Global anisotropies in TeV cosmic rays related to the Sun's local galactic environment from IBEX.

Observations with the Interstellar Boundary Explorer (IBEX) have shown enhanced energetic neutral atom (ENA) emission from a narrow, circular ribbon likely centered on the direction of the local interstellar medium (LISM) magnetic field. Here, we show that recent determinations of the local interstellar velocity, based on interstellar atom measurements with IBEX, are consistent with the interstellar modulation of high-energy (tera-electron volts, TeV) cosmic rays and diffusive propagation from supernova sources revealed in global anisotropy maps of ground-based high-energy cosmic-ray observatories (Milagro, Asγ, and IceCube). Establishing a consistent local interstellar magnetic field direction using IBEX ENAs at hundreds to thousands of eV and galactic cosmic rays at tens of TeV has wide-ranging implications for the structure of our heliosphere and its interactions with the LISM, which is particularly important at the time when the Voyager spacecraft are leaving our heliosphere.

Limits on a muon flux from neutralino annihilations in the sun with the IceCube 22-string detector.

A search for muon neutrinos from neutralino annihilations in the Sun has been performed with the IceCube 22-string neutrino detector using data collected in 104.3 days of live time in 2007. No excess over the expected atmospheric background has been observed. Upper limits have been obtained on the annihilation rate of captured neutralinos in the Sun and converted to limits on the weakly interacting massive particle (WIMP) proton cross sections for WIMP masses in the range 250-5000 GeV. These results are the most stringent limits to date on neutralino annihilation in the Sun.

Extending the search for neutrino point sources with IceCube above the horizon.

Point source searches with the IceCube neutrino telescope have been restricted to one hemisphere, due to the exclusive selection of upward going events as a way of rejecting the atmospheric muon background. We show that the region above the horizon can be included by suppressing the background through energy-sensitive cuts. This improves the sensitivity above PeV energies, previously not accessible for declinations of more than a few degrees below the horizon due to the absorption of neutrinos in Earth. We present results based on data collected with 22 strings of IceCube, extending its field of view and energy reach for point source searches. No significant excess above the atmospheric background is observed in a sky scan and in tests of source candidates. Upper limits are reported, which for the first time cover point sources in the southern sky up to EeV energies.

Limits on the high-energy gamma and neutrino fluxes from the SGR 1806-20 giant flare of 27 December 2004 with the AMANDA-II detector.

On 27 December 2004, a giant gamma flare from the Soft Gamma-Ray Repeater 1806-20 saturated many satellite gamma-ray detectors, being the brightest transient event ever observed in the Galaxy. AMANDA-II was used to search for down-going muons indicative of high-energy gammas and/or neutrinos from this object. The data revealed no significant signal, so upper limits (at 90% C.L.) on the normalization constant were set: 0.05(0.5) TeV-1 m;{-2} s;{-1} for gamma=-1.47 (-2) in the gamma flux and 0.4(6.1) TeV-1 m;{-2} s;{-1} for gamma=-1.47 (-2) in the high-energy neutrino flux.

Search for extraterrestrial point sources of neutrinos with AMANDA-II.

We present the results of a search for point sources of high-energy neutrinos in the northern hemisphere using AMANDA-II data collected in the year 2000. Included are flux limits on several active-galactic-nuclei blazars, microquasars, magnetars, and other candidate neutrino sources. A search for excesses above a random background of cosmic-ray-induced atmospheric neutrinos and misreconstructed downgoing cosmic-ray muons reveals no statistically significant neutrino point sources. We show that AMANDA-II has achieved the sensitivity required to probe known TeV gamma-ray sources such as the blazar Markarian 501 in its 1997 flaring state at a level where neutrino and gamma-ray fluxes are equal.

Limits on diffuse fluxes of high energy extraterrestrial neutrinos with the AMANDA-B10 detector.

