σ. |Δm_{32}^{2}| has been measured, in appearance mode, with an accuracy of 20%. The measurement of the ν_{τ} charged-current cross section, for the first time with a negligible contamination from ν[over ¯]_{τ}, and the first direct evidence for the ν_{τ} lepton number are also reported.

Pregnancy and neonatal outcomes among a cohort of HIV-infected women in a large Italian teaching hospital: a 30-year retrospective study.

The primary study objective was to investigate three decades from 1985 to 2014 of changes in pregnancies among HIV-infected women. The secondary objective was to assess risk factors associated with preterm delivery and severe small-for-gestational-age (SGA) infants in HIV-infected women. A retrospective review of deliveries among pregnant HIV-infected women at the University of Genoa and IRCCS San Martino-IST in Genoa between 1985 and 2014 was performed. Univariate and multivariable analyses were used to study the variables associated with neonatal outcomes. Overall, 262 deliveries were included in the study. An increase in median age (26 years in 1985-1994 vs. 34 years in 2005-2014), in the proportion of foreigners (none in 1985-1994 vs. 27/70 (38·6%) in 2005-2014), and a decrease in intravenous drug use (75·2% (91/121) in 1985-1994 vs. 12·9% (9/70) in 2005-2014) among pregnant HIV-infected women was observed. Progressively, HIV infections were diagnosed sooner (prior to pregnancy in 80% (56/70) of women in the last decade). An increase in combined antiretroviral therapy (cART) prescription during pregnancy (50% (27/54) in 1995-2004 vs. 92·2% (59/64) in 2005-2014) and in HIV-RNA <50 copies/ml at delivery (19·2% (5/26) in 1995-2004 vs. 82·3% (53/64) in 2005-2014) was observed. The rate of elective caesarean section from 1985 to 1994 was 9·1%, which increased to 92·3% from 2004 to 2015. Twelve (10·1%) mother-to-child transmissions (MTCT) occurred in the first decade, and six (8·3%) cases occurred in the second decade, the last of which was in 2000. Preterm delivery (<37 weeks gestation) was 5% (6/121) from 1985 to 1994 and increased to 17·1% (12/70) from 2005 to 2014. In univariate and multivariable logistic regression analyses, advancing maternal age and previous pregnancies were associated with preterm delivery (odds ratio (OR) 2·7; 95% confidence intervals (CI) 1-7·8 and OR 2·6; 95% CI 1·1-6·7, respectively). In the logistic regression analysis, use of heroin or methadone was found to be the only risk factor for severe SGA (OR 3·1; 95% CI 1·4-6·8). In conclusion, significant changes in demographic, clinical and therapeutic characteristics of HIV-infected pregnant women have occurred over the last 30 years. Since 2000, MTCT has decreased to zero. An increased risk of preterm delivery was found to be associated with advancing maternal age and previous pregnancies but not with cART. The use of heroin or methadone has been confirmed as a risk factor associated with severe SGA.

Improved Direct Measurement of the 64.5 keV Resonance Strength in the

The ^{17}O(p,α)^{14}N reaction plays a key role in various astrophysical scenarios, from asymptotic giant branch stars to classical novae. It affects the synthesis of rare isotopes such as ^{17}O and ^{18}F, which can provide constraints on astrophysical models. A new direct determination of the E_{R}=64.5 keV resonance strength performed at the Laboratory for Underground Nuclear Astrophysics (LUNA) accelerator has led to the most accurate value to date ωγ=10.0±1.4_{stat}±0.7_{syst} neV, thanks to a significant background reduction underground and generally improved experimental conditions. The (bare) proton partial width of the corresponding state at E_{x}=5672 keV in ^{18}F is Γ_{p}=35±5_{stat}±3_{syst} neV. This width is about a factor of 2 higher than previously estimated, thus leading to a factor of 2 increase in the ^{17}O(p, α)^{14}N reaction rate at astrophysical temperatures relevant to shell hydrogen burning in red giant and asymptotic giant branch stars. The new rate implies lower ^{17}O/^{16}O ratios, with important implications on the interpretation of astrophysical observables from these stars.

