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Canuto, V.M., A.M. Howard, C.J. Muller, and S.R. Jaynes, 2006: GISS Mixing Model with tides: Enhanced bottom mixing and new bottom boundary layer. J. Phys. Oceanog., submitted.
Canuto, V.M., 2008: Turbulence in astrophysical and geophysical flows. In Interdisciplinary Aspects of Turbulence. W. Hillebrandt and F. Kukpa, Eds., Lecture Notes in Physics, vol. 756. Springer, in press.
Canuto, V.M., Y. Cheng, and A.M. Howard, 2008: A new model for Double Diffusion + Turbulence using a Reynolds stress model. Geophys. Res. Lett., 35, L02613, doi:10.1029/2007GL032580.
Canuto, V.M., Y. Cheng, A.M. Howard, and E.N. Essau, 2008: Stably stratified flows: A model with no Ri(cr). J. Atmos. Sci., 65, 2437-2447, doi:10.1175/2007JAS2470.1.
Ferrari, R., J.C. McWilliams, V.M. Canuto, and M. Dubovikov, 2008: Parameterization of eddy fluxes near oceanic boundaries. J. Climate, 31, 2770-2789, doi:10.1175/2007JCLI1510.1.
Canuto, V.M., Y. Cheng, and A.M. Howard, 2007: Non-local ocean mixing model and a new plume model for deep convection. Ocean Model., 16, 28-46, doi:10.1016/j.ocemod.2006.07.003.
Canuto, V.M., and M.S. Dubovikov, 2007: The effect of mesoscales on the tracer equation in z-coordinates OGCMs. Ocean Model., 16, 17-27, doi:10.1016/j.ocemod.2006.06.002.
Canuto, V.M., and M.S. Dubovikov, 2007: Reply to the comment by McDougall et al. Ocean Model., 17, 172-181, doi:10.1016/j.ocemod.2006.11.005.
Hansen, J., Mki. Sato, R. Ruedy, P. Kharecha, A. Lacis, R.L. Miller, L. Nazarenko, K. Lo, G.A. Schmidt, G. Russell, I. Aleinov, S. Bauer, E. Baum, B. Cairns, V. Canuto, M. Chandler, Y. Cheng, A. Cohen, A. Del Genio, G. Faluvegi, E. Fleming, A. Friend, T. Hall, C. Jackman, J. Jonas, M. Kelley, N.Y. Kiang, D. Koch, G. Labow, J. Lerner, S. Menon, T. Novakov, V. Oinas, Ja. Perlwitz, Ju. Perlwitz, D. Rind, A. Romanou, R. Schmunk, D. Shindell, P. Stone, S. Sun, D. Streets, N. Tausnev, D. Thresher, N. Unger, M. Yao, and S. Zhang, 2007: Dangerous human-made interference with climate: A GISS modelE study. Atmos. Chem. Phys., 7, 2287-2312.
Hansen, J., Mki. Sato, R. Ruedy, P. Kharecha, A. Lacis, R.L. Miller, L. Nazarenko, K. Lo, G.A. Schmidt, G. Russell, I. Aleinov, S. Bauer, E. Baum, B. Cairns, V. Canuto, M. Chandler, Y. Cheng, A. Cohen, A. Del Genio, G. Faluvegi, E. Fleming, A. Friend, T. Hall, C. Jackman, J. Jonas, M. Kelley, N.Y. Kiang, D. Koch, G. Labow, J. Lerner, S. Menon, T. Novakov, V. Oinas, Ja. Perlwitz, Ju. Perlwitz, D. Rind, A. Romanou, R. Schmunk, D. Shindell, P. Stone, S. Sun, D. Streets, N. Tausnev, D. Thresher, N. Unger, M. Yao, and S. Zhang, 2007: Climate simulations for 1880-2003 with GISS modelE. Clim. Dynam., 29, 661-696, doi:10.1007/s00382-007-0255-8.
Canuto, V.M., and M.S. Dubovikov, 2006: Dynamical model of mesoscales in z-coordinates. Ocean Model., 11, 123-166, doi:10.1016/j.ocemod.2004.12.002.
Dubovikov, M.S., and V.M. Canuto, 2006: Complete Eulerian-mean tracer equation for coarse resolution OGCMs. Geophys. Astrophys. Fluid Dyn., 100, 197-214, doi:10.1080/03091920600799830.
Schmidt, G.A., R. Ruedy, J.E. Hansen, I. Aleinov, N. Bell, M. Bauer, S. Bauer, B. Cairns, V. Canuto, Y. Cheng, A. Del Genio, G. Faluvegi, A.D. Friend, T.M. Hall, Y. Hu, M. Kelley, N.Y. Kiang, D. Koch, A.A. Lacis, J. Lerner, K.K. Lo, R.L. Miller, L. Nazarenko, V. Oinas, Ja. Perlwitz, Ju. Perlwitz, D. Rind, A. Romanou, G.L. Russell, Mki. Sato, D.T. Shindell, P.H. Stone, S. Sun, N. Tausnev, D. Thresher, and M.-S. Yao, 2006: Present day atmospheric simulations using GISS ModelE: Comparison to in-situ, satellite and reanalysis data. J. Climate, 19, 153-192, doi:10.1175/JCLI3612.1.
