PLOT SPECIFICATIONS


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Star Formation Rate
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Model Name Parameters Plot Specify Introduction
Astrophysical Models
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        M(chirp mass) [1MΘ, 2.5MΘ]:
        λ(mass fraction) [0, 1MΘ-1]:
        η(mass ratio) [0, 0.25]
        χ(spin parameter) [-0.85, 0.85]
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        M(chirp mass) [1MΘ, 2.5MΘ]:
        λ(mass fraction) [0, 1MΘ-1]:
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          a(model detail 1)[5, 150]
          b(model detail 2)[40, 400]
          λ(mass fraction)[0, 1MΘ-1]
          E_v(energy carried away by neutrinos)
          <q>(luminosity weighted average neutrino anisotropy)
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            epsilon (efficiency)
            alpha (fraction of mass converted to black hole)
            a (spin factor)
            Minimum Progenitor Mass (in units of solar mass)
            Maximum Progenitor Mass (in units of solar mass)
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            B-Field[7e13G, 1e17G]:
            ε(ellipticity) [1e-6 - 1e-2]:
            P0(rot period) [1e-3s,5e-3s]:
            λ(mass fraction) [1e-4MΘ-1, 1e-2MΘ-1]:
            Iz(moment of inertia) [in g·cm2]:
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            a (spin factor)
            epsilon (efficiency)
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            M(chirp mass) [1MΘ, 2.5MΘ]:
            λ(mass fraction) [0, 1MΘ-1]:
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              d0m(Crust core differential shear) [1e-4,1e3]:
              N(NS Fraction) [1e-6,1]:
              v(kinematic viscosity) [0.1,10]:
              M_star(NS mass) [1MΘ,2MΘ]:
              R_star(NS radius) [7km,20km]:
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                D. Hils and P. L. Bender, Ap. J., 360, 75-94 (1990)
              P0(period) [0.5ms, 10ms]:
              λ(mass fraction) [0, 1e-2MΘ-1]:
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              P0(period) [0.5ms, 10ms]:
              λ(mass fraction) [0, 1e-2MΘ-1]:
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              Cosmological Models
              p(potential form) 1 or 2:
              ξcmb; (ξ at Φcmb)[1.2 2.7]:
              Ncmb(Number of e-foldings)[45 65]:
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              P(probability)[1e-3, 1]:
              ε(size)[1e-13, 1]:
              Gμ[1e-12,1e-6]:
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              r (Tensor-to-Scalar Ratio)
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              T(critical temperature) , GeV
              g(relativistic d.o.f)
              v(bubble wall velocity)[0,1]
              Beta/H(energy density parameter)[10, 1000]
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              Case # (1: non-runaway bubbles 2: runaway bubbles in a plasma 3: runaway bubbles in vacuum):
              α:
              β/H*:
              T*:
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              μ(0, 2]:
              F1[1e8, 1e11]:
              Fs[1, 1e11]:
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              r (Tensor-to-Scalar Ratio)
              w (Effective Equation of State Parameter)
              n (Effective Tensor Index)
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              Experimental Limits
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              Projected sensitivities
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                    Old Results
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                      Up to Date Results
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                        [Please note there may be up to 30 second wait for plots]