Observation of Gravitational Waves from a Binary Black Hole Merger

On September 14, 2015 at 09:50:45 UTC the two detectors of the Laser Interferometer Gravitational-Wave Observatory simultaneously observed a transient gravitational-wave signal. The signal sweeps upwards in frequency from 35 to 250 Hz with a peak gravitational-wave strain of 1.0×10(-21). It matches the waveform predicted by general relativity for the inspiral and merger of a pair of black holes and the ringdown of the resulting single black hole. The signal was observed with a matched-filter signal-to-noise ratio of 24 and a false alarm rate estimated to be less than 1 event per 203,000 years, equivalent to a significance greater than 5.1σ. The source lies at a luminosity distance of 410(-180)(+160)  Mpc corresponding to a redshift z=0.09(-0.04)(+0.03). In the source frame, the initial black hole masses are 36(-4)(+5)M⊙ and 29(-4)(+4)M⊙, and the final black hole mass is 62(-4)(+4)M⊙, with 3.0(-0.5)(+0.5)M⊙c(2) radiated in gravitational waves. All uncertainties define 90% credible intervals. These observations demonstrate the existence of binary stellar-mass black hole systems. This is the first direct detection of gravitational waves and the first observation of a binary black hole merger.

GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

On August 17, 2017 at 12∶41:04 UTC the Advanced LIGO and Advanced Virgo gravitational-wave detectors made their first observation of a binary neutron star inspiral. The signal, GW170817, was detected with a combined signal-to-noise ratio of 32.4 and a false-alarm-rate estimate of less than one per 8.0×10^{4}  years. We infer the component masses of the binary to be between 0.86 and 2.26  M_{⊙}, in agreement with masses of known neutron stars. Restricting the component spins to the range inferred in binary neutron stars, we find the component masses to be in the range 1.17-1.60  M_{⊙}, with the total mass of the system 2.74_{-0.01}^{+0.04}M_{⊙}. The source was localized within a sky region of 28  deg^{2} (90% probability) and had a luminosity distance of 40_{-14}^{+8}  Mpc, the closest and most precisely localized gravitational-wave signal yet. The association with the γ-ray burst GRB 170817A, detected by Fermi-GBM 1.7 s after the coalescence, corroborates the hypothesis of a neutron star merger and provides the first direct evidence of a link between these mergers and short γ-ray bursts. Subsequent identification of transient counterparts across the electromagnetic spectrum in the same location further supports the interpretation of this event as a neutron star merger. This unprecedented joint gravitational and electromagnetic observation provides insight into astrophysics, dense matter, gravitation, and cosmology.

GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence

We report the observation of a gravitational-wave signal produced by the coalescence of two stellar-mass black holes. The signal, GW151226, was observed by the twin detectors of the Laser Interferometer Gravitational-Wave Observatory (LIGO) on December 26, 2015 at 03:38:53 UTC. The signal was initially identified within 70 s by an online matched-filter search targeting binary coalescences. Subsequent off-line analyses recovered GW151226 with a network signal-to-noise ratio of 13 and a significance greater than 5σ. The signal persisted in the LIGO frequency band for approximately 1 s, increasing in frequency and amplitude over about 55 cycles from 35 to 450 Hz, and reached a peak gravitational strain of 3.4_{-0.9}^{+0.7}×10^{-22}. The inferred source-frame initial black hole masses are 14.2_{-3.7}^{+8.3}M_{⊙} and 7.5_{-2.3}^{+2.3}M_{⊙}, and the final black hole mass is 20.8_{-1.7}^{+6.1}M_{⊙}. We find that at least one of the component black holes has spin greater than 0.2. This source is located at a luminosity distance of 440_{-190}^{+180}  Mpc corresponding to a redshift of 0.09_{-0.04}^{+0.03}. All uncertainties define a 90% credible interval. This second gravitational-wave observation provides improved constraints on stellar populations and on deviations from general relativity.

GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2

We describe the observation of GW170104, a gravitational-wave signal produced by the coalescence of a pair of stellar-mass black holes. The signal was measured on January 4, 2017 at 10∶11:58.6 UTC by the twin advanced detectors of the Laser Interferometer Gravitational-Wave Observatory during their second observing run, with a network signal-to-noise ratio of 13 and a false alarm rate less than 1 in 70 000 years. The inferred component black hole masses are 31.2_{-6.0}^{+8.4}M_{⊙} and 19.4_{-5.9}^{+5.3}M_{⊙} (at the 90% credible level). The black hole spins are best constrained through measurement of the effective inspiral spin parameter, a mass-weighted combination of the spin components perpendicular to the orbital plane, χ_{eff}=-0.12_{-0.30}^{+0.21}. This result implies that spin configurations with both component spins positively aligned with the orbital angular momentum are disfavored. The source luminosity distance is 880_{-390}^{+450}  Mpc corresponding to a redshift of z=0.18_{-0.07}^{+0.08}. We constrain the magnitude of modifications to the gravitational-wave dispersion relation and perform null tests of general relativity. Assuming that gravitons are dispersed in vacuum like massive particles, we bound the graviton mass to m_{g}≤7.7×10^{-23}  eV/c^{2}. In all cases, we find that GW170104 is consistent with general relativity.

GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence

On August 14, 2017 at 10∶30:43 UTC, the Advanced Virgo detector and the two Advanced LIGO detectors coherently observed a transient gravitational-wave signal produced by the coalescence of two stellar mass black holes, with a false-alarm rate of ≲1 in 27 000 years. The signal was observed with a three-detector network matched-filter signal-to-noise ratio of 18. The inferred masses of the initial black holes are 30.5_{-3.0}^{+5.7}M_{⊙} and 25.3_{-4.2}^{+2.8}M_{⊙} (at the 90% credible level). The luminosity distance of the source is 540_{-210}^{+130}  Mpc, corresponding to a redshift of z=0.11_{-0.04}^{+0.03}. A network of three detectors improves the sky localization of the source, reducing the area of the 90% credible region from 1160   deg^{2} using only the two LIGO detectors to 60  deg^{2} using all three detectors. For the first time, we can test the nature of gravitational-wave polarizations from the antenna response of the LIGO-Virgo network, thus enabling a new class of phenomenological tests of gravity.

GW170817: Measurements of Neutron Star Radii and Equation of State

On 17 August 2017, the LIGO and Virgo observatories made the first direct detection of gravitational waves from the coalescence of a neutron star binary system. The detection of this gravitational-wave signal, GW170817, offers a novel opportunity to directly probe the properties of matter at the extreme conditions found in the interior of these stars. The initial, minimal-assumption analysis of the LIGO and Virgo data placed constraints on the tidal effects of the coalescing bodies, which were then translated to constraints on neutron star radii. Here, we expand upon previous analyses by working under the hypothesis that both bodies were neutron stars that are described by the same equation of state and have spins within the range observed in Galactic binary neutron stars. Our analysis employs two methods: the use of equation-of-state-insensitive relations between various macroscopic properties of the neutron stars and the use of an efficient parametrization of the defining function p(ρ) of the equation of state itself. From the LIGO and Virgo data alone and the first method, we measure the two neutron star radii as R_{1}=10.8_{-1.7}^{+2.0}  km for the heavier star and R_{2}=10.7_{-1.5}^{+2.1}  km for the lighter star at the 90% credible level. If we additionally require that the equation of state supports neutron stars with masses larger than 1.97  M_{⊙} as required from electromagnetic observations and employ the equation-of-state parametrization, we further constrain R_{1}=11.9_{-1.4}^{+1.4}  km and R_{2}=11.9_{-1.4}^{+1.4}  km at the 90% credible level. Finally, we obtain constraints on p(ρ) at supranuclear densities, with pressure at twice nuclear saturation density measured at 3.5_{-1.7}^{+2.7}×10^{34}  dyn cm^{-2} at the 90% level.