Canuto, V.M., Y. Cheng, and A.M. Howard, 2005: What causes the divergences in local second-order closure models? J. Atmos. Sci., 62, 1645-1651, doi:10.1175/JAS3420.1.
Canuto, V.M., and M.S. Dubovikov, 2005: Modeling mesoscale eddies. Ocean Model., 8, 1-30, doi:10.1016/j.ocemod.2003.11.003.
Canuto, V.M., M.S. Dubovikov, and Y. Cheng, 2005: Entrainment: Local and non-local turbulence models with double diffusion. Geophys. Res. Lett., 32, L22604, doi:10.1029/2005GL023771.
Cheng, Y., V.M. Canuto, and A.M. Howard, 2005: Nonlocal convective PBL model based on new third- and fourth-order moments. J. Atmos. Sci., 62, 2189-2204, doi:10.1175/JAS3474.1.
Dubovikov, M.S., and V.M. Canuto, 2005: Dynamic model of mesoscale eddies. Eddy parameterization for coarse resolution ocean circulation models. Geophys. Astrophys. Fluid Dyn., 99, 19-47, doi:10.1080/03091920412331336406.
Hansen, J., Mki. Sato, R. Ruedy, L. Nazarenko, A. Lacis, G.A. Schmidt, G. Russell, I. Aleinov, M. Bauer, S. Bauer, N. Bell, B. Cairns, V. Canuto, M. Chandler, Y. Cheng, A. Del Genio, G. Faluvegi, E. Fleming, A. Friend, T. Hall, C. Jackman, M. Kelley, N.Y. Kiang, D. Koch, J. Lean, J. Lerner, K. Lo, S. Menon, R.L. Miller, P. Minnis, T. Novakov, V. Oinas, Ja. Perlwitz, Ju. Perlwitz, D. Rind, A. Romanou, D. Shindell, P. Stone, S. Sun, N. Tausnev, D. Thresher, B. Wielicki, T. Wong, M. Yao, and S. Zhang, 2005: Efficacy of climate forcings. J. Geophys. Res., 110, D18104, doi:10.1029/2005JD005776.
Canuto, V.M., A. Howard, Y. Cheng, and R.L. Miller, 2004: Latitude-dependent vertical mixing and the tropical thermocline in a global OGCM. Geophys. Res. Lett., 31, L16305, doi:10.1029/2004GL019891.
Canuto, V.M., A. Howard, P. Hogan, Y. Cheng, M.S. Dubovikov, and L.M. Montenegro, 2004: Modeling ocean deep convection. Ocean Model., 7, 75-95, doi:10.1016/S1463-5003(03)00038-6.
Cheng, Y., V.M. Canuto, and A.M. Howard, 2004: Reply to Comments on "An improved model for the turbulent PBL" by Hassid and Galperin. J. Atmos. Sci., 61, 1200-1204, doi:10.1175/1520-0469(2004)061<1200:R>2.0.CO;2.
Cheng, Y., V.M. Canuto, and A.M. Howard, 2003: Comments on "An improved model for the turbulent PBL". J. Atmos. Sci., 60, 3043-3046, doi:10.1175/1520-0469(2003)060<3043:COOAIM>2.0.CO;2.
Canuto, V.M., 2002: Diffusion in stars: The case of gravity waves, rigid rotation and stable stratification. M. Not. Royal Astron. Soc., 337, 713-719, doi:10.1046/j.1365-8711.2002.05962.x.
Canuto, V.M., 2002: Critical Richardson numbers and gravity waves. Astron. Astrophys., 384, 1119-1123, doi:10.1051/0004-6361:20011773.
Canuto, V.M., A. Howard, Y. Cheng, and M.S. Dubovikov, 2002: Ocean turbulence. Part II: Vertical diffusivities of momentum, heat, salt, mass, and passive scalars. J. Phys. Oceanog., 32, 240-264, doi:10.1175/1520-0485(2002)032<0240:OTPIVD>2.0.CO;2.
Cheng, Y., V.M. Canuto, and A.M. Howard, 2002: An improved model for the turbulent PBL. J. Atmos. Sci., 59, 1550-1565, doi:10.1175/1520-0469(2002)059<1550:AIMFTT>2.0.CO;2.
Canuto, V.M., Y. Cheng, and A. Howard, 2001: New third-order moments for the convective boundary layer. J. Atmos. Sci., 58, 1169-1172, doi:10.1175/1520-0469(2001)058<1169:NTOMFT>2.0.CO;2.
Canuto, V.M., A. Howard, Y. Cheng, and M.S. Dubovikov, 2001: Ocean turbulence. Part I: One-point closure model-momentum and heat vertical diffusivities. J. Phys. Oceanog., 31, 1413-1426, doi:10.1175/1520-0485(2001)031<1413:OTPIOP>2.0.CO;2.
Canuto, V.M., and F. Minotti, 2001: Mixing and transport in stars. I. Formalism: Momentum, heat and mean molecular weight. M. Not. Royal Astron. Soc., 328, 829-838, doi:10.1046/j.1365-8711.2001.04911.x.
Canuto, V.M., 2000: Semiconvection and overshooting: Schwarzschild and Ledoux criteria revisited. Astrophys. J., 534, L113-L115, doi:10.1086/312654.
