THE TRANSLATION PRODUCTS OF MOLONEY MURINE SARCOMA VIRUS 124 GENOMIC RNA

Murine sarcoma viruses constitute a class of replication-defective retroviruses. Cellular transformation may be induced by these viruses in vitro; whereas, fibrosarcomas may result in animals infected with them in vivo (Tooze, 1973; Bishop, 1978). Hybridization studies suggest that murine sarcoma viruses arose by recombination between nondefective murine leukemia virus sequences and certain cellular sequences present in uninfected mouse cells (Hu et al., 1977). A specific gene product, however, has not been implicated in murine sarcoma virus transformation.^ One line of murine sarcoma virus-producing cells, Mo-MuSV-clone 124, (Ball et al., 1973), was studied biochemically because it mainly produces the sarcoma virus as a pseudotype packaged with helper murine leukemia virus proteins. The sarcoma viral RNA was translated in a sophisticated cell-free protein synthesizing system (Murphy and Arlinghaus, 1978). The translation products were analyzed by a number of techniques, including electrophoresis in denaturing gels of SDS polyacrylamide, immunoprecipitation, and peptide mapping. The major products of the total RNA purified from the virus preparation were shown to have molecular weights of about 63,000 (P63('gag)), 42,000 (P42), 40,000 (P40), 38,000 (P38), and 23,000 (P23). The size class of mRNA coding for each of the cell-free products was estimated using a poly(A) selection technique and sucrose gradient fractionation. These analyses were used to localize the coding information related to each of the in vitro synthesized cell-free products within the sarcoma virus genome.^ The major findings of these studies were: (1) the 5' half of the sarcoma viral RNA codes for the 63,000 dalton polypeptide and 42,000 - 38,000 dalton polypeptides derived from the "gag" gene; and (2) the 3' half of the sarcoma viral RNA codes for a 38,000 dalton polypeptide and possibly derived from the cellular acquired sequences. ^

Response of liquid xenon to Compton electrons down to 1.5 keV

The response of liquid xenon to low-energy electronic recoils is relevant in the search for dark-matter candidates which interact predominantly with atomic electrons in the medium, such as axions or axionlike particles, as opposed to weakly interacting massive particles which are predicted to scatter with atomic nuclei. Recently, liquid-xenon scintillation light has been observed from electronic recoils down to 2.1 keV, but without applied electric fields that are used in most xenon dark-matter searches. Applied electric fields can reduce the scintillation yield by hindering the electron-ion recombination process that produces most of the scintillation photons. We present new results of liquid xenon's scintillation emission in response to electronic recoils as low as 1.5 keV, with and without an applied electric field. At zero field, a reduced scintillation output per unit deposited energy is observed below 10 keV, dropping to nearly 40% of its value at higher energies. With an applied electric field of 450 V/cm, we observe a reduction of the scintillation output to about 75% relative to the value at zero field. We see no significant energy dependence of this value between 1.5 and 7.8 keV. With these results, we estimate the electronic-recoil energy thresholds of ZEPLIN-III, XENON10, XENON100, and XMASS to be 2.8, 2.5, 2.3, and 1.1 keV, respectively, validating their excellent sensitivity to low-energy electronic recoils.

Dual-Phase Liquid Xenon Detectors for Dark Matter Searches

Dual-phase time projection chambers (TPCs) filled with the liquid noble gas xenon (LXe) are currently the most sensitive detectors searching for interactions of WIMP dark matter in a laboratory-based experiment. This is achieved by combining a large, monolithic dark matter target of a very low background with the capability to localize the interaction vertex in three dimensions, allowing for target fiducialization and multiple-scatter rejection. The background in dual-phase LXe TPCs is further reduced by the simultaneous measurement of the scintillation and ionization signal from a particle interaction, which is used to distinguish signal from background signatures. This article reviews the principle of dual-phase LXe TPCs, and provides an overview about running as well as future experimental efforts.

