Selection and reconstruction of the top quarks in the all-hadronic decays at a Linear Collider

A method of reconstruction of the top quarks produced in the process E+E- -> t\bar{t} -> 6 jets at a Linear Collider (LC) is proposed. The approach does not involve a kinematic fit, as well as assumptions on the invariant masses of the dijets originating from the decays of W bosons and, therefore, the method is expected to be less sensitive to theoretical and experimental uncertainties on the top-mass measurement than traditional reconstruction methods. For the first time, the reconstruction of the top quarks was investigated using the full LC detector simulation after taking into account the background arising from QCD multi-jet production.Comment: 22 pages, including 13 figures and 3 table

Les Houches Guidebook to Monte Carlo Generators for Hadron Collider Physics

Recently the collider physics community has seen significant advances in the formalisms and implementations of event generators. This review is a primer of the methods commonly used for the simulation of high energy physics events at particle colliders. We provide brief descriptions, references, and links to the specific computer codes which implement the methods. The aim is to provide an overview of the available tools, allowing the reader to ascertain which tool is best for a particular application, but also making clear the limitations of each tool.Comment: 49 pages Latex. Compiled by the Working Group on Quantum ChromoDynamics and the Standard Model for the Workshop ``Physics at TeV Colliders'', Les Houches, France, May 2003. To appear in the proceeding

Macro-language planning for multilingual education : focus on programmes and provision

This overview identifies some common features of macro-level language planning and briefly summarises the changing approaches to the analysis of macro-planning in the field. It previews six cases of language-in-education planning in response to linguistic diversity presented by the contributors to this issue. The cases show how macro-planning can either fail to recognise diverse ethnolinguistic identities or work to acknowledge them. Three common themes in language planning for multilingual education can be identified from the contributions: (i) top-down definitions of what counts as mother tongue can have both intended and unintended outcomes; (ii) language-as-problem responses to linguistic diversity can work to reinforce social exclusion; and (iii) the acknowledgement of diversity and minority language rights needs to flow through from statements of intent to on-the-ground implementation if they are to become a reality

Out and About in Medicine: GW Out For Health

The time is right to devise and implement a more coordinated approach to LGBT patient care and health professional training within the Washington, DC metropolitan area and beyond. The following George Washington University School of Medicine and Health Sciences (GWSMHS) and Hospital (GWUH) LGBT Health Initiative proposal highlights possible strategies for addressing this need through a more centralized fashion. The seven focus areas proposed for the GW LGBT Health Initiative include: 1) Climate/Visibility; 2) Health Education; 3) Policy/Advocacy; 4) Community Outreach; 5) Research; 6) Patient Care; and 7) HIV/AIDS. A key stakeholder that is helping to realize this vision of a comprehensive, coordinated GW LGBT Health Initiative is the student organization GW Out for Health (GWOFH). Led by an executive board of medical students and a faculty advisor, GWOFH has been working to improve the climate for LGBT and ally professional health students and visibility of LGBT health issues on campus through grass roots efforts. GWOFH has approached these goals by emulating aspects of successful student organizations, namely Student National Medical Association, as well as reaching out and building relationships with LGBT resources in the community. Altogether, members of the group will provide critical perspectives on the initial needs assessment and gap analysis of LGBT health at GWSMHS and GWUH necessary to developing a strategic plan for the GW LGBT Health Initiative. In the past year, GWOFH has achieved concrete steps towards improving the climate and visibility of LGBT health issues by building up their organizational infrastructure and membership, which is evidenced by the three-fold growth in membership and creation of a private campus Listserv. To provide social support for LGBT and ally medical students, GWOFH hosted a welcome potluck for GWSMHS students and a social mixer with the LGBT student organizations at Georgetown and Howard medical schools. To improve the visibility of LGBT health issues on campus, GWOFH launched a successful Lunchtime Lecture Series on current research and best practices for reducing LGBT health disparities. GWOFH’s accomplishments have set a solid foundation for providing professional and social support for incoming LGBT and ally professional health students. Furthermore, GWOFH’s reputable presence on campus will be leveraged to help support the proposed GW LGBT Health Initiative in the coming year by providing an advisory role on the development of an initial needs assessment and gap analysis, especially in the areas of climate and visibility, health education, political advocacy, and patient care

Dark matter allowed scenarios for Yukawa-unified SO(10) SUSY GUTs

Simple supersymmetric grand unified models based on the gauge group SO(10) require --in addition to gauge and matter unification-- the unification of t-b-\tau Yukawa couplings. Yukawa unification, however, only occurs for very special values of the soft SUSY breaking parameters. We perform a search using a Markov Chain Monte Carlo (MCMC) technique to investigate model parameters and sparticle mass spectra which occur in Yukawa-unified SUSY models, where we also require the relic density of neutralino dark matter to saturate the WMAP-measured abundance. We find the spectrum is characterizd by three mass scales: first/second generation scalars in the multi-TeV range, third generation scalars in the TeV range, and gauginos in the \sim 100 GeV range. Most solutions give far too high a relic abundance of neutralino dark matter. The dark matter discrepancy can be rectified by 1. allowing for neutralino decay to axino plus photon, 2. imposing gaugino mass non-universality or 3. imposing generational non-universality. In addition, the MCMC approach finds 4. a compromise solution where scalar masses are not too heavy, and where neutralino annihilation occurs via the light Higgs h resonance. By imposing weak scale Higgs soft term boundary conditions, we are also able to generate 5. low \mu, m_A solutions with neutralino annihilation via a light A resonance, though these solutions seem to be excluded by CDF/D0 measurements of the B_s\to \mu^+\mu^- branching fraction. Based on the dual requirements of Yukawa coupling unification and dark matter relic density, we predict new physics signals at the LHC from pair production of 350--450 GeV gluinos. The events are characterized by very high b-jet multiplicity and a dilepton mass edge around mz2-mz1 \sim 50-75 GeV.Comment: 35 pages with 21 eps figure

Analysis of Neptune's 2017 Bright Equatorial Storm

We report the discovery of a large ($\sim$8500 km diameter) infrared-bright storm at Neptune's equator in June 2017. We tracked the storm over a period of 7 months with high-cadence infrared snapshot imaging, carried out on 14 nights at the 10 meter Keck II telescope and 17 nights at the Shane 120 inch reflector at Lick Observatory. The cloud feature was larger and more persistent than any equatorial clouds seen before on Neptune, remaining intermittently active from at least 10 June to 31 December 2017. Our Keck and Lick observations were augmented by very high-cadence images from the amateur community, which permitted the determination of accurate drift rates for the cloud feature. Its zonal drift speed was variable from 10 June to at least 25 July, but remained a constant $237.4 \pm 0.2$ m s$^{-1}$ from 30 September until at least 15 November. The pressure of the cloud top was determined from radiative transfer calculations to be 0.3-0.6 bar; this value remained constant over the course of the observations. Multiple cloud break-up events, in which a bright cloud band wrapped around Neptune's equator, were observed over the course of our observations. No "dark spot" vortices were seen near the equator in HST imaging on 6 and 7 October. The size and pressure of the storm are consistent with moist convection or a planetary-scale wave as the energy source of convective upwelling, but more modeling is required to determine the driver of this equatorial disturbance as well as the triggers for and dynamics of the observed cloud break-up events.Comment: 42 pages, 14 figures, 6 tables; Accepted to Icaru