Canuto, V.M., 2000: The physics of subgrid scales in numerical simulations of stellar convection: Are they dissipative, advective, or diffusive? Astrophys. J., 541, L79-L82, doi:10.1086/312895.
Canuto, V.M., 2000: Turbulence and laminar structures: Can they co-exist. M. Not. Royal Astron. Soc., 317, 985-988, doi:10.1046/j.1365-8711.2000.03786.x.
Canuto, V.M., 2000: Turbulent convection: Is 2D a good proxy of 3D? Astron. Astrophys., 357, 177-179.
Canuto, V.M., 1999: Overshooting in massive stars: Conceptual problems and suggested solution. Astrophys. J., 518, L119-L122, doi:10.1086/312082.
Canuto, V.M., 1999: Turbulence in stars. III. Unified treatment of diffusion, convection, semiconvection, salt fingers, and differential rotation. Astrophys. J., 524, 311-340, doi:10.1086/307783.
Canuto, V.M., and M.S. Dubovikov, 1999: A dynamical model for turbulence. VII. Complete system of five orthogonal tensors for shear-driven flows. Phys. Fluids, 11, 659-664, doi:10.1063/1.869937.
Canuto, V.M., M.S. Dubovikov, and G. Yu, 1999: A dynamical model for turbulence. IX. Reynolds stresses for shear-driven flows. Phys. Fluids, 11, 678-691, doi:10.1063/1.869939.
Canuto, V.M., M.S. Dubovikov, and G. Yu, 1999: A dynamical model for turbulence. VIII. IR and UV Reynolds stress spectra for shear-driven flows. Phys. Fluids, 11, 665-677, doi:10.1063/1.869938.
Canuto, V.M., 1998: Turbulence in stars. II. Shear, stable stratification, and radiative losses. Astrophys. J., 508, 767-779, doi:10.1086/306427.
Canuto, V.M., 1998: Missing mixing? Astrophys. J., 505, L47-L50, doi:10.1086/311596.
Canuto, V.M., 1998: Solar tachocline revisited. Astrophys. J., 497, L51-L54, doi:10.1086/311275.
Canuto, V.M., 1998: Overshooting and the µ-barrier. Astrophys. J., 508, L103-L104, doi:10.1086/311722.
Canuto, V.M., and J. Christensen-Dalgaard, 1998: Turbulence in astrophysics: Stars. Annual Rev. Fluid Mech., 30, 167-198, doi:10.1146/annurev.fluid.30.1.167.
Canuto, V.M., and M. Dubovikov, 1998: Stellar turbulent convection. I. Theory. Astrophys. J., 493, 834-847, doi:10.1086/305141.
Canuto, V.M., and M.S. Dubovikov, 1998: Two scaling regimes for rotating Rayleigh-Bénard convection. Phys. Rev. Lett., 80, 281-284, doi:10.1103/PhysRevLett.80.281.
Canuto, V.M., 1997: Overshooting in stars: Five old fallacies and a new model. Astrophys. J., 489, L71-L74, doi:10.1086/310955.
Canuto, V.M., 1997: Sub-grid scale modeling: Correct models and others. Astrophys. J., 478, 322-325, doi:10.1086/303772.
Canuto, V.M., 1997: Compressible turbulence. Astrophys. J., 482, 827-851, doi:10.1086/304175.
Canuto, V.M., and Y. Cheng, 1997: Determination of the Smagorinski-Lilly constant CS. Phys. Fluids, 9, 1368-1378, doi:10.1063/1.869251.
Canuto, V.M., and M. Dubovikov, 1997: Overshooting: Mixing length yields divergent results. Astrophys. J., 484, L161-L163, doi:10.1086/310792.
Canuto, V.M., and M.S. Dubovikov, 1997: A new approach to turbulence. Int. J. Mod. Phys. A, 12, 3121-3152, doi:10.1142/S0217751X9700164X.
Canuto, V.M., and M.S. Dubovikov, 1997: A dynamical model for turbulence. V. The effect of rotation. Phy. Fluids, 9, 2132-2140, doi:10.1063/1.869332.
Canuto, V.M., and M.S. Dubovikov, 1997: Physical regimes and dimensional structure of rotating turbulence. Phys. Rev. Lett., 78, 666-669, doi:10.1103/PhysRevLett.78.666.
Canuto, V.M., M.S. Dubovikov, and A. Dienstfrey, 1997: Turbulent convection in a spectral model. Phys. Rev. Lett., 78, 662-665, doi:10.1103/PhysRevLett.78.662.
Canuto, V.M., M.S. Dubovikov, and A. Dienstfrey, 1997: A dynamical model for turbulence. IV. Buoyancy-driven flows. Phys. Fluids, 9, 2118-2131, doi:10.1063/1.869331.
Canuto, V.M., M.S. Dubovikov, and D.J. Wielaard, 1997: A dynamical model for turbulence. VI. Two-dimensional turbulence. Phys. Fluids, 9, 2141-2147, doi:10.1063/1.869333.
Ying, R., and V.M. Canuto, 1997: Numerical simulation of flow over two-dimensional hills using a second-order turbulence closure model. Bound.-Lay. Meteorol., 85, 447-474, doi:10.1023/A:1000534921008.