Tests of General Relativity with GW150914

The LIGO detection of GW150914 provides an unprecedented opportunity to study the two-body motion of a compact-object binary in the large-velocity, highly nonlinear regime, and to witness the final merger of the binary and the excitation of uniquely relativistic modes of the gravitational field. We carry out several investigations to determine whether GW150914 is consistent with a binary black-hole merger in general relativity. We find that the final remnant's mass and spin, as determined from the low-frequency (inspiral) and high-frequency (postinspiral) phases of the signal, are mutually consistent with the binary black-hole solution in general relativity. Furthermore, the data following the peak of GW150914 are consistent with the least-damped quasinormal mode inferred from the mass and spin of the remnant black hole. By using waveform models that allow for parametrized general-relativity violations during the inspiral and merger phases, we perform quantitative tests on the gravitational-wave phase in the dynamical regime and we determine the first empirical bounds on several high-order post-Newtonian coefficients. We constrain the graviton Compton wavelength, assuming that gravitons are dispersed in vacuum in the same way as particles with mass, obtaining a 90%-confidence lower bound of 10^{13}  km. In conclusion, within our statistical uncertainties, we find no evidence for violations of general relativity in the genuinely strong-field regime of gravity.

The use of ginger (Zingiber officinale Rosc.) as a potential anti-inflammatory and antithrombotic agent

The effect of an aqueous extract of ginger (Zingiber officinale) on serum cholesterol and triglyceride levels as well as platelet thromboxane-B(2) and prostaglandin-E(2) production was examined. A raw aqueous extract of ginger was administered daily for a period of 4 weeks, either orally or intraperitoneally (IP) to rats. Fasting blood serum was investigated for thromboxane-B(2), prostaglandin-E(2), cholesterol and triglycerides. A low dose of ginger (50 mg/kg) administered either orally or IP did not produce any significant reduction in the serum thromboxane-B(2) levels when compared to saline-treated animals. However, ginger administered orally caused significant changes in the serum PGE(2) at this dose. High doses of ginger (500 mg/kg) were significantly effective in lowering serum PGE(2) when given either orally or IP. However, TXB(2) levels were significantly lower in rats given 500 mg/kg ginger orally but not IP. A significant reduction in serum cholesterol was observed when a higher dose of ginger (500 mg/kg) was administered. At a low dose of ginger (50 mg/kg), a significant reduction in the serum cholesterol was observed only when ginger was administered IP. No significant changes in serum triglyceride levels were observed upon administration of either the low or high dose of ginger. These results suggest that ginger could be used as an cholesterol-lowering, antithrombotic and anti-inflammatory agent.

Management of failed cycles in an IVF/GIFT programme with the combination of a GnRH analogue and HMG

The addition of the gonadotropin releasing hormone (GnRH) agonist Buserelin to human menopausal gonadotrophin/human chorionic gonadotropin (HMG/HCG) during ovarian stimulation was evaluated in 23 cycles of 21 women who previously had unsuccessful IVF treatments when stimulated with clomiphene--HMG/HCG. No adverse effects of GnRH-agonist on folliculogenesis were seen. A mean number of 7.2 oocytes per retrieval was collected in 20 treatment cycles. Oocytes quality, fertilization and cleavage parameters were normal. Replacements by gamete intra-Fallopian transfer (GIFT) or IVF took place for 16 patients. Four patients became pregnant in their treatment cycle, one aborted. For 8 patients 18 embryos were cryopreserved, one transfer of a frozen--thawed embryo in a subsequent natural cycle led to a pregnancy. Inadequate luteal phases were constantly observed when supplementation was omitted. Further study is required to confirm that systematic luteal support improves the pregnancy rate.

The luteal phase and early pregnancy after combined GnRH-agonist/HMG treatment for superovulation in IVF or GIFT

Endometrial biopsies showing inadequate development were observed after ovarian stimulation with the GnRH agonist Buserelin and HMG for IVF or GIFT when luteal supplementation was omitted. Ninety-one patients were randomly allocated to two luteal supplementation regimens: in 41 women HCG and in 50 women progesterone and oestradiol valerate. The pregnancy patients treated with a combination of the GnRH agonist and HMG a delay of implantation of 1.3 days was observed compared to pregnancies after clomiphene citrate-HMG stimulation. This delay was not due to slower preimplantation embryo development after GnRH agonist-HMG treatment. Temporarily defective function of the corpus luteum was evidenced by measuring serum progesterone, 17 beta-oestradiol and 17-hydroxyprogesterone in the patients receiving progesterone and oestradiol valerate. This inadequate corpus luteum function could be related to the prolonged blockage of pituitary gonadotrophic function after arrest of the GnRH agonist.

