Solar axion search with the CAST experiment

The CAST (CERN Axion Solar Telescope) experiment is searching for solar axions by their conversion into photons inside the magnet pipe of an LHC dipole. The analysis of the data recorded during the first phase of the experiment with vacuum in the magnet pipes has resulted in the most restrictive experimental limit on the coupling constant of axions to photons. In the second phase, CAST is operating with a buffer gas inside the magnet pipes in order to extent the sensitivity of the experiment to higher axion masses. We will present the first results on the $^{4}{\rm He}$ data taking as well as the system upgrades that have been operated in the last year in order to adapt the experiment for the $^{3}{\rm He}$ data taking. Expected sensitivities on the coupling constant of axions to photons will be given for the recent $^{3}{\rm He}$ run just started in March 2008.Comment: Proceedings of the ICHEP 2008 conferenc

Search for low Energy solar Axions with CAST

We have started the development of a detector system, sensitive to single photons in the eV energy range, to be suitably coupled to one of the CAST magnet ports. This system should open to CAST a window on possible detection of low energy Axion Like Particles emitted by the sun. Preliminary tests have involved a cooled photomultiplier tube coupled to the CAST magnet via a Galileian telescope and a switched 40 m long optical fiber. This system has reached the limit background level of the detector alone in ideal conditions, and two solar tracking runs have been performed with it at CAST. Such a measurement has never been done before with an axion helioscope. We will present results from these runs and briefly discuss future detector developments.Comment: Paper submitted to the proceedings of the "4th Patras Workshop on Axions, WIMPs and WISPs", DESY, Hamburg Site - Germany, 18-21 June 2008. Author affiliations are reported on the title page of the paper. In version 2: 1 affiliation change, 3 references adde

A pleomorphic rhabdomyosarcoma mimicking an inguinal hernia: A case report and review of the literature

A 59-year-old male presented with a painful right inguinal swelling and deep vein thrombosis at the ipsilateral leg. An inguinal hernia was initially diagnosed, but during surgery a large mass was found anteriorly to the peritoneal sheaths. Histology revealed a high-grade pleomorphic rhabdomyosarcoma. The mass advanced rapidly, occupying the whole right iliac fossa and metastasizing to the lung. Despite first- and second-line chemotherapy, the patient deteriorated rapidly and died. Rhabdomyosarcomas should be managed in specialized centres as they have prognostic factors and histologic features still controversial and poorly clarified. Copyright © 2012 S. Karger AG, Basel

Testicular function in poor-risk nonseminomatous germ cell tumors treated with methotrexate, paclitaxel, ifosfamide, and cisplatin combination chemotherapy

Our objective was to investigate the impact of methotrexate, paclitaxel, ifosfamide, and cisplatin (M-TIP) on long-term fertility in poor-risk nonseminomatous germ cell tumors (NSGCT). Thirty patients with poor-risk NSGCT (median age, 29 years; range, 17-62 years) were treated with methotrexate 250 mg/m2 with folinic acid rescue (day 1) and paclitaxel 175 mg/m2 (day 1), followed by ifosfamide 1.2 g/m2 and cisplatin 20 mg/m2 (days 2-6). Treatment consisted of 4 cycles of M-TIP administered every 3 weeks. Twenty-one patients were continuously disease-free at a median follow-up of 5.3 years (range, 0.9-8.4 years). Sperm count and hormonal analyses were examined prechemotherapy (30 patients) and postchemotherapy (21 patients). Counts were classified as follows: lower than 1 × 106/mL, azoospermia; 1-20 × 106/mL, oligospermia (OS); higher than 20 × 106/mL, normospermia (NS). Patients were followed for a median of 2.3 years (range, 0.9-3.8 years) postchemotherapy. The prechemotherapy median luteinizing hormone (LH) serum levels were slightly above the upper normal limit, whereas the serum levels of follicle-stimulating hormone (FSH) and testosterone (T) were within the reference interval. Eleven (52.3%) patients had NS prechemotherapy. Among the patients with NS, 72.7% still had NS following chemotherapy. Overall, 17 of 21 (80.9%; 33.3% OS and 47.6% NS) patients had recovery of spermatogenesis after treatment. The median FSH serum levels were significantly elevated at least 1 year postchemotherapy when compared with the pretreatment levels. Eighteen months after the completion of chemotherapy the median FSH levels had returned to the reference limits. Serum LH and T levels were unaffected by chemotherapy. Prior to chemotherapy 4 of 30 patients had fathered 5 children. Since completion of chemotherapy, 5 patients have fathered 5 children. The majority of men with poor-risk germ cell tumors who were treated with the M-TIP regimen demonstrated recovery spermatogenesis after treatment, and Leydig cell function was unaffected. Copyright © American Society of Andrology