Canuto, V., M.S. Dubovikov, Y. Cheng, and A. Dienstfrey, 1996: Dynamical model for turbulence. III. Numerical results. Phys. Fluids, 8, 599-613, doi:10.1063/1.868844.
Canuto, V.M., 1996: Turbulent convection: Old and new models. Astrophys. J., 467, 385-396, doi:10.1086/177613.
Canuto, V.M., and M.S. Dubovikov, 1996: A dynamical model for turbulence. I. General formalism. Phys. Fluids, 8, 571-585, doi:10.1063/1.868842.
Canuto, V.M., and M.S. Dubovikov, 1996: A dynamical model for turbulence. II. Shear-driven flows. Phys. Fluids, 8, 587-598, doi:10.1063/1.868843.
Canuto, V.M., I. Goldman, and I. Mazzitelli, 1996: Stellar turbulent convection: A self-consistent model. Astrophys. J., 473, 550-559, doi:10.1086/178166.
Ying, R., and V.M. Canuto, 1996: Turbulence modelling over two-dimensional hills using an algebraic Reynolds stress expression. Bound.-Lay. Meteorol., 77, 69-99, doi:10.1007/BF00121859.
Canuto, V.M., 1994: Large eddy simulation of turbulence: A subgrid scale model including shear, vorticity, rotation, and buoyancy. Astrophys. J., 428, 729-752, doi:10.1086/174281.
Canuto, V.M., F. Minotti, C. Ronchi, and R.M. Ypma, 1994: Second-order closure PBL model with new third-order moments: Comparison with LES data. J. Atmos. Sci., 51, 1605-1618, doi:10.1175/1520-0469(1994)051<1605:SOCPMW>2.0.CO;2.
Canuto, V.M., F.O. Minotti, and O. Schilling, 1994: Differential rotation and turbulent convection: A new Reynolds stress model and comparison with solar data. Astrophys. J., 425, 303-325, doi:10.1086/173986.
Cheng, Y., and V.M. Canuto, 1994: Stably stratified shear turbulence: A new model for the energy dissipation length scale. J. Atmos. Sci., 51, 2384-2396, doi:10.1175/1520-0469(1994)051<2384:SSSTAN>2.0.CO;2.
Ying, R., V.M. Canuto, and R.M Ypma, 1994: Numerical simulation of flow data over two-dimensional hills. Bound.-Lay. Meteorol., 70, 401-427, doi:10.1007/BF00713778.
Canuto, V.M., 1993: Turbulent convection with overshooting: Reynolds stress approach. II. Astrophys. J., 416, 331-354, doi:10.1086/173238.
Canuto, V.M., and F. Minotti, 1993: Stratified turbulence in the atmosphere and oceans: A new subgrid model. J. Atmos. Sci., 50, 1925-1935, doi:10.1175/1520-0469(1993)050<1925:STITAA>2.0.CO;2.
Goldman, I., and V.M. Canuto, 1993: Cosmic turbulence revisited. Astrophys. J., 409, 495-503, doi:10.1086/172681.
Paterno, L., R. Ventura, V.M. Canuto, and I. Mazzitelli, 1993: Helioseismological test of a new model for stellar convection. Astrophys. J., 402, 733-740, doi:10.1086/172173.
Canuto, V.M., 1992: Turbulent convection with overshooting: Reynolds stress approach. Astrophys. J., 392, 218-232, doi:10.1086/171420.
Canuto, V.M., and I. Mazzitelli, 1992: Further improvements of a new model for turbulent convection in stars. Astrophys. J., 389, 724-730, doi:10.1086/171245.
Ronchi, C., M. Ypma, and V.M. Canuto, 1992: On the application of the Germano identity to subgrid-scale modeling. Phys. Fluids A, 12, 2927-2929, doi:10.1063/1.858346.
Savolainen, V., V.M. Canuto, and O. Schilling, 1992: Penetrative convection: Parameterized expression for the growth rates. Phys. Fluids A, 4, 626-629, doi:10.1063/1.858278.
Batchelor, G.K., V.M. Canuto, and J.R. Chasnov, 1991: Homogeneous buoyancy-generated turbulence. Phys. Fluids A, 3, 1444, doi:10.1063/1.858031.
Canuto, V.M., 1991: Turbulent convection: A new model. In The Sun and cool stars: Activity, magnetism, dynamos. I. Tuominen, D. Moss, and G. Rüdiger, Eds., Lecture Notes in Physics, vol. 380. Springer, pp. 27-32, doi:10.1007/3-540-53955-7_100.
Canuto, V.M., Y. Cheng, G.J. Hartke, and O. Schilling, 1991: Source function approach to turbulence bulk properties. Phys. Fluids A, 3, 1633-1644, doi:10.1063/1.857942.
Canuto, V.M., and I. Mazzitelli, 1991: Stellar turbulent convection: A new model and applications. Astrophys. J., 370, 295-311, doi:10.1086/169815.
Cabot, W., O. Hubickyj, J.B. Pollack, P. Cassen, and V.M. Canuto, 1990: Direct numerical simulations of turbulent convection: I. Variable gravity and uniform rotation. Geophys. Astrophys. Fluid Dynam., 53, 1-42.
Canuto, V.M., 1990: The mixing length parameter α. Astron. Astrophys., 227, 282-284.