Calcium pump isoforms: diversity, selectivity and plasticity. Review article

Ca2+ pumps are essential for removing cytosolic Ca2+ either across the plasma membrane (PM) or into internal organelles such as the sarcoplasmic reticulum (SR). Four genes (PMCA1, PMCA2, PMCA3 and PMCA4) have been reported to encode the PM Ca2+ pumps and three (SERCA1, SERCA2 and SERCA3) to encode the SR Ca2+ pumps. The PM Ca2+ pumps are stimulated by calmodulin, the SR Ca2+ pumps encoded by SERCA1 and SERCA2 are stimulated by phospholamban while the product of SERCA3 may be regulated directly by cAMP-dependent protein kinase. Alternative splicing of the primary transcripts of several of these genes has been reported to occur in a tissue selective manner and for others to alter during ontogeny. For the PM Ca2+ pump, alternative RNA splicing may result in isoforms with altered cyclic nucleotide dependent protein kinase sensitivity. The diversity in distribution of Ca2+ pump isoforms and their regulatory factors when coupled with different Ca2+ entry mechanisms allows for tissue selectivity and plasticity in stimulus-response coupling. The roles of various Ca2+ pump isoforms, the rationale behind their tissue selective expression and the plasticity in this expression are among the new challenges to researchers in this field.

Drug absorption in vitro model: filter-immobilized artificial membranes. 2. Studies of the permeability properties of lactones in Piper methysticum Forst

The assessment of transport properties of 23 drug and natural product molecules was made using the in vitro model based on filter-immobilized artificial membranes (filter-IAM), assembled from phosphatidylcholine in dodecane, in buffer solutions at pH 7.4. Five of the compounds were lactones extracted from the roots of the kava-kava plant. Experiments were designed to test the effects of stirring (0-600 rpm) during assays and the effects of varying the assay times (2-15 h). The highly mobile kava lactones permeated in the order dihydromethisticin (40)>yangonin (37)>kavain (34)>methisticin (32)>desmethoxyyangonin (26), the numbers in parentheses being the measured effective permeabilities in units of 10(-6) cm/s. By comparison, commercial drugs ranked: phenazopyridine (35)>testosterone (19)>propranolol (13)>ketoconazole (6.3)>piroxicam (2.2)>caffeine (1.7)>metoprolol (0.8)>terbutaline (0.01). In addition to permeability measurements, membrane retention of compounds was determined. Yangonin, desmethoxyyangonin, ketoconazole, and phenazopyridine were more than 60% retained by the artificial membranes containing phospholipids. Stirring during assay significantly increased the observed permeabilities for highly mobile molecules, but had minimal impact on the poorly permeable molecules. The influence of hydrogen bonding was explored by determining permeabilities using filters coated with dodecane free of phospholipids. In the filter-IAM method, concentrations were determined by microtitre plate UV spectrophotometry and by LC-MS. Higher-throughput was achieved with direct UV by the use of 96-well microtitre plate formats and with LC-MS by the use of cassette dosing (five-in-one).

Curcumin attenuates inflammation through inhibition of TLR-4 receptor in experimental colitis

