The Design Build Experience in the Context of A Self-Consolidating Grout Research Project

The purpose of this project was to experience the design-build project delivery method in the context of a research-fueled, procedural testing investigation. Thus, this project consisted of 3 main components each of which will be addressed in this report. The first aspect to be addressed is the research aspect. The goal of our research was to establish a chemical understanding of how replacement of cement with pozzolans in a grout mixture affects chemical processes and resulting structural characteristics within and of the grout. This research was then applied to formulation of potentially self-consolidating mix designs to be tested in the next aspect of the project. The next aspect of the project to be addressed is the application of the research to formulation of mix designs followed by the evaluation and analyses of said mix designs. This included ASTM procedurally guided testing of slump flow, j-ring slump flow, visual stability index identification, blocking assessment, compressive testing, and consolidation assessment. The goal of this testing was to establish a self consolidating grout mix design in accordance with ASTM C 476 which defines a self consolidating mix by its performance in terms of slump, visual stability, and compressive strength. The final aspect of the project to be addressed is the design build experience encountered while carrying out the procedural portion of the project. This will be discussed on the basis of criteria outlined by the Design Build Institute of American, namely 3 key terms assigned to successful design build project delivery, collaboration, integration, and communication. Each of these terms will be discussed in the context of our experience on this project

TRON 2.0 - The Experience

The goal of this senior project was to come up with a structural-engineering-related schematic design for a roller coaster to be installed in Disneyland called TRON 2.0: The Experience. This involved looking at both design processes that we had already learned through our curriculum as well as researching concepts that were previously foreign to us, namely the dynamic application of loads and the effects of fatigue stresses. A story was established based on the source material: the TRON movies produced by Walt Disney Studios. Thematic elements from the story were used as the basis for design implications that would become necessary as the process continued. These design implication influenced the design of the Ride System, Track Layout, and Ride Vehicle Design. These factors would end up influencing applicable loads, which would be utilized in the design of the Track Layout. The site was chosen to be constructed on Disneyland proper so that realistic site parameters and dimensions would give a sense of scale to the project and eliminate ambiguity. However, existing elements on the site would cause challenges for us to work around. Once the site was chosen, Queue and Show buildings were designated simple designs to tie back to story-driven implications and reinforce the standards set by the Walt Disney Imagineering process model. In addition, we gained more information such as crowd capacity to dictate further mechanical design and dynamic applications. The mechanical side of the process saw the development of a ride system used to propel the Ride Vehicles, all designed by the Mechanical Engineers on the project. The Ride Vehicle weights became relevant for the design of the track. A Track Layout was created and inputted into simulation software so that dynamic accelerations could be developed as new loading conditions for Track Design. Finally, all of the preceding elements of design were culminated into a schematic design of a roller coaster track making sure to account for subjects such as dynamic applications, torsion, and fatigue. All designs were replicated in modeling software to confirm constructability and viability of the resulting schematic design

Form factors from free fermionic Fock fields, the Federbush model

By representing the field content as well as the particle creation operators in terms of fermionic Fock operators, we compute the corresponding matrix elements of the Federbush model. Only when these matrix elements satisfy the form factor consistency equations involving anyonic factors of local commutativity, the corresponding operators are local. We carry out the ultraviolet limit, analyze the momentum space cluster properties and demonstrate how the Federbush model can be obtained from the $SU(3)_3$-homogeneous sine-Gordon model. We propose a new Lagrangian which on one hand constitutes a generalization of the Federbush model in a Lie algebraic fashion and on the other a certain limit of the homogeneous sine-Gordon models.Comment: 30 pages Latex, one section adde

Multi-year characterisation of the broad-band emission from the intermittent extreme BL Lac 1ES~2344+514