Probing the eV-Mass range for solar axions with CAST

The CERN Axion Solar Telescope (CAST) is searching for solar axions which could be produced in the core of the Sun via the so-called Primakoff effect. Not only would these hypothetical particles solve the strong CP problem, but they are also one of the favored candidates for dark matter. In order to look for axions originating from the Sun, CAST uses a decommissioned LHC prototype magnet. In its 10 m long magnetic field region of 9 Tesla, axions could be reconverted into X-ray photons. Different X-ray detectors are installed on both ends of the magnet, which is mounted on a structure built to follow the Sun during sunrise and sunset for a total of about 3 hours per day. The analysis of the data acquired during the first phase of the experiment with vacuum in the magnetic field region yielded the most restrictive experimental upper limit on the axion-to-photon coupling constant for axion masses up to about 0.02 eV. In order to extend the sensitivity of the experiment to a wider mass range, the CAST experiment continues its search for axions with helium in the magnet bores. In this way it is possible to restore coherence of conversion for larger masses. Changing the pressure of the helium gas enables the experiment to scan different axion masses in the range of up to about 1.2 eV. Especially at high pressures, a precise knowledge of the gas density distribution is crucial to obtain accurate results. In the first part of this second phase of CAST, 4He was used and the axion mass region was extended up to 0.39 eV, a part of phase space favored by axion models. In CAST's ongoing 3He phase the studied mass range is now being extended further. In this contribution the final results of CAST's 4He phase will be presented and the current status of the 3He run will be given. This includes latest results as well as prospects of future axion experiments

Probing the eV-Mass range for solar axions with CAST

Çetin, Serkant Ali (Dogus Author) -- Yıldız, Süleyman C. (Dogus Author) -- Conference full title: 2010 IEEE Nuclear Science Symposium conference record (NSS/MIC 2010) : [including the 2010 IEEE Nuclear Science Symposium, Medical Imaging Conference, and the 17th International Workshop on Room-Temperature Semiconductor X-Ray and Gamma-Ray Detectors (RTSD)]; Knoxville, Tennessee, USA, 30 October - 6 November 2010The CERN Axion Solar Telescope (CAST) is searching for solar axions which could be produced in the core of the Sun via the so-called Primakoff effect. Not only would these hypothetical particles solve the strong CP problem, but they are also one of the favored candidates for dark matter. In order to look for axions originating from the Sun, CAST uses a decommissioned LHC prototype magnet. In its 10 m long magnetic field region of 9 Tesla, axions could be reconverted into X-ray photons. Different X-ray detectors are installed on both ends of the magnet, which is mounted on a structure built to follow the Sun during sunrise and sunset for a total of about 3 hours per day. The analysis of the data acquired during the first phase of the experiment with vacuum in the magnetic field region yielded the most restrictive experimental upper limit on the axion-to-photon coupling constant for axion masses up to about 0.02 eV. In order to extend the sensitivity of the experiment to a wider mass range, the CAST experiment continues its search for axions with helium in the magnet bores. In this way it is possible to restore coherence of conversion for larger masses. Changing the pressure of the helium gas enables the experiment to scan different axion masses in the range of up to about 1.2 eV. Especially at high pressures, a precise knowledge of the gas density distribution is crucial to obtain accurate results. In the first part of this second phase of CAST, 4He was used and the axion mass region was extended up to 0.39 eV, a part of phase space favored by axion models. In CAST's ongoing 3He phase the studied mass range is now being extended further. In this contribution the final results of CAST's 4He phase will be presented and the current status of the 3He run will be given. This includes latest results as well as prospects of future axion experiments.Nucl. Plasma Sci. Soc. Inst. Electr. Electron. Eng. (NPSS

CAST: Recent results & future outlook

The CAST (CERN Axion Solar Telescope) experiment is searching for solar axions by their conversion into photons inside the magnet pipes of an LHC dipole. The analysis of data taken so far has shown no signal above the background, thus implying an upper limit to the axion-photon coupling of ga\u3b3 < 0.85 7 10 1210GeV 121 at 95% CL for ma < 0.02 eV/c2. Ongoing measurements, with the magnet bores filled with a buffer gas (3He), are improving the sensitivity of the experiment for higher axion masses towards 1 eV/c2. Recent results, new ideas for Axion-Like Particle (WISPs) searches with CAST in the near future and the prospects of a new generation Helioscope are presented here