Neutrino physics with multi-ton scale liquid xenon detectors

We study the sensitivity of large-scale xenon detectors to low-energy solar neutrinos, to coherent neutrino-nucleus scattering and to neutrinoless double beta decay. As a concrete example, we consider the xenon part of the proposed DARWIN (Dark Matter WIMP Search with Noble Liquids) experiment. We perform detailed Monte Carlo simulations of the expected backgrounds, considering realistic energy resolutions and thresholds in the detector. In a low-energy window of 2–30 keV, where the sensitivity to solar pp and 7Be-neutrinos is highest, an integrated pp-neutrino rate of 5900 events can be reached in a fiducial mass of 14 tons of natural xenon, after 5 years of data. The pp-neutrino flux could thus be measured with a statistical uncertainty around 1%, reaching the precision of solar model predictions. These low-energy solar neutrinos will be the limiting background to the dark matter search channel for WIMP-nucleon cross sections below ~2X 10-48 cm2 and WIMP masses around 50 GeV c 2, for an assumed 99.5% rejection of electronic recoils due to elastic neutrino-electron scatters. Nuclear recoils from coherent scattering of solar neutrinos will limit the sensitivity to WIMP masses below ~6 GeV c-2 to cross sections above ~4X10-45cm2. DARWIN could reach a competitive half-life sensitivity of 5.6X1026 y to the neutrinoless double beta decay of 136Xe after 5 years of data, using 6 tons of natural xenon in the central detector region.

Ms. hebr. oct. 124 - [Sammelband in 2 Teilen: Handschriftenkonvolut]

Vorbesitzer: Eljāqīm Carmoly; Abraham Merzbacher

Ms. lat. qu. 124 - Neue Venezianische Adelsfamilien 1646 - 1669

Vorbesitzer: Johann Hieronymus Zum Jungen;

Ms. Barth. 124 - De consolatione philosophiae

Vorbesitzer: Inzelerius (Bischof von Budva und Weihbischof von Würzburg) ; Bartholomaeusstift Frankfurt am Main

Dark matter sensitivity of multi-ton liquid xenon detectors

We study the sensitivity of multi ton-scale time projection chambers using a liquid xenon target, e.g., the proposed DARWIN instrument, to spin-independent and spin-dependent WIMP-nucleon scattering interactions. Taking into account realistic backgrounds from the detector itself as well as from neutrinos, we examine the impact of exposure, energy threshold, background rejection efficiency and energy resolution on the dark matter sensitivity. With an exposure of 200 t x y and assuming detector parameters which have been already demonstrated experimentally, spin-independent cross sections as low as 2.5×10−49 cm2 can be probed for WIMP masses around 40 GeV/c2. Additional improvements in terms of background rejection and exposure will further increase the sensitivity, while the ultimate WIMP science reach will be limited by neutrinos scattering coherently off the xenon nuclei.

Cosmogenic activation of xenon and copper

Rare event search experiments using liquid xenon as target and detection medium require ultra-low background levels to fully exploit their physics potential. Cosmic ray induced activation of the detector components and, even more importantly, of the xenon itself during production, transportation and storage at the Earth's surface, might result in the production of radioactive isotopes with long half-lives, with a possible impact on the expected background. We present the first dedicated study on the cosmogenic activation of xenon after 345 days of exposure to cosmic rays at the Jungfraujoch research station at 3470m above sea level, complemented by a study of copper which has been activated simultaneously. We have directly observed the production of 7Be, 101Rh, 125Sb, 126I and 127Xe in xenon, out of which only 125Sb could potentially lead to background for a multi-ton scale dark matter search. The production rates for five out of eight studied radioactive isotopes in copper are in agreement with the only existing dedicated activation measurement, while we observe lower rates for the remaining ones. The specific saturation activities for both samples are also compared to predictions obtained with commonly used software packages, where we observe some underpredictions, especially for xenon activation.

Na 50 Nachlass Arthur Schopenhauer - 'Schopenhauer-Archiv', 124 - Hervorhebung der langen Freundschaft

u.a.: Beschreibung der schwierigen Lebenssituation in Paris; Reisen nach Belgien sowie Köln und Frankfurt;

Ms. Praed. 124 - Theologisch-philosophische Sammelhandschrift

Vorbesitzer: Dominikanerkloster Frankfurt am Main

Ms.Ff.F.Stoltze 3. 124 - Brief von Max Hirschfeld an Friedrich Stoltze

Verhandlungen wegen Lieferungen von Beiträgen zur Frankfurter Latern

Na 1 Nachlass Max Horkheimer, 364 - Korrespondenzen mit Alexander Mitscherlich (p. V 124, 1-102a)

1 Brief von Alexander Mitscherlich an Georg August Zinn (Ministerpräsident), 1961; 9 Briefe zwischen Prof. Tobias Brocher und Max Horkheimer; beteiligt: Alexander Mitscherlich, 1964-1968;