Curcumin, an active ingredient of Curcumin longa mediates its anti-inflammatory effects through inhibition of NFkB. Several pathways including toll-like receptors (TLR) induce NFkB leading to inflammation. In this study, we investigated the effects of curcumin on the expression of TLR-4 and MyD88, the upstream signaling pathway in experimental colitis induced in the Sprague-Dawley male rats by intra-rectal administration of trinitrobenzenesulfonic acid (TNBS). The animals which received TNBS were divided into two groups: Group 1, received aqueous suspension of curcumin (100 mg/Kg body weight) 2 h prior to inducing colitis, and the treatment was repeated every day for 5 days, and Group 2 and non-colitis (Group 3) animals received phosphate buffered saline (PBS) in a similar fashion. Non-colitis animals (Group 4) received curcumin and served as controls. Animals were sacrificed on day 5 post-TNBS by cervical dislocation, colon was taken out, and cleaned with PBS. Levels of TLR-4, MyD88, and NFkB proteins were measured using ECL Western blot analysis, and TLR-4 mRNA by a competitive RT-PCR method. Colitis was confirmed histologically by measuring myeloperoxidase (MPO) activity and malondialdehyde (MDA) levels in the colonic tissues. TNBS-induced increase in the level of MPO activity and MDA concentrations was reversed by curcumin treatment, whereas the same dose of curcumin did not affect their levels in the non-colitis animals. Increases in the levels of TLR-4, MyD88, and NFkB proteins in inflamed tissue were also suppressed significantly by curcumin treatment. The level of TLR-4 mRNA remained unchanged in the colitis animals. These findings demonstrate that signaling pathway of curcumin-induced inhibition of inflammation involves TLR-4 and MyD88, and therefore may serve as an important therapeutic target in IBD.

Previous inflammation alters the response of the rat colon to stress

BACKGROUND & AIMS

Patients with inflammatory bowel disease have symptoms of irritable bowel syndrome (IBS) with a higher than expected prevalence. Stress is an important factor in the pathogenesis of IBS. Thus, previous inflammation may predispose to IBS by rendering the bowel more susceptible to the impact of stress. The aim of this study was to examine the effect of previous colitis on stress-induced responses in rats.

METHODS

Acute colitis was induced in rats by intrarectal administration of trinitrobenzene sulfonic acid (TNBS), and the rats were allowed to recover for 6 weeks before application of mild restraint stress for 3 consecutive days. In vitro measurements included myeloperoxidase activity, plasma corticosterone levels, interleukin 1 beta messenger RNA expression, and [3H]noradrenaline release from the myenteric plexus.

RESULTS

Six weeks after administration of TNBS, stress caused a significant increase in myeloperoxidase activity in TNBS-treated rats but not in stressed controls; plasma corticosterone responses were similar. Stress also caused an exaggerated and significant suppression of [3H]noradrenaline release in TNBS-treated stressed rats compared with stressed controls. This was accompanied by a significant decrease in interleukin 1 beta messenger RNA expression in the colon.

CONCLUSIONS

Previous colitis rendered the colon more susceptible to effects of stress on enteric nerve function and also increased some parameters of inflammation in response to stress.

Glanders in animals: a review on epidemiology, clinical presentation, diagnosis and countermeasures

Glanders or farcy, caused by Burkholderia mallei, is an infectious and zoonotic disease of solipeds. Horses, donkeys and mules are the only known natural reservoir of B. mallei. Although glanders has been eradicated from most countries, it has regained the status of a re-emerging disease because of the numerous recent outbreaks. Pre-symptomatic or carrier animals are the potential source of infection for the healthy equine population and play a crucial role in the spreading of the infectious agent. Glanders is characterized by ulcerating nodular lesions of the skin and mucous membrane. Generalized symptoms include fever, malaise, depression, cough, anorexia and weight loss. Burkholderia mallei can invade its host through mucous membranes, gastrointestinal tract and the integument. Its virulence mechanisms and pathogenesis are not yet completely understood. A major problem when using serological tests for diagnosing glanders is the occurrence of false-positive and false-negative results leading to difficulties in international trade with equids and to the spread of glanders to disease-free regions. Moreover, poor tests critically result in poor control of disease. These tests are not only incapable of discriminating between B. mallei and B. pseudomallei antibodies, they are also unable to differentiate between malleinized and naturally infected animals. Combined use of both serological and molecular detection methods increases the detection rate of glanders. Countermeasures against glanders include early detection of disease in susceptible animals, stringent quarantine measures, testing and safe destruction of infected carcasses, adequate compensation to the animal owners, disinfection of infected premises and awareness about glanders and the zoonotic implications through veterinary extension services. An account of the clinical picture and successful experimental therapy of spontaneous equine glanders is also given.