Data from the AMANDA-B10 detector taken during the austral winter of 1997 have been searched for a diffuse flux of high energy extraterrestrial muon neutrinos. This search yielded no excess events above those expected from background atmospheric neutrinos, leading to upper limits on the extraterrestrial neutrino flux measured at the earth. For an assumed E-2 spectrum, a 90% classical confidence level upper limit has been placed at a level E2Phi(E)=8.4 x 10(-7) cm(-2) s(-1) sr(-1) GeV (for a predominant neutrino energy range 6-1000 TeV), which is the most restrictive bound placed by any neutrino detector. Some specific predicted model spectra are excluded. Interpreting these limits in terms of the flux from a cosmological distributions of sources requires the incorporation of neutrino oscillations, typically weakening the limits by a factor of 2.

Observation of high-energy neutrinos using Cerenkov detectors embedded deep in Antarctic ice.

Neutrinos are elementary particles that carry no electric charge and have little mass. As they interact only weakly with other particles, they can penetrate enormous amounts of matter, and therefore have the potential to directly convey astrophysical information from the edge of the Universe and from deep inside the most cataclysmic high-energy regions. The neutrino's great penetrating power, however, also makes this particle difficult to detect. Underground detectors have observed low-energy neutrinos from the Sun and a nearby supernova, as well as neutrinos generated in the Earth's atmosphere. But the very low fluxes of high-energy neutrinos from cosmic sources can be observed only by much larger, expandable detectors in, for example, deep water or ice. Here we report the detection of upwardly propagating atmospheric neutrinos by the ice-based Antarctic muon and neutrino detector array (AMANDA). These results establish a technology with which to build a kilometre-scale neutrino observatory necessary for astrophysical observations.

Short-term effects of atenolol and nifedipine on atrial natriuretic peptide, plasma renin activity, and plasma aldosterone in patients with essential hypertension.

The short-term effects of atenolol and nifedipine on plasma levels of atrial natriuretic peptide (ANP), plasma renin activity (PRA), and plasma aldosterone (PA) were studied in two groups of patients with uncomplicated essential hypertension. Urinary catecholamines, and sodium and potassium excretion were also studied. A group of 20 patients with hypertension, after a wash-out period of at least 10 days, was randomly subdivided into two protocol therapy subgroups. One group (six men and four women) received atenolol (100 mg/d), and the other group (six men and four women) received nifedipine (30 mg/d). Circulating plasma levels of ANP, PRA, and PA were determined by radioimmunoassay, and other variables were determined by routine laboratory techniques before therapy and at day 3 and day 7 after the treatment began. Arterial blood pressure and heart rate were monitored during the study. Both drugs reduced arterial blood pressure (P less than .001) significantly. The atenolol therapy decreased heart rate (P less than .001), increased plasma ANP levels and urinary catecholamine excretion, and decreased PRA and circulating PA levels. Nifedipine treatment did not modify plasma ANP values, whereas it increased PRA and PA circulating levels and urinary catecholamine excretion. No differences were shown for urinary volume, urinary sodium, and potassium excretions during the two different treatments. These findings suggest that the increased plasma ANP levels could contribute to the antihypertensive effects of the beta-adrenoreceptor blockers, by a reduction in PRA and PA levels and a vasodilatative effect.(ABSTRACT TRUNCATED AT 250 WORDS)

A possible role of atrial natriuretic peptide in ethanol-induced acute diuresis.

The acute effects of ethanol on plasma atrial natriuretic peptide levels were investigated in 4 clinically healthy males, aged 24-26 years, consumed either 750 ml of water as a control study, or the same beverage with 1 ml/kg alcohol added, which increased the plasma alcohol concentration to 99.12 +/- 15.10 mg/dl at 60 min. Plasma atrial natriuretic peptide levels were significantly higher in the alcohol study compared to the control study at each time point (10, 20, 30, 60, 120 min after drinking onset), and with a peak at 10 min. Atrial natriuretic peptide levels showed a positive significant correlation with plasma antidiuretic hormone in the control group, while no relationship was found between the two peptides in the alcohol study. Moreover, a significant correlation exists between plasma atrial natriuretic peptide levels and systolic arterial blood pressure, and heart rate, and between the variations in atrial natriuretic peptide values and the variations in plasma sodium, serum ethanol, and plasma osmolality in the alcohol study. Acute ethanol intake causes an increase in urinary volume, and a decrease in urinary potassium excretion and urinary osmolality, and no change in urinary sodium excretion. These data suggest that acute ethanol administration causes a rapid increase in plasma levels of atrial natriuretic peptide, which could be an important factor of ethanol-induced diuresis. The main mechanisms for increased atrial natriuretic peptide release from atria after acute ethanol ingestion seem to be atrial stretch, due to the increase in arterial blood pressure, in heart rate, in sympathetic tone, and in plasma osmolality, and to a direct secretory effect by antidiuretic hormone.