The BL Lac 1ES 2344+514 is known for temporary extreme properties (e.g., a shift of the synchrotron SED peak energy $\nu_{synch,p}$ above 1keV). While those extreme states were so far observed only during high flux levels, additional multi-year observing campaigns are required to achieve a coherent picture. Here, we report the longest investigation of the source from radio to VHE performed so far, focusing on a systematic characterisation of the intermittent extreme states. While our results confirm that 1ES 2344+514 typically exhibits $\nu_{synch,p}>$1keV during elevated flux periods, we also find periods where the extreme state coincides with low flux activity. A strong spectral variability thus happens in the quiescent state, and is likely caused by an increase of the electron acceleration efficiency without a change in the electron injection luminosity. We also report a strong X-ray flare (among the brightest for 1ES 2344+514) without a significant shift of $\nu_{synch,p}$. During this particular flare, the X-ray spectrum is among the softest of the campaign. It unveils complexity in the spectral evolution, where the common harder-when-brighter trend observed in BL Lacs is violated. During a low and hard X-ray state, we find an excess of the UV flux with respect to an extrapolation of the X-ray spectrum to lower energies. This UV excess implies that at least two regions contribute significantly to the infrared/optical/ultraviolet/X-ray emission. Using the simultaneous MAGIC, XMM-Newton, NuSTAR, and AstroSat observations, we argue that a region possibly associated with the 10 GHz radio core may explain such an excess. Finally, we investigate a VHE flare, showing an absence of simultaneous variability in the 0.3-2keV band. Using a time-dependent leptonic modelling, we show that this behaviour, in contradiction to single-zone scenarios, can instead be explained by a two-component model.Comment: Accepted for publication in Astronomy & Astrophysic

The Great Markarian 421 Flare of 2010 February: Multiwavelength Variability and Correlation Studies

We report on variability and correlation studies using multiwavelength observations of the blazar Mrk 421 during the month of 2010 February, when an extraordinary flare reaching a level of ∼27 Crab Units above 1 TeV was measured in very high energy (VHE) γ-rays with the Very Energetic Radiation Imaging Telescope Array System (VERITAS) observatory. This is the highest flux state for Mrk 421 ever observed in VHE γ-rays. Data are analyzed from a coordinated campaign across multiple instruments, including VHE γ-ray (VERITAS, Major Atmospheric Gamma-ray Imaging Cherenkov), high-energy γ-ray (Fermi-LAT), X-ray (Swift, Rossi X-ray Timing Experiment, MAXI), optical (including the GASP-WEBT collaboration and polarization data), and radio (Metsahovi, Owens Valley Radio Observatory, University of Michigan Radio Astronomy Observatory). Light curves are produced spanning multiple days before and after the peak of the VHE flare, including over several flare "decline" epochs. The main flare statistics allow 2 minute time bins to be constructed in both the VHE and optical bands enabling a cross-correlation analysis that shows evidence for an optical lag of ∼25-55 minutes, the first time-lagged correlation between these bands reported on such short timescales. Limits on the Doppler factor (δ ⪆ 33) and the size of the emission region (δ-1RB≲ 3.8 × 1013cm) are obtained from the fast variability observed by VERITAS during the main flare. Analysis of 10 minute binned VHE and X-ray data over the decline epochs shows an extraordinary range of behavior in the flux-flux relationship, from linear to quadratic to lack of correlation to anticorrelation. Taken together, these detailed observations of an unprecedented flare seen in Mrk 421 are difficult to explain with the classic single-zone synchrotron self-Compton model

Unraveling the Complex Behavior of Mrk 421 with Simultaneous X-Ray and VHE Observations during an Extreme Flaring Activity in 2013 April*