Three New Low-Energy Resonances in the

The ^{22}Ne(p,γ)^{23}Na reaction takes part in the neon-sodium cycle of hydrogen burning. This cycle affects the synthesis of the elements between ^{20}Ne and ^{27}Al in asymptotic giant branch stars and novae. The ^{22}Ne(p,γ)^{23}Na reaction rate is very uncertain because of a large number of unobserved resonances lying in the Gamow window. At proton energies below 400 keV, only upper limits exist in the literature for the resonance strengths. Previous reaction rate evaluations differ by large factors. In the present work, the first direct observations of the ^{22}Ne(p,γ)^{23}Na resonances at 156.2, 189.5, and 259.7 keV are reported. Their resonance strengths are derived with 2%-7% uncertainty. In addition, upper limits for three other resonances are greatly reduced. Data are taken using a windowless ^{22}Ne gas target and high-purity germanium detectors at the Laboratory for Underground Nuclear Astrophysics in the Gran Sasso laboratory of the National Institute for Nuclear Physics, Italy, taking advantage of the ultralow background observed deep underground. The new reaction rate is a factor of 20 higher than the recent evaluation at a temperature of 0.1 GK, relevant to nucleosynthesis in asymptotic giant branch stars.

Discovery of τ Neutrino Appearance in the CNGS Neutrino Beam with the OPERA Experiment.

The OPERA experiment was designed to search for ν_{µ}→ν_{τ} oscillations in appearance mode, i.e., by detecting the τ leptons produced in charged current ν_{τ} interactions. The experiment took data from 2008 to 2012 in the CERN Neutrinos to Gran Sasso beam. The observation of the ν_{µ}→ν_{τ} appearance, achieved with four candidate events in a subsample of the data, was previously reported. In this Letter, a fifth ν_{τ} candidate event, found in an enlarged data sample, is described. Together with a further reduction of the expected background, the candidate events detected so far allow us to assess the discovery of ν_{µ}→ν_{τ} oscillations in appearance mode with a significance larger than 5σ.

First direct measurement of the 2H(α,γ)6Li cross section at big bang energies and the primordial lithium problem.

Recent observations of (6)Li in metal poor stars suggest a large production of this isotope during big bang nucleosynthesis (BBN). In standard BBN calculations, the (2)H(α,γ)(6)Li reaction dominates (6)Li production. This reaction has never been measured inside the BBN energy region because its cross section drops exponentially at low energy and because the electric dipole transition is strongly suppressed for the isoscalar particles (2)H and α at energies below the Coulomb barrier. Indirect measurements using the Coulomb dissociation of (6)Li only give upper limits owing to the dominance of nuclear breakup processes. Here, we report on the results of the first measurement of the (2)H(α,γ)(6)Li cross section at big bang energies. The experiment was performed deep underground at the LUNA 400 kV accelerator in Gran Sasso, Italy. The primordial (6)Li/(7)Li isotopic abundance ratio has been determined to be (1.5 ± 0.3) × 10(-5), from our experimental data and standard BBN theory. The much higher (6)Li/(7)Li values reported for halo stars will likely require a nonstandard physics explanation, as discussed in the literature.

First direct measurement of the 17O(p,γ)18F 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,γ)(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 E(c.m.)~/= 200-370 keV appropriate to hydrogen burning in classical novae. In addition, the E(c.m.)=183 keV resonance strength, ωγ=1.67±0.12 µeV, has been measured with the highest precision to date. The uncertainty on the (17)O(p,γ)(18)F reaction rate has been reduced by a factor of 4, thus leading to firmer constraints on accurate models of novae nucleosynthesis.

OPERA tau neutrino charged current interactions.

The OPERA experiment was designed to discover the vτ appearance in a vµ beam, due to neutrino oscillations. The detector, located in the underground Gran Sasso Laboratory, consisted of a nuclear photographic emulsion/lead target with a mass of about 1.25 kt, complemented by electronic detectors. It was exposed from 2008 to 2012 to the CNGS beam: an almost pure vµ beam with a baseline of 730 km, collecting a total of 1.8·1020 protons on target. The OPERA Collaboration eventually assessed the discovery of vµâ†’vτ oscillations with a statistical significance of 6.1 σ by observing ten vτ CC interaction candidates. These events have been published on the Open Data Portal at CERN. This paper provides a detailed description of the vτ data sample to make it usable by the whole community.