Canuto, V.M., G.J. Hartke, A. Battaglia, J. Chasnov, and G.F. Albrecht, 1990: Theoretical study of turbulent channel flow: Bulk properties, pressure fluctuations, and propagation of electromagnetic waves. J. Fluid Mech., 211, 1-35, doi:10.1017/S0022112090001471.
Canuto, V.M., 1989: AMLT: Anisotropic mixing length theory. Astron. Astrophys., 217, 333-343.
Canuto, V.M., and I. Goldman, 1989: Astrophysical consequences of a violation of the strong equivalence principle. Intl. J. Theor. Phys., 28, 1019-1033, doi:10.1007/BF00670345.
Canuto, V.M., and I. Goldman, 1989: Atomic and gravitational clock. Intl. J. Theor. Phys., 28, 1005-1017, doi:10.1007/BF00670344.
Chasnov, J., V.M. Canuto, and R.S. Rogallo, 1989: Turbulence spectrum of strongly conductive temperature field in a rapidly stirred fluid. Phys. Fluids A, 1, 1698-1700, doi:10.1063/1.857535.
Canuto, V.M., I. Goldman, and J. Chasnov, 1988: Turbulent viscosity. Astron. Astrophys., 200, 291-300.
Chasnov, J., V.M. Canuto, and R.S. Rogallo, 1988: Turbulence spectrum of a passive temperature field: Results of a numerical simulation. Phys. Fluids, 31, 2065-2067, doi:10.1063/1.867013.
Hartke, G.J., V.M. Canuto, and C.T. Alonso, 1988: A direct interaction approximation treatment of turbulence in a compressible flud. I. Formalism. Phys. Fluids, 31, 1034-1050, doi:10.1063/1.866784.
Hartke, G.J., V.M. Canuto, and W.P. Dannevik, 1988: A direct interaction approximation treatment of high Rayleigh number convective turbulence and comparison with experiment. Phys. Fluids, 31, 256-262, doi:10.1063/1.866856.
Cabot, W., V.M. Canuto, O. Hubickyj, and J.B. Pollack, 1987: The role of turbulent convection in the primitive solar nebula: II. Results. Icarus, 69, 423-457, doi:10.1016/0019-1035(87)90017-0.
Cabot, W., V.M. Canuto, O. Hubickyj, and J.B. Pollack, 1987: The role of turbulent convection in the primitive solar nebula: I. Theory. Icarus, 69, 387-422, doi:10.1016/0019-1035(87)90016-9.
Canuto, V.M., I. Goldman, and J. Chasnov, 1987: A model for fully developed turbulence. Phys. Fluids, 30, 3391-3418, doi:10.1063/1.866472.
Canuto, V.M., and G.J. Hartke, 1986: Convective turbulence with rotation and magnetic fields. Astron. Astrophys., 168, 89-104.
Canuto, V.M., and G.J. Hartke, 1986: Propagation of electromagnetic waves in a turbulent medium. J. Opt. Soc. Amer. A, 3, 808-817.
Canuto, V.M., and A. Battaglia, 1985: Turbulence in molecular clouds: A new diagnostic tool to probe their origin. Astrophys. J., 294, L125-L129, doi:10.1086/184523.
Canuto, V.M., W. Cabot, G.J. Hartke, and A. Battaglia, 1985: Is the Kolmogoroff model applicable to large-scale turbulence? Astrophys. Space Sci., 116, 367-375, doi:10.1007/BF00653791.
Canuto, V.M., and I. Goldman, 1985: Analytical model for large-scale turbulence. Phys. Rev. Lett., 54, 430-433, doi:10.1103/PhysRevLett.54.430.
Canuto, V.M., I. Goldman, and O. Hubickyj, 1984: A formula for the Shakura-Sunyaev turbulent viscosity parameter. Astrophys. J., 280, L55-L58, doi:10.1086/184269.
Canuto, V.M., I. Goldman, and I.I. Shapiro, 1984: Testing the Strong Equivalence Principle by radio ranging. Astrophys. J., 276, 1-3, doi:10.1086/161587.
Adams, P.J., V.M. Canuto, I. Goldman, and R.W. Hellings, 1983: Testing for a cosmological influence on local physics using atomic and gravitational clocks. Phys. Rev. D, 28, 1822-1828, doi:10.1103/PhysRevD.28.1822.
Canuto, V.M., and I. Goldman, 1983: Astrophysical consequences of a violation of the strong equivalence principle. Nature, 304, 311-315, doi:10.1038/304311a0.
Canuto, V.M., and I. Goldman, 1983: The opacity of the universe and the strong equivalence principle. Phys. Lett. A, 95, 65-68, doi:10.1016/0375-9601(83)90784-3.
Canuto, V.M., J.S. Levine, T.R. Augustsson, and C.L. Imhoff, 1983: Oxygen and ozone in the early Earth's atmosphere. Precambrian Res., 20, 109-120, doi:10.1016/0301-9268(83)90068-2.
Canuto, V.M., J.S. Levine, T.R. Augustsson, C.L. Imhoff, and M.S. Giampapa, 1983: The young Sun and the atmosphere and photochemistry of the early Earth. Nature, 305, 281-286, doi:10.1038/305281a0.