SOCCAR: A randomised phase II trial comparing sequential versus concurrent chemotherapy and radical hypofractionated radiotherapy in patients with inoperable stage III Non-Small Cell Lung Cancer and good performance status

BACKGROUND

Cure of lung cancer is impossible without local tumour control. This can be compromised by accelerated repopulation of tumour cells during radiotherapy and chemotherapy. A strategy to minimise accelerated repopulation might improve local control. We investigated whether concurrent chemo-radiotherapy could be given safely over four weeks.

METHODS

We conducted a randomised phase II trial in which patients with inoperable Stage III Non-Small Cell Lung Cancer (NSCLC) received a radical radiation dose over four weeks rather than conventional fractionation. Treatment was given either sequentially or concurrently with three to four cycles of cisplatinum and vinorelbine. 130 patients with inoperable stage III NSCLC and PS 0-1 were randomised to receive cisplatinum and vinorelbine with either sequential or concurrent chemo-radiation using 55Gy in 20 fractions over four weeks. The primary end-point was treatment related mortality. Secondary end-points were toxicity and survival.

FINDINGS

Treatment related mortality was: 2.9% (exact 95% confidence interval [CI] 0.36-10.2%) and 1.7% (exact 95% CI 0.043-9.1%) for the Concurrent and Sequential group respectively; relative risk (RR) 1.25; (95% CI 0.55, 2.84). Toxicity was similar between arms; grade 3 or worse oesophagitis was 8.8% versus 8.5%; RR 1.02 (95% CI 0.58, 1.79). OS HR was 0.92; 95% CI (0.60-1.39; p=0.682). The 2 year overall survival rates were: 50% versus 46%; RR 1.06 (95% CI 0.77, 1.46) for Concurrent versus Sequential.

INTERPRETATION

A strategy to minimise the effects of accelerated repopulation using accelerated hypofractionated radiotherapy with chemotherapy is feasible, and reasonably safe for patients with stage III NSCLC. The reported two year survival is promising and suggests that a four week regime of radiotherapy should be compared with conventionally fractionated radiotherapy in an adequately powered randomised controlled phase III trial.

Properties of the Binary Black Hole Merger GW150914

On September 14, 2015, the Laser Interferometer Gravitational-Wave Observatory (LIGO) detected a gravitational-wave transient (GW150914); we characterize the properties of the source and its parameters. The data around the time of the event were analyzed coherently across the LIGO network using a suite of accurate waveform models that describe gravitational waves from a compact binary system in general relativity. GW150914 was produced by a nearly equal mass binary black hole of masses 36_{-4}^{+5}M_{⊙} and 29_{-4}^{+4}M_{⊙}; for each parameter we report the median value and the range of the 90% credible interval. The dimensionless spin magnitude of the more massive black hole is bound to be <0.7 (at 90% probability). The luminosity distance to the source is 410_{-180}^{+160}  Mpc, corresponding to a redshift 0.09_{-0.04}^{+0.03} assuming standard cosmology. The source location is constrained to an annulus section of 610  deg^{2}, primarily in the southern hemisphere. The binary merges into a black hole of mass 62_{-4}^{+4}M_{⊙} and spin 0.67_{-0.07}^{+0.05}. This black hole is significantly more massive than any other inferred from electromagnetic observations in the stellar-mass regime.

Increasing the Astrophysical Reach of the Advanced Virgo Detector via the Application of Squeezed Vacuum States of Light

Current interferometric gravitational-wave detectors are limited by quantum noise over a wide range of their measurement bandwidth. One method to overcome the quantum limit is the injection of squeezed vacuum states of light into the interferometer's dark port. Here, we report on the successful application of this quantum technology to improve the shot noise limited sensitivity of the Advanced Virgo gravitational-wave detector. A sensitivity enhancement of up to 3.2±0.1  dB beyond the shot noise limit is achieved. This nonclassical improvement corresponds to a 5%-8% increase of the binary neutron star horizon. The squeezing injection was fully automated and over the first 5 months of the third joint LIGO-Virgo observation run O3 squeezing was applied for more than 99% of the science time. During this period several gravitational-wave candidates have been recorded.