The gluteal fold fascio-cutaneous flap for reconstruction after radical excision of primary vulvar cancers.

OBJECTIVES: Reconstructive surgery plays an important role in cosmetic and functional results of major excisional surgery performed as a treatment for invasive vulvar cancer. Traditional techniques -- gracilis myocutaneous o rectus abdominis flaps -- have several limits. We describe here a different surgical approach that we have used since 1998 in an effort to obtain better results in vulvar reconstruction. METHODS: From January 1998 to June 2007, thirty three patients who underwent excisional radical surgery for invasive vulvar tumors, were treated with vulvar reconstruction using the gluteal fold fascio-cutaneous local flap. Flaps were designed along the gluteal fold in adequate length and size. They were oval or triangular in shape depending on the defect they were supposed to cover. The flaps -- which always included the fascial layer -- were raised up to identify a perforator branch of the internal pudendal artery and then harvested as an island flap to achieve better mobility. RESULTS: We had no major complications, only two patients presented marginal necrosis and eight patients experienced significant seromas. Advantages over the alternative techniques included reduced dimensions of scars, absence of flap liponecrosis, no need of modifying patient's position on the surgical table, and very limited blood loss. CONCLUSIONS: We conclude that gluteal fold flap offers excellent cosmetic and functional results with a low complication rate. Therefore we support the gluteal fold flap as a valid surgical option whenever reconstruction is needed after radical excision of vulvar neoplasms.

Effect of tamoxifen on endometrial proliferation.

PURPOSE: An increase in the incidence of endometrial cancer and a potential increase in related mortality has been associated with the administration of 20 mg tamoxifen, the dose adopted in breast cancer chemoprevention trials, thus urging studies on intermediate markers of risk. PATIENTS AND METHODS: Thirty-three women who received 20 mg tamoxifen as adjuvant breast cancer treatment underwent endometrial biopsy. Samples were divided for histologic examination, including a quantitative analysis of stromal:epithelial ratio, and an assessment of DNA ploidy and proliferation by flow cytometry. Results were compared with 37 symptomatic subjects. RESULTS: All histograms were DNA diploid. Compared with controls, a significant increase in the risk of proliferation as measured by the hyperdiploid fraction was associated with tamoxifen duration (< or = 36 months: cumulative odds ratio = 16.5, 95% confidence interval, 1.85 to 146.5; > 36 months: cumulative odds ratio = 28.2, 95% confidence interval, 2.56 to 310.6, P for trend < .05). Tamoxifen-induced risk was significantly reduced by the extent of menopausal status. No cases of cancer or epithelial hyperplasia were observed in the tamoxifen group, whereas seven cases of epithelial hyperplasia without atypia were observed in the control group. The effect of tamoxifen on proliferation was associated with an increase in the stromal component. CONCLUSION: Tamoxifen at 20 mg/d exerts a time-dependent proliferative effect on the endometrium, particularly in premenopausal and early postmenopausal women. This effect appears to be mediated by the stromal component, which accounts for the discrepancy between flow cytometry and histology. Our study provides preliminary evidence that the DNA flow cytometric hyperdiploid fraction may be a useful tool for monitoring endometrial cell proliferation in women exposed to tamoxifen.

Efficacy of the association of 13-cis-retinoic acid (13cRA) and alpha-interferon 2a (alpha-IFN 2a) in moderate-severe cervical intraepithelial neoplasia (CIN II-III): a pilot study.