[Atrial natriuretic peptide, renin-aldosterone system and arterial pressure. Analysis by circadian rhythm measurement]. / Peptide natriuretico atriale, sistema renina-aldosterone e pressione arteriosa. Analisi ritmometrica circadiana.

Six voluntary, clinically healthy, non-smoking, male subjects were studied to estimate and eventually quantify the role of the circadian rhythm of atrial natriuretic peptide and of the renin-aldosterone system in the conditioning and genesis of the circadian rhythm of arterial blood pressure. After a week of standard life condition, during the span of a day, with the subjects in constant supine position, venous blood samples were drawn every four hours, while arterial blood pressure was measured every two hours. Plasma levels of atrial natriuretic peptide, renin activity, and aldosterone were determined by radioimmunoassay. The time-related values of each variable were analysed by the "cosinor" method. The cosinor analysis shows a statistically significant (p less than 0.05) circadian rhythm for all variables studied. These data suggest an inverse relationship between the circadian rhythm of atrial natriuretic peptide and that of arterial blood pressure, with a chronological sequence in the atrial natriuretic peptide-plasma renin activity-aldosterone axis.

[Circadian rhythm of atrial natriuretic peptide, plasma renin and aldosterone activity in healthy subjects and in patients with compensated liver cirrhosis]. / Ritmo circadiano del peptide natriuretico atriale, dell'attività reninica plasmatica e dell'aldosterone in soggetti ed in pazienti con cirrosi epatica compensata.

The circadian variations in atrial natriuretic peptide (ANP), plasma renin activity (PRA) and plasma aldosterone (PA) have been investigated in a group of 6 patients with compensated cirrhosis of the liver compared with a group of 6 healthy subjects. All studied subjects were kept for a week on standardized life conditions, with a defined daily intake of 120 mEq of sodium and 60 mEq of potassium. Venous blood samples were collected during a whole day at 6, 8, 12, 18, 20 and 24 hours, with the subjects resting in the clinostatic position during the study. Plasma levels of ANP, PRA and PA were determined by radioimmunoassay. The data were analyzed by the cosinor method. The results show that healthy subjects present a significant circadian rhythm for the three biological variables, while patients with cirrhosis of the liver present a significant rhythm for PA only. Acrophase and amplitude of PA do not present any difference between control and patient groups. The levels of PRA and ANP are significantly higher in the cirrhotic patients. These data suggest in cirrhosis a deep variation in the secreting rhythm of PRA and ANP with maintenance, even at higher levels, of intrinsic PA rhythm. This is a possible index of time-related alterations of water-electrolyte balance and cardiovascular processes in liver cirrhosis.

Atrial natriuretic peptide-renin-aldosterone system in cirrhosis of the liver: circadian study.

Plasma levels of immunoreactive atrial natriuretic peptide (ANP), plasma renin activity (PRA), and plasma aldosterone (PA) were measured for an entire day at 6:00 am, 8:00 am, 12:00 pm, 6:00 pm, 8:00 pm, and 12:00 am in 6 healthy subjects, in 10 patients with compensated cirrhosis of the liver, and in 10 cirrhotics with ascites. The subjects, after synchronized standard life conditions lasting for 6 days were held in a clinostatic position during the study. The data were analyzed by the "cosinor" method. The results show significant circadian rhythms for the three biological variables in healthy subjects. In the compensated cirrhotic group, a circadian rhythm was detected only for PA. No rhythm was demonstrated in the ascitic patients. These data suggest that in cirrhosis of the liver, great variations in secretion rhythmicity for PRA and ANP are present, while maintaining the intrinsic PA rhythmicity, which is lost in patients with ascites. This progressive derangement in PA circadian rhythm in the ANP-PRA-PA system can be considered as an index of evolution in the natural history of cirrhosis of the liver.