378 research outputs found

    Linear approach to the orbiting spacecraft thermal problem

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    We develop a linear method for solving the nonlinear differential equations of a lumped-parameter thermal model of a spacecraft moving in a closed orbit. Our method, based on perturbation theory, is compared with heuristic linearizations of the same equations. The essential feature of the linear approach is that it provides a decomposition in thermal modes, like the decomposition of mechanical vibrations in normal modes. The stationary periodic solution of the linear equations can be alternately expressed as an explicit integral or as a Fourier series. We apply our method to a minimal thermal model of a satellite with ten isothermal parts (nodes) and we compare the method with direct numerical integration of the nonlinear equations. We briefly study the computational complexity of our method for general thermal models of orbiting spacecraft and conclude that it is certainly useful for reduced models and conceptual design but it can also be more efficient than the direct integration of the equations for large models. The results of the Fourier series computations for the ten-node satellite model show that the periodic solution at the second perturbative order is sufficiently accurate.Comment: 20 pages, 11 figures, accepted in Journal of Thermophysics and Heat Transfe

    Deconfinement transition and string tensions in SU(4) Yang-Mills Theory

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    We present results from numerical lattice calculations of SU(4) Yang-Mills theory. This work has two goals: to determine the order of the finite temperature deconfinement transition on an Nt=6N_t = 6 lattice and to study the string tensions between static charges in the irreducible representations of SU(4). Motivated by Pisarski and Tytgat's argument that a second-order SU(\infty) deconfinement transition would explain some features of the SU(3) and QCD transitions, we confirm older results on a coarser, Nt=4N_t = 4, lattice. We see a clear two-phase coexistence signal, characteristic of a first-order transition, at 8/g2=10.798/g^2 = 10.79 on a 6×2036\times 20^3 lattice, on which we also compute a latent heat of Δϵ0.6ϵSB\Delta\epsilon\approx 0.6 \epsilon_{SB}. Computing Polyakov loop correlation functions we calculate the string tension at finite temperature in the confined phase between fundamental charges, σ1\sigma_1, between diquark charges, σ2\sigma_2, and between adjoint charges σ4\sigma_4. We find that 1<σ2/σ1<21 < \sigma_2/\sigma_1 < 2, and our result for the adjoint string tension σ4\sigma_4 is consistent with string breaking.Comment: 10 pages with included figures. For version 2: New calculation and discussion of latent heat added; 2 new figures and 1 new table. Typo in abstract corrected for v3. To appear in Physical Review

    Masculinity as Governance: police, public service and the embodiment of authority, c. 1700-1850

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    About the book: Public Men offers an introduction to an exciting new field: the history of masculinities in the political domain and will be essential reading for students and specialists alike with interests in gender or political culture. By building upon new work on gender and political culture, these new case studies explore the gendering of the political domain and the masculinities of the men who have historically dominated it. As such, Public Men is a major contribution to our understanding of the history of Britain between the Eighteenth and the Twentieth centuries

    Nonlinear analysis of spacecraft thermal models

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    We study the differential equations of lumped-parameter models of spacecraft thermal control. Firstly, we consider a satellite model consisting of two isothermal parts (nodes): an outer part that absorbs heat from the environment as radiation of various types and radiates heat as a black-body, and an inner part that just dissipates heat at a constant rate. The resulting system of two nonlinear ordinary differential equations for the satellite's temperatures is analyzed with various methods, which prove that the temperatures approach a steady state if the heat input is constant, whereas they approach a limit cycle if it varies periodically. Secondly, we generalize those methods to study a many-node thermal model of a spacecraft: this model also has a stable steady state under constant heat inputs that becomes a limit cycle if the inputs vary periodically. Finally, we propose new numerical analyses of spacecraft thermal models based on our results, to complement the analyses normally carried out with commercial software packages.Comment: 29 pages, 4 figure

    The equation of state for two flavor QCD at N_t=6

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    We calculate the two flavor equation of state for QCD on lattices with lattice spacing a=(6T)^{-1} and find that cutoff effects are substantially reduced compared to an earlier study using a=(4T)^{-1}. However, it is likely that significant cutoff effects remain. We fit the lattice data to expected forms of the free energy density for a second order phase transition at zero-quark-mass, which allows us to extrapolate the equation of state to m_q=0 and to extract the speed of sound. We find that the equation of state depends weakly on the quark mass for small quark mass.Comment: 24 pages, latex, 11 postscipt figure

    The BKB_K Kaon Parameter in the Chiral Limit

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    We introduce four-point functions in the hadronic ladder resummation approach to large NcN_c QCD Green functions. We determine the relevant one to calculate the BKB_K kaon parameter in the chiral limit. This four-point function contains both the large momenta QCD OPE and the small momenta ChPT at NLO limits, analytically. We get B^Kχ=0.38±0.15\hat B_K^\chi = 0.38 \pm 0.15. We also give the ChPT result at NLO for the relevant four-point function to calculate BKB_K outside the chiral limit, while the leading QCD OPE is the same as the chiral limit one.Comment: 17 page

    Quenched Lattice QCD with Domain Wall Fermions and the Chiral Limit

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    Quenched QCD simulations on three volumes, 83×8^3 \times, 123×12^3 \times and 163×3216^3 \times 32 and three couplings, β=5.7\beta=5.7, 5.85 and 6.0 using domain wall fermions provide a consistent picture of quenched QCD. We demonstrate that the small induced effects of chiral symmetry breaking inherent in this formulation can be described by a residual mass (\mres) whose size decreases as the separation between the domain walls (LsL_s) is increased. However, at stronger couplings much larger values of LsL_s are required to achieve a given physical value of \mres. For β=6.0\beta=6.0 and Ls=16L_s=16, we find \mres/m_s=0.033(3), while for β=5.7\beta=5.7, and Ls=48L_s=48, \mres/m_s=0.074(5), where msm_s is the strange quark mass. These values are significantly smaller than those obtained from a more naive determination in our earlier studies. Important effects of topological near zero modes which should afflict an accurate quenched calculation are easily visible in both the chiral condensate and the pion propagator. These effects can be controlled by working at an appropriately large volume. A non-linear behavior of mπ2m_\pi^2 in the limit of small quark mass suggests the presence of additional infrared subtlety in the quenched approximation. Good scaling is seen both in masses and in fπf_\pi over our entire range, with inverse lattice spacing varying between 1 and 2 GeV.Comment: 91 pages, 34 figure

    A Lattice Study of the Nucleon Excited States with Domain Wall Fermions

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    We present results of our numerical calculation of the mass spectrum for isospin one-half and spin one-half non-strange baryons, i.e. the ground and excited states of the nucleon, in quenched lattice QCD. We use a new lattice discretization scheme for fermions, domain wall fermions, which possess almost exact chiral symmetry at non-zero lattice spacing. We make a systematic investigation of the negative-parity NN^* spectrum by using two distinct interpolating operators at β=6/g2=6.0\beta=6/g^2=6.0 on a 163×32×1616^3 \times 32 \times 16 lattice. The mass estimates extracted from the two operators are consistent with each other. The observed large mass splitting between this state, N(1535)N^*(1535), and the positive-parity ground state, the nucleon N(939), is well reproduced by our calculations. We have also calculated the mass of the first positive-parity excited state and found that it is heavier than the negative-parity excited state for the quark masses studied.Comment: 46 pages, REVTeX, 11 figures included, revised version accepted for publication in Phys. Rev.
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