In vitro and in vivo effects of the triazolobenzodiazepine alprazolam on hypothalamic-pituitary-adrenal function: pharmacological and clinical implications

We report here a study of the effects of alprazolam on in vivo pituitary-adrenal function in jacketed nonrestrained nonhuman primates and on in vitro CRH release from rat hypothalami and ACTH release from rat dispersed anterior pituicytes. We undertook this study because alprazolam is the only benzodiazepine effective in treating both major depressive and anxiety disorders, and recent data suggest that the hypercortisolism of major depression reflects hypersecretion of CRH. Moreover, the intracerebroventricular administration of CRH can reproduce many of the components of the symptom complex of major depression, including not only hypercortisolism, but also hypothalamic hypogonadism, decreased libido, anorexia, and intense anxiety. As a comparison, we also assessed the effects of diazepam on in vitro CRH release, because in contrast to alprazolam, diazepam is effective in anxiety states but not in depression. Alprazolam (0.01-0.3 mg/kg, iv) produced a dose-dependent inhibition of both plasma ACTH and cortisol secretion in non-restrained adult male rhesus monkeys. Our in vitro studies showed that alprazolam significantly inhibited serotonin (5HT)-induced CRH release in a dose-dependent fashion (10(-10)-10(-5) M). Diazepam also inhibited 5HT-induced CRH release, but was 40 times less potent than alprazolam. Alprazolam was ineffective in blocking basal or CRH-induced ACTH release from rat dispersed anterior pituicytes, suggesting that its in vivo effects are through inhibition of CRH secretion. As expected, the inactive benzodiazepine ligand Ro 15-1788 inhibited the effects of alprazolam on 5HT-induced CRH release, but this occurred only at doses below 10(-7) M. Interestingly, when incubated alone in higher doses with our rat hypothalamic organ culture, Ro 15-1788, like alprazolam, produced a dose-dependent inhibition of 5HT-induced CRH release (10(-7)-10(-5) M), suggesting an agonistic action of Ro 15-1788 at the benzodiazepine receptor at higher concentrations. We conclude that alprazolam is capable of suppressing the primate pituitary-adrenal axis, and that this suppression most likely reflects suppression of the CRH neuron rather than of the pituitary corticotroph cell. We speculate that the enhanced capacity of alprazolam to suppress the CRH neuron relative to other benzodiazepines may contribute to its unique efficacy among this class of drugs in the treatment of major depression. The capacity of Ro 15-1788 to reverse alprazolam-induced suppression of the CRH neuron indicates that the effects of alprazolam are mediated at least in part via its interaction with the benzodiazepine component of the gamma-aminobutyric acidA macromolecular complex.

Sol-gel trapping of functional intermediates of hemoglobin: geminate and bimolecular recombination studies

The encapsulation of proteins in porous sol-gels is a promising technique for generating, trapping, and probing functionally significant nonequilibrium protein species. An essential step needed in the pursuit of that goal is establishing the degree to which the sol-gel limits conformational change upon adding or removing substrates. In the present study, geminate recombination and solvent phase bimolecular recombination of CO to human adult hemoglobin (HbA) are used as sensitive probes of the degree of conformational constraint within the sol-gel. Two forms of CO saturated encapsulated HbA are generated. In one case, designated [COHbA], the equilibrium form of COHbA is directly encapsulated. In the second case, designated as [deoxyHbA] + CO, the equilibrium form of deoxyHbA is encapsulated and only after the sample has aged is CO introduced to the HbA through the porous sol-gel matrix. Three different preparative protocols are used to generate the sol-gels for each of the two forms of encapsulated COHbA. The kinetic traces obtained from these encapsulated samples allow for an easy evaluation of the extent to which the sol-gel is locking in the initial tertiary/quaternary structure. The results show that the sol-gel encapsulated samples can be used with pulsed laser sources and that one of the tested encapsulation protocols is far superior with respect to conformational locking. This protocol is used to trap and probe nonequilibrium forms such as the liganded T state of HbA, a species whose properties are needed to fully explore allostery in HbA.