Hellings, R.W., P.J. Adams, J.D. Anderson, M.S. Keesey, E.L. Lau, E.M. Standish, V.M. Canuto, and I. Goldman, 1983: Experimental test of the variability of G using Viking Lander ranging data. Phys. Rev. Lett, 51, 1609-1612, doi:10.1103/PhysRevLett.51.1609.
Canuto, V.M., and I. Goldman, 1982: Atomic and gravitational clocks. Nature, 296, 709-713, doi:10.1038/296709a0.
Canuto, V.M., and I. Goldman, 1982: Why a variable G? Astrophys. Space Sci., 86, 225-227, doi:10.1007/BF00651845.
Canuto, V.M., J.S. Levine, T.R. Augustsson, and C.L. Imhoff, 1982: UV radiation from the young Sun and oxygen and ozone levels in the prebiological palaeoatmosphere. Nature, 296, 816-820, doi:10.1038/296816a0.
Canuto, V.M., 1981: On the variation of G and scale invariant gravitation — A reply. M. Not. Royal Astron. Soc., 197, 1093-1095.
Canuto, V.M., 1981: The Earth's radius and the G variation. Nature, 290, 739-744, doi:10.1038/290739a0.
Canuto, V.M., and S.-H. Hsieh, 1981: Scale covariant gravitation. VI. Stellar structure and evolution. Astrophys. J., 248, 801-812, doi:10.1086/159204.
Hsieh, S.-H., and V.M. Canuto, 1981: Scale covariant gravitation. V. Kinetic theory. Astrophys. J., 248, 790-800, doi:10.1086/159203.
Canuto, V., and S.-H. Hsieh, 1980: Comment on the paper 'A cosmological limit on the possible variation of G'. M. Not. Royal Astron. Soc., 191, 605-606.
Canuto, V., and S.-H. Hsieh, 1980: Primordial nucleosynthesis and Dirac's large numbers hypothesis. Astrophys. J. Lett., 239, L91, doi:10.1086/183299.
Canuto, V., S.-H. Hsieh, and J.R. Owen, 1980: Possible determination of the deceleration parameter using lunar occultations and laser ranging observations. Astrophys. J., 241, 886-888, doi:10.1086/158401.
Canuto, V.M., and S.-H. Hsieh, 1980: Case for an open universe. Phys. Rev. Lett., 44, 695-698, doi:10.1103/PhysRevLett.44.695.
Canuto, V.M., and S.-H. Hsieh, 1980: Cosmological variation of G and the solar luminosity. Astrophys. J., 237, 613-615, doi:10.1086/157905.
Canuto, V.M., S.-H. Hsieh, and J.R. Owen, 1980: Cosmological considerations on the diffuse γ-ray isotropic background. Astrophys. J., 235, 688-693, doi:10.1086/157672.
Canuto, V.M., and J.V. Narlikar, 1980: Cosmological tests of the Hoyle-Narlikar conformal gravity. Astrophys. J., 236, 6-23, doi:10.1086/157714.
Canuto, V.M., J.R. Owen, and J.V. Narlikar, 1980: The diffuse gamma-ray background in the Hoyle-Narlikar cosmology. Astron. Astrophys., 92, 26-29.
Canuto, V., and B. Datta, 1979: High density matter in the universe. Nuclear Phys. A, 328, 320-351, doi:10.1016/0375-9474(79)90226-4.
Canuto, V., B. Datta, and G. Kalman, 1979: Astrophysical determination of the scale parameter in QCD. Phys. Lett. B, 85, 467-470, doi:10.1016/0370-2693(79)91297-8.
Canuto, V.M., S.-H. Hsieh, and J.R. Owen, 1979: Varying G. M. Not. Royal Astron. Soc., 188, 829-837.
Canuto, V.M., and J.R. Owen, 1979: Scale covariance and G-varying cosmology. IV. The log N-log S relation. Astrophys. J. Supp. Series, 41, 301-326, doi:10.1086/190620.
Canuto, V.M., and S.-H. Shieh, 1979: Scale covariance and G-varying cosmology. II - Thermodynamics, radiation, and the 3 K background. Astrophys. J. Supp. Series, 41, 243-262, doi:10.1086/190618.
Chou, C.K., L. Fassio-Canuto, and V. Canuto, 1978: Photoneutrino reactions in a superstrong magnetoactive plasma. Astrophys. J., 227, 974-986, doi:10.1086/156806.
Canuto, V., 1978: On the origin of Hawking mini black-holes and the cold early universe. M. Not. Royal Astron. Soc., 184, 721-725.
Canuto, V., B. Datta, and G. Kalman, 1978: Superdense neutron matter. Astrophys. J., 221, 274-283, doi:10.1086/156026.
Canuto, V., and S.-H. Hsieh, 1978: Scale covariant cosmology and the temperature of the Earth. Astron. Astrophys., 65, 389-391.
Canuto, V., and S.-H. Hsieh, 1978: The 3 K blackbody radiation, Dirac's Large Numbers Hypothesis, and scale-covariant cosmology. Astrophys. J., 224, 302-307, doi:10.1086/156378.
Canuto, V., S.-H. Hsieh, and P.J. Adams, 1978: Mach's principle, the cosmological constant, and the scale-covariant theory of gravity. Phys. Rev. D, 18, 3577-3580, doi:10.1103/PhysRevD.18.3577.