Recent in vitro studies have suggested a possible therapeutic synergism between alpha-IFN 2a and 13cRA in certain neoplasias, while encouraging in vivo findings strongly support the enhanced effectiveness of the two agents when used in combination. The specific aim of our study was to evaluate the efficacy and the toxicity of the association of 13cRA and alpha-IFN 2a in patients with CIN II and CIN III who refused surgical treatment. Twenty-one patients (aged between 25 and 58 years), of which 14 were CIN II and 7 CIN III, entered the study. 13cRA (orally at 0.5-1 mg/Kg/day) and alpha-IFN 2a (intramuscular at 3x10(6) I.U./day for the first 15 days, then 3 times/week for the following four weeks) were administered simultaneously for eight consecutive weeks. 13/21 (62%) histologically verified objective responses (6 complete and 7 partial) were achieved. We also obtained 8 stable diseases. Compliance was generally good and no delays in therapy due to toxicity were recorded (except for two patients presenting WHO degree III cutaneous and mucosal toxicity which regressed one week after suspending treatment). Human Papilloma Virus (HPV) was initially detected in 16/21 (76%) patients, while HPV negativization after treatment was observed in 3/16 (19%). Although preliminary and requiring long-term assessment, the encouraging results of this study confirm the need for further investigation on the role of systemic medical therapy in the treatment of CINs.

Evaluation of the sensitivity of cervicography in a consecutive colposcopic series.

Cervicography was performed in 606 women referred for colposcopy. Cervigrams were blindly reviewed by two independent readers. The positivity rate at cervicography was high (operator A = 50%, B = 58.8%). The sensitivity for papillomavirus infection (HPV)/cervical intraepithelial neoplasia I (CIN I) (n = 141) was 79.4% for operator A and 80.8% for operator B. The sensitivity for CIN II or more severe lesions (n = 22) was 95.2% and 90.5% for operators A and B, respectively. The positive predictive value for HPV/CIN I or CIN II, or more severe lesions was 36.9% and 6.9% for operator A and 32.1% and 5.3% for operator B, respectively. Interobserver variability was acceptable (kappa = 0.62). Cervicography suspected 27 HPV/CIN I, 1 CIN II and 1 CIN III which showed no cytologic abnormalities. This study confirms that cervicography has a good sensitivity for cervical lesions, but it is based on a selected series, not representative of a screening condition. The combination of cervicography and cytology in screening is presently under evaluation in a prospective study of screened women.

[Proposal for the treatment of cervix dysplasia with immunomodulators]. / Proposta di terapia con immunomodulanti nelle displasie cervicali.

The study included 60 patients: 43 suffered from slight portio dysplasia (12 had HPV infection also), while 17 had moderate dysplasia (7 had HPV infections also). The treatment was carried out by self-administration in 3 stages: attack (50 mg of thymopentin by s.c. injection every day for two weeks); maintenance (50 mg of thymopentin by s.c. injection every other day for ten weeks); recall 6 months after (50 mg of thymopentin every day for 4 weeks). The drug was well tolerated by all of the patients and the recovery rate in a 9-months follow-up period was significantly higher versus an historical control group.

[Smoking in a sample of nursing students in Genoa. Reflections on the role of professional educators]. / Abitudine al fumo di un campione di allievi infermieri genovesi. Riflessioni sul ruolo educativo della professione.

Of all European Union member states, Italy has one of the highest rates of smokers among health care personnel. One important step towards the development of a "prevention-oriented culture" is the raising of the awareness of professional working in health care structures in order to involve them in preventive actions, this making these more effective. Before undertaking measures of this kind, it is imperative to first assess the extent of the smoking habit, even at the local level, so as to target actions as precisely as possible. We herein present the results of a study carried out in two professional nursing schools of the Province of Genoa (I). In all, 341 subjects, aged between 18 and 34, were interviewed. Findings show a high percentage of smokers among both sexes, with 50.0% of males and 40.0% of females claiming to be smokers. These figures are well above national averages (32% of males and 26% of females in the national population). The age at which most interviewees began smoking ranged from 15 to 18 years; however, a rather high percentage of respondents (25.1% for males and 26.1% for females) began after 18 years of age. Our results confirm the importance of school age oriented health education programs, but highlight as well the usefulness of similar awareness initiatives for future professionals. The Italian League for the Fight Against Cancer and the Italian Association of Cancer Nurses propose to vocational training schools a collaborative effort aiming to promote healthy lifestyles among nursing students and to re-assess the role of trainers.