GW190521: A Binary Black Hole Merger with a Total Mass of 150 M_{⊙}

On May 21, 2019 at 03:02:29 UTC Advanced LIGO and Advanced Virgo observed a short duration gravitational-wave signal, GW190521, with a three-detector network signal-to-noise ratio of 14.7, and an estimated false-alarm rate of 1 in 4900 yr using a search sensitive to generic transients. If GW190521 is from a quasicircular binary inspiral, then the detected signal is consistent with the merger of two black holes with masses of 85_{-14}^{+21}  M_{⊙} and 66_{-18}^{+17}  M_{⊙} (90% credible intervals). We infer that the primary black hole mass lies within the gap produced by (pulsational) pair-instability supernova processes, with only a 0.32% probability of being below 65  M_{⊙}. We calculate the mass of the remnant to be 142_{-16}^{+28}  M_{⊙}, which can be considered an intermediate mass black hole (IMBH). The luminosity distance of the source is 5.3_{-2.6}^{+2.4}  Gpc, corresponding to a redshift of 0.82_{-0.34}^{+0.28}. The inferred rate of mergers similar to GW190521 is 0.13_{-0.11}^{+0.30}  Gpc^{-3} yr^{-1}.

Ambulatory blood pressure monitoring after renal transplantation in children

Hypertension occurs commonly following renal transplantation and may cause end organ damage, such as cardiac hypertrophy. This study seeks to determine which features of hypertension are related to cardiac hypertrophy in children after renal transplantation. Ambulatory blood pressure monitoring (ABPM) was performed in 45 pediatric patients, 4.9+/-3.0 years after renal transplantation. ABPM data were related to clinical features and echocardiographic measurements. Hypertension was demonstrated in 33% of patients by casual blood pressure (BP) measurement and in 40% by ABPM. The mean percentage nighttime decline in BP (dipping) was 8.9+/-5.0% for systolic and 13.9+/-7.7% for diastolic BP. Abnormal dipping (<10%) was seen in 58% of patients. BP load (percentage of BP recordings above 95th percentile) was >30% in 44% of patients. Patients taking antihypertensive medication had more abnormal dipping and greater nighttime BP load. The prevalence of left ventricular hypertrophy was 72% before transplantation, 75% after transplantation, and 54% near to ABPM. Left ventricular mass (LVM) indexed to height(3) decreased significantly after transplantation. (40.2+/-14.7 vs. 35.0+/-8.3 g/m(3), P=0.0002). There was no significant relationship between ABPM data and LVM. ABPM was not able to differentiate those patients with persistently elevated LVM. The results suggest that hypertension is not always associated with cardiac hypertrophy following pediatric renal transplantation.

Expression of cytokines in the longitudinal muscle myenteric plexus of the inflamed intestine of rat

BACKGROUND/AIMS

Trichinella spiralis infection in the rat produces mucosal injury and inflammation and causes changes in muscle function and neurotransmitter release in the longitudinal muscle myenteric plexus (LMMP). Whether these changes in LMMP reflect the production of inflammatory mediators in the LMMP remains unknown. The objective of this study was to investigate the profile of interleukins (IL) 1-alpha, 1-beta, and 6 and tumor necrosis factor (TNF) alpha in the LMMP of infected rats. Because muscle changes are T-cell dependent, we also studied the cytokine profile in infected athymic rats.

METHODS

Cytokine messenger RNA (mRNA) was examined using semiquantitative polymerase chain reaction, and protein was measured by enzyme-linked immunosorbent assay, radioimmunoassay, or bioassay.

RESULTS

There was increased expression of IL1-alpha and -beta, IL-6, and TNF-alpha mRNA and protein in the LMMP of both euthymic and athymic infected rats. Increased expression of each cytokine was observed by 24 hours postinfection and, in the case of IL1-beta and TNF-alpha, remained elevated by day 6 postinfection.

CONCLUSIONS

Mucosal injury following T. spiralis infection is accompanied by enhanced expression of proinflammatory cytokines in the LMMP. The expression of IL1-, IL-6, and TNF-alpha in infected athymic rats suggests that these cytokines do not contribute to the changes in muscle growth or contraction but may mediate the previously described changes in neurotransmitter release in this model.