Canuto, V., and L. Owen, 1978: On the origin of the absorption spectra of quasi-stellar and BL Lacertae objects. Astrophys. J., 225, 79-82, doi:10.1086/156469.
Canuto, V., P.J. Adams, S.-H. Hsieh, and E. Tsiang, 1977: Scale-covariant theory of gravitation and astrophysical applications. Phys. Rev. D, 16, 1643-1663, doi:10.1103/PhysRevD.16.1643.
Canuto, V., H.S. Hsieh, and P.J. Adams, 1977: Scale-covariant theory of gravitation and astrophysical applications. Phys. Rev. Lett., 39, 429-432, doi:10.1103/PhysRevLett.39.429.
Canuto, V., and J.F. Lee, 1977: The cosmological constant, broken gauge theories and 3 K black-body radiation. Phys. Lett. B, 72, 281-284, doi:10.1016/0370-2693(77)90722-5.
Canuto, V., and J. Lodenquai, 1977: Dirac cosmology. Astrophys. J., 211, 342-356.
Canuto, V., and E. Tsiang, 1977: On the hydrodynamic expansion of a relativistic gas. Astrophys. J., 213, 27-37, doi:10.1086/155124.
Adams, P.J., and V. Canuto, 1976: Dirac cosmology and the onset of galactic nucleosynthesis. Phys. Lett. B, 65, 187-188, doi:10.1016/0370-2693(76)90029-0.
Adams, P.J., V. Canuto, and H.-Y. Chiu, 1976: Magnetic monopoles and cosmology. Phys. Lett. B, 61, 397-399, doi:10.1016/0370-2693(76)90598-0.
Canuto, V., 1976: Inhomogeneities in the early universe. Astrophys. J., 205, 659-673.
Canuto, V., P.J. Adams, S.H. Hsieh, and E. Tsiang, 1976: Particle creation and Dirac's Large Numbers Hypothesis. Nature, 264, 485, doi:10.1038/264485a0.
Canuto, V., P.J. Adams, and E. Tsiang, 1976: Crystal structure and Dirac's Large Numbers Hypothesis. Nature, 261, 438, doi:10.1038/261438a0.
Canuto, V., and E. Tsiang, 1976: On the equation of state for an electron gas in an intense magnetic field. Phys. Lett. B, 62, 366-368, doi:10.1016/0370-2693(76)90098-8.
Kalman, G., V. Canuto, and B. Datta, 1976: Self-consistency condition and high-density virial theorem in relativistic many-particle systems. Phys. Rev. D, 13, 3493-3494, doi:10.1103/PhysRevD.13.3493.
Adams, P.J., and V. Canuto, 1975: Exact solution of the Lifshitz equations governing the growth of fluctuations in cosmology. Phys. Rev. D, 12, 3793-3799, doi:10.1103/PhysRevD.12.3793.
Canuto, V., 1975: Equation of state at ultrahigh densities: Part 2. Ann. Rev. Astron. Astrophys., 13, 335-380.
Canuto, V., and B. Datta, 1975: Meson-meson interactions and the equation of state for dense nucleons. Phys. Lett. B, 56, 148-150, doi:10.1016/0370-2693(75)90289-0.
Canuto, V., B. Datta, and J. Lodenquai, 1975: Structure of neutron star cores. Astrophys. Space Sci., 34, 223-229, doi:10.1007/BF00646762.
Canuto, V., and J. Lodenquai, 1975: Behavior of matter at superhigh density. Phys. Rev. D, 11, 233-244, doi:10.1103/PhysRevD.11.233.
Canuto, V., and J. Lodenquai, 1975: Solidification of neutron matter. Phys. Rev. C, 12, 2033-2037, doi:10.1103/PhysRevC.12.2033.
Canuto, V., and S.M. Chitre, 1974: Crystallization of dense neutron matter. Phys. Rev. D, 9, 1587-1613, doi:10.1103/PhysRevD.9.1587.
Canuto, V., C. Chiuderi, C.K. Chou, and L. Fassio-Canuto, 1974: Neutrino reactions in strong magnetic field. Astrophys. Space Sci., 28, 145-161, doi:10.1007/BF00642244.
Canuto, V., J. Lodenquai, L. Paris, and S.M. Chitre, 1974: t-Matrix calculation of the ground-state energies of solid 3He. J. Low Temp. Phys., 17, 179-190, doi:10.1007/BF00654553.
Chen, H.-H., M.A. Ruderman, and V. Canuto, 1974: Neutrino emission from plasmons in strong magnetic fields. Astrophys. Space Sci., 31, 187-191, doi:10.1007/BF00642609.
Lodenquai, J., V. Canuto, M. Ruderman, and S. Tsuruta, 1974: Photon opacity in surfaces of magnetic neutron stars. Astrophys. J., 190, 141-152.
Canuto, V., and S.M. Chitre, 1973: Solidification of neutron matter. Phys. Rev. Lett., 30, 99-1002, doi:10.1103/PhysRevLett.30.999.
Canuto, V., and C.K. Chou, 1973: New dispersion relation for a strongly magnetized degenerate electron plasma with anisotropic pressure. Phys. Fluids, 16, 1273-1276, doi:10.1063/1.1694508.
