11,814 research outputs found

    Stop-list slicing.

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    Traditional program slicing requires two parameters: a program location and a variable, or perhaps a set of variables, of interest. Stop-list slicing adds a third parameter to the slicing criterion: those variables that are not of interest. This third parameter is called the stoplist. When a variable in the stop-list is encountered, the data-flow dependence analysis of slicing is terminated for that variable. Stop-list slicing further focuses on the computation of interest, while ignoring computations known or determined to be uninteresting. This has the potential to reduce slice size when compared to traditional forms of slicing. In order to assess the size of the reduction obtained via stop-list slicing, the paper reports the results of three empirical evaluations: a large scale empirical study into the maximum slice size reduction that can be achieved when all program variables are on the stop-list; a study on a real program, to determine the reductions that could be obtained in a typical application; and qualitative case-based studies to illustrate stop-list slicing in the small. The large-scale study concerned a suite of 42 programs of approximately 800KLoc in total. Over 600K slices were computed. Using the maximal stoplist reduced the size of the computed slices by about one third on average. The typical program showed a slice size reduction of about one-quarter. The casebased studies indicate that the comprehension effects are worth further consideration

    An empirical study of computation equivalence as determined by decomposition slice equivalence.

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    In order to further understand and assess decomposition slicing we characterize and evaluate the size of reductions obtained by computing equivalent decomposition slices from the perspective of the comprehender, maintainer, tester and researcher. The analysis was performed on 68 C language systems of sizes 100 to 50,000 lines. All decomposition slices were computed and compared for simple equality. From this data, we were able to determine with 95% confidence that the true mean percentage of equivalent decomposition slices is between 50.0% and 60.3%, with a p-value < 0.005. This has clear and significant impact for software testing, as any coverage method used for one of the variables used in an equivalence will apply to all variables in the class; for software comprehension as the number of items (variables) used for the understander is substantially reduced; for the software maintenance, as the number computational relationships is reduced; and for the researcher, in attempting to ascertain the underlying cause of this phenomena

    Determination of the Rb ng-series quantum defect by electric-field-induced resonant energy transfer between cold Rydberg atoms

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    Resonant energy transfer between cold Rydberg atoms was used to determine Rydberg atom energy levels, at precisions approaching those obtainable in microwave spectroscopy. Laser cooled Rb atoms from a magneto-optical trap were optically excited to 32d Rydberg states. The two-atom process 32d(j=5/2) + 32d(j=5/2) -> 34p(j=3/2) + 30g is resonant at an electric field of approximately 0.3 V/cm. This process is driven by the electric dipole-dipole interaction, which is allowed due to the partial f character that the g state acquires in an electric field. The experimentally observed resonant field, together with the Stark map calculation is used to make a determination of the Rb ng-series quantum defect: delta_g (n=30) = 0.00405(6)

    Spectroscopic observation of resonant electric dipole-dipole interactions between cold Rydberg atoms

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    Resonant electric dipole-dipole interactions between cold Rydberg atoms were observed using microwave spectroscopy. Laser-cooled Rb atoms in a magneto-optical trap were optically excited to 45d Rydberg states using a pulsed laser. A microwave pulse transferred a fraction of these Rydberg atoms to the 46p state. A second microwave pulse then drove atoms in the 45d state to the 46d state, and was used as a probe of interatomic interactions. The spectral width of this two-photon probe transition was found to depend on the presence of the 46p atoms, and is due to the resonant electric dipole-dipole interaction between 45d and 46p Rydberg atoms.Comment: 5 pages, 3 figures. Accepted for publication in Phys. Rev. Lett. Titles and e-print numbers of references added to this versio

    Seeking large-scale magnetic fields in a pure-disk dwarf galaxy NGC 2976

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    It is still unknown how magnetic field-generation mechanisms could operate in low-mass dwarf galaxies. Here, we present a detailed study of a nearby pure-disk dwarf galaxy NGC 2976. Unlike previously observed dwarf objects, this galaxy possesses a clearly defined disk. For the purpose of our studies, we performed deep multi-frequency polarimetric observations of NGC 2976 with the VLA and Effelsberg radio telescopes. Additionally, we supplement them with re-imaged data from the WSRT-SINGS survey. The magnetic field morphology discovered in NGC 2976 consists of a southern polarized ridge. This structure does not seem to be due to just a pure large-scale dynamo process (possibly cosmic-ray driven) at work in this object, as indicated by the RM data and dynamo number calculations. Instead, the field of NGC 2976 is modified by past gravitational interactions and possibly also by ram pressure inside the M 81 galaxy group environment. The estimates of total (7 muG) and ordered (3 muG) magnetic field strengths, as well as degree of field order (0.46), which is similar to those observed in spirals, suggest that tidally generated magnetized gas flows can further enhance dynamo action in the object. NGC 2976 is apparently a good candidate for the efficient magnetization of its neighbourhood. It is able to provide an ordered (perhaps also regular) magnetic field into the intergalactic space up to a distance of about 5 kpc. Tidal interactions (and possibly also ram pressure) can lead to the formation of unusual magnetic field morphologies (like polarized ridges) in galaxies out of the star-forming disks, which do not follow any observed component of the interstellar medium (ISM), as observed in NGC 2976. These galaxies are able to provide ordered magnetic fields far out of their main disks.Comment: 16 page

    Cosmic Pathways for Compact Groups in the Milli-Millennium Simulation

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    We detected 10 compact galaxy groups (CGs) at z=0z=0 in the semi-analytic galaxy catalog of Guo et al. (2011) for the milli-Millennium Cosmological Simulation (sCGs in mGuo2010a). We aimed to identify potential canonical pathways for compact group evolution and thus illuminate the history of observed nearby compact groups. By constructing merger trees for z=0z=0 sCG galaxies, we studied the cosmological evolution of key properties, and compared them with z=0z=0 Hickson CGs (HCGs). We found that, once sCG galaxies come within 1 (0.5) Mpc of their most massive galaxy, they remain within that distance until z=0z=0, suggesting sCG "birth redshifts". At z=0z=0 stellar masses of sCG most-massive galaxies are within 1010≲M∗/M⊙≲101110^{10} \lesssim M_{\ast}/M_{\odot} \lesssim 10^{11}. In several cases, especially in the two 4- and 5-member systems, the amount of cold gas mass anti-correlates with stellar mass, which in turn correlates with hot gas mass. We define the angular difference between group members' 3D velocity vectors, Δθvel\Delta\theta_{\rm vel}, and note that many of the groups are long-lived because their small values of Δθvel\Delta\theta_{\rm vel} indicate a significant parallel component. For triplets in particular, Δθvel\Delta\theta_{\rm vel} values range between 20∘20^{\circ} and 40∘40^{\circ} so that galaxies are coming together along roughly parallel paths, and pairwise separations do not show large pronounced changes after close encounters. The best agreement between sCG and HCG physical properties is for M∗M_{\ast} galaxy values, but HCG values are higher overall, including for SFRs. Unlike HCGs, due to a tail at low SFR and M∗M_{\ast}, and a lack of M∗≳1011M⊙M_{\ast}\gtrsim 10^{11}M_{\odot} galaxies, only a few sCG galaxies are on the star-forming main sequence.Comment: Style fixes to better match ApJ published version. Uses likeapj1.1 style files: 17 pages, 13 figures, 2 tables. LaTex style files available at https://github.com/qtast/likeapj/releases/lates

    Dear Wife : the Civil War letters of Chester K. Leach

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    Occasional paper (University of Vermont. Center for Research on Vermont) ; no. 20
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