We report on a multiband variability and correlation study of the TeV blazar Mrk 421 during an exceptional flaring activity observed from 2013 April 11 to 19. The study uses, among others, data from GLAST-AGILE Support Program (GASP) of the Whole Earth Blazar Telescope (WEBT), Swift, Nuclear Spectroscopic Telescope Array (NuSTAR), Fermi Large Area Telescope, Very Energetic Radiation Imaging Telescope Array System (VERITAS), and Major Atmospheric Gamma Imaging Cherenkov (MAGIC). The large blazar activity and the 43 hr of simultaneous NuSTAR and MAGIC/VERITAS observations permitted variability studies on 15 minute time bins over three X-ray bands (3-7 keV, 7-30 keV, and 30-80 keV) and three very-high-energy (VHE; >0.1 TeV) gamma-ray bands (0.2-0.4 TeV, 0.4-0.8 TeV, and >0.8 TeV). We detected substantial flux variations on multi-hour and sub-hour timescales in all of the X-ray and VHE gamma-ray bands. The characteristics of the sub-hour flux variations are essentially energy independent, while the multi-hour flux variations can have a strong dependence on the energy of the X-rays and the VHE gamma-rays. The three VHE bands and the three X-ray bands are positively correlated with no time lag, but the strength and characteristics of the correlation change substantially over time and across energy bands. Our findings favor multi-zone scenarios for explaining the achromatic/chromatic variability of the fast/slow components of the light curves, as well as the changes in the flux-flux correlation on day-long timescales. We interpret these results within a magnetic reconnection scenario, where the multi-hour flux variations are dominated by the combined emission from various plasmoids of different sizes and velocities, while the sub-hour flux variations are dominated by the emission from a single small plasmoid moving across the magnetic reconnection layer

The Great Markarian 421 Flare of 2010 February: Multiwavelength Variability and Correlation Studies

We report on variability and correlation studies using multiwavelength observations of the blazar Mrk 421 during the month of 2010 February, when an extraordinary flare reaching a level of ∼27 Crab Units above 1 TeV was measured in very high energy (VHE) γ-rays with the Very Energetic Radiation Imaging Telescope Array System (VERITAS) observatory. This is the highest flux state for Mrk 421 ever observed in VHE γ-rays. Data are analyzed from a coordinated campaign across multiple instruments, including VHE γ-ray (VERITAS, Major Atmospheric Gamma-ray Imaging Cherenkov), high-energy γ-ray (Fermi-LAT), X-ray (Swift, Rossi X-ray Timing Experiment, MAXI), optical (including the GASP-WEBT collaboration and polarization data), and radio (Metsahovi, Owens Valley Radio Observatory, University of Michigan Radio Astronomy Observatory). Light curves are produced spanning multiple days before and after the peak of the VHE flare, including over several flare "decline" epochs. The main flare statistics allow 2 minute time bins to be constructed in both the VHE and optical bands enabling a cross-correlation analysis that shows evidence for an optical lag of ∼25-55 minutes, the first time-lagged correlation between these bands reported on such short timescales. Limits on the Doppler factor (δ ⪆ 33) and the size of the emission region (δ-1RB≲ 3.8 × 1013cm) are obtained from the fast variability observed by VERITAS during the main flare. Analysis of 10 minute binned VHE and X-ray data over the decline epochs shows an extraordinary range of behavior in the flux-flux relationship, from linear to quadratic to lack of correlation to anticorrelation. Taken together, these detailed observations of an unprecedented flare seen in Mrk 421 are difficult to explain with the classic single-zone synchrotron self-Compton model.</p

In Vivo Profiling of Estrogen Receptor/Specificity Protein-Dependent Transactivation

17β-Estradiol (E2) activates the estrogen receptor (ER) through multiple genomic and nongenomic pathways in various tissues/organs. ERα/specificity protein-dependent activation of E2-responsive genes containing GC-rich promoters has been identified in breast and other cancer cell lines, and in this study, we describe transgenic animals overexpressing a transgene containing three tandem GC-rich sites linked to a minimal TATA or thymidine kinase promoter and a luciferase gene. Several mouse lines expressing the transgenes were characterized and, in line 15, E2 induced a 9-fold increase in luciferase activity in the female mouse uterus, and the synthetic estrogens bisphenol A and nonylphenol also induced uterine luciferase activity. The pure antiestrogen ICI 182,780 induced luciferase activity in the mouse uterus, and similar results were observed for ICI 182,780 in breast cancer cells transfected with this construct. Differences in the ER agonist and antagonist activities of E2, nonylphenol, bisphenol A, and ICI 182,780 were investigated in the male testis and penis and the male and female stomach in line 15 transgenic mice. All of these tissues were hormone responsive; however, the patterns of induced or repressed luciferase activity were ligand structure, tissue, and sex dependent. These results demonstrate for the first time hormonal activation or repression of a GC-rich promoter in vivo, and the results suggest that the ERα/specificity protein pathway may contribute to E2-dependent induction and repression of genes