ABSTRACT
OBJECTIVE: Sinonasal disease can contribute to poor asthma control. There are reports that link obesity with an increased prevalence of sinonasal disease, but no studies evaluating the severity of sinonasal disease in obese asthmatics, and how this impacts asthma control. The purpose of the current study was to determine if obesity is associated with increased severity of sinonasal disease, and/or affects response to nasal corticosteroid treatment in asthma. METHODS: This study included 236 adults participating in a 24-week randomized, double-masked, placebo-controlled study of nasal mometasone for the treatment of poorly controlled asthma. Sinonasal disease severity was assessed using validated questionnaires, and compared in participants of differing BMIs. Eosinophilic inflammation was assessed using markers in nasal lavage, serum and exhaled nitric oxide. Response to treatment was compared in different BMI groups. RESULTS: Obesity had no effect on the severity of sinonasal disease symptoms in asthmatics (Sino-Nasal Outcome Test 22 (SNOT 22) score [mean ± SD] 35.4 ± 18.5, 40.2 ± 22.8, and 39.1 ± 21.7, p = 0.43, in lean, overweight and obese participants), nor on nasal, bronchial or systemic markers of allergic inflammation. Nasal steroids had some limited effects on symptoms, lung function and inflammatory markers in lean participants, but no detectable effect was found in obese patients. CONCLUSIONS: Obesity does not affect severity of sinonasal disease in patients with asthma; the association of sinonasal disease symptoms with increased asthma severity and markers of Type 2 inflammation are consistent across all BMI groups. The response of obese patients to nasal corticosteroids requires further study.
Subject(s)
Asthma , Nose Diseases , Obesity , Adult , Anti-Asthmatic Agents/therapeutic use , Asthma/drug therapy , Asthma/physiopathology , Double-Blind Method , Female , Humans , Male , Middle Aged , Mometasone Furoate/therapeutic use , Nose Diseases/drug therapy , Nose Diseases/physiopathology , Obesity/drug therapy , Obesity/physiopathology , Respiratory Function Tests , Severity of Illness Index , Young AdultABSTRACT
The PICASSO project is a cold dark matter (CDM) search experiment relying on the superheated droplet technique. The detectors use superheated freon liquid droplets (active material) dispersed and trapped in a polymerised gel. This detection technique is based on the phase transition of superheated droplets at about room temperature and ambient pressure. The phase transition is induced by nuclear recoils when an atomic nucleus in the droplets interacts with incoming subatomic particles. This includes CDM particles candidate as the neutralino (a yet-to-discover particle predicted in extensions of the standard model of particle physics). Simulations performed to understand the detector response to neutrons and alpha particles are presented along with corresponding data obtained at the Montreal Laboratory.
Subject(s)
Computer-Aided Design , Cosmic Radiation , Extraterrestrial Environment , Linear Energy Transfer , Microbubbles , Models, Chemical , Thermoluminescent Dosimetry/instrumentation , Computer Simulation , Dose-Response Relationship, Radiation , Equipment Design , Equipment Failure Analysis , Materials Testing , Radiation Dosage , Reproducibility of Results , Sensitivity and Specificity , Surface Properties , Thermoluminescent Dosimetry/methodsABSTRACT
The PICASSO experiment investigates the presence and nature of dark matter in the Universe. The experiment is based on the detection of acoustic signals generated in explosive phase transitions induced by dark matter particles. This technique is an alternative more traditional detection technique like scintillation and ionisation, which are largely employed for dark matter search. One of the main advantages of this technique, besides its sensitivity to very low nuclear recoil energies (few keV), is its excellent background suppression features. A pilot experiment consisting of six superheated droplet detectors (40 g of active mass) is presently taking data at the Sudbury Neutrino Observatory (SNO) at a depth of 2000 m. We discuss the operation, calibration and data acquisition of the experiment and also the ongoing work to increase the sensitivity and the active mass of the detectors.
Subject(s)
Cosmic Radiation , Extraterrestrial Environment , Hot Temperature , Microbubbles , Thermoluminescent Dosimetry/instrumentation , Dose-Response Relationship, Radiation , Equipment Design , Equipment Failure Analysis , Gels/chemistry , Gels/radiation effects , Materials Testing , Radiation Dosage , Reproducibility of Results , Sensitivity and Specificity , Surface Properties , Thermoluminescent Dosimetry/methodsABSTRACT
A rare case of hydatidiform mole occurring 7 consecutive times in a Chinese woman is presented. She was first seen in 1979 at the age of 23 years, with a molar pregnancy and subsequently had 6 consecutive moles, the last being in July, 1986; at this visit the patient and her husband were very depressed, and convinced that a normal pregnancy was unlikely and requested a hysterectomy. They were warned earlier several times, of the possible long-term consequences of a recurrent mole and that their chance of having a normal baby was very remote. A total hysterectomy was performed at her last presentation as the patient requested one, instead of dilatation and curettage for a persistently high HCG and bulky uterus following suction evacuation. Histology revealed an invasive mole. The beta HCG level was less than 4IU/l by the end of September, 1986 and she is still being followed-up.