Canuto, V., and L. Fassio-Canuto, 1973: Pair annihilation into neutrinos in strong magnetic fields. Phys. Rev. D, 7, 1593-1600, doi:10.1103/PhysRevD.7.1593.
Canuto, V., and L. Fassio-Canuto, 1973: Photoneutrino energy losses in strong magnetic fields. Phys. Rev. D, 7, 1601-1608, doi:10.1103/PhysRevD.7.1601.
Canuto, V., J. Lodenquai, and S.M. Chitre, 1973: T-matrix calculations of the ground-state energies of solid He3 and solid H2. Phys. Rev. A, 8, 949-963, doi:10.1103/PhysRevA.8.949.
Canuto, V., and D.C. Kelly, 1972: Hydrogen atom in intense magnetic field. Astrophys. Space Sci., 17, 277-291, doi:10.1007/BF00642901.
Canuto, V., and J. Ventura, 1972: Quantum theory of the dielectric constant of a magnetized plasma and astrophysical applications. I: Theory. Astrophys. Space Sci., 18, 104-120, doi:10.1007/BF00645284.
Tsuruta, S., V. Canuto, J. Lodenquai, and M. Ruderman, 1972: Cooling of Pulsars. Astrophys. J., 176, 739-744.
Canuto, V., 1971: Quantum-mechanical relation for a magnetized electron gas. Phys. Rev. A, 3, 648-650, doi:10.1103/PhysRevA.3.648.
Canuto, V., and H.Y. Chiu, 1971: Intense magnetic fields in astrophysics. Space Sci. Rev., 12, 3-74, doi:10.1007/BF00172129.
Canuto, V., and C.K. Chou, 1971: Neutrino luminosity by the ordinary URCA process in an intense magnetic field. Astrophys. Space Sci., 10, 246-264, doi:10.1007/BF00704085.
Canuto, V., J. Lodenquai, and M. Ruderman, 1971: Thomson scattering in a strong magnetic field. Phys. Rev. D, 3, 2303-2308, doi:10.1103/PhysRevD.3.2303.
Chiu, H.Y., and V. Canuto, 1971: Theory of radiation mechanism of pulsars. I. Astrophys. J., 163, 577-594.
Canuto, V., 1970: Electrical conductivity and conductive opacity of a relativistic electron gas. Astrophys. J., 159, 641-652.
Canuto, V., 1970: Radiative opacities and Compton scattering in strong magnetic fields. Astrophys. J., 160, L153-L155.
Canuto, V., and H.Y. Chiu, 1970: Nonrelativistic electron bremsstrahlung in a strongly magnetized plasma. Phys. Rev. A, 2, 518-525, doi:10.1103/PhysRevA.2.518.
Canuto, V., H.Y. Chiu, C. Chiuderi, and H.J. Lee, 1970: New source of intense magnetic fields in neutron stars. Nature, 225, 47-48, doi:10.1038/225047a0.
Canuto, V., H.Y. Chiu, and C.K. Chou, 1970: Neutrino bremsstrahlung in an intense magnetic field. Phys. Rev. D, 2, 281-287, doi:10.1103/PhysRevD.2.281.
Canuto, V., and C. Chiuderi, 1970: Transverse electrical conductivity of a relativistic gas in an intense magnetic field. Phys. Rev. D, 1, 2219-2226, doi:10.1103/PhysRevD.1.2219.
Canuto, V., C. Chiuderi, and C.K. Chou, 1970: Plasmon neutrinos emission in a strong magnetic field. I: Transverse plasmons. Astrophys. Space Sci., 7, 407-415, doi:10.1007/BF00653279.
Canuto, V., C. Chiuderi, and C.K. Chou, 1970: Plasmon neutrinos emission in a strong magnetic field. II: Longitudinal plasmons. Astrophys. Space Sci., 7, 453-460, doi:10.1007/BF00649583.
Canuto, V., and A.B. Solinger, 1970: Conductivity in neutron star crusts. Astrophys. Lett., 6, 141-142.
Chiu, H.-Y., and V. Canuto, 1970: Bremsstrahlung radiation in an intense magnetic field and emission from pulsars. Nature, 225, 1230-1231, doi:10.1038/2251230a0.
Canuto, V., and H.-Y. Chiu, 1969: Longitudinal electrical conductivity of a relativistic gas in an intense magnetic field. Phys. Rev., 188, 2446-2454, doi:10.1103/PhysRev.188.2446.
Canuto, V., H.-Y. Chiu, and L. Fassio-Canuto, 1969: Electron bremsstrahlung in intense magnetic fields. Phys. Rev., 185, 1607-1613, doi:10.1103/PhysRev.185.1607.
Canuto, V., H.-Y. Chiu, and L. Fassio-Canuto, 1969: Thermodynamic approach to the equation of state of a magnetized Fermi gas. Astrophys. Space Sci., 3, 258-267, doi:10.1007/BF00651031.
Chiu, H.-Y., and V. Canuto, 1969: Radio emission from magnetic neutron stars. A possible model for pulsars. Phys. Rev. Lett., 22, 415-419, doi:10.1103/PhysRevLett.22.415.
Chiu, H.-Y., V. Canuto, and L. Fassio-Canuto, 1969: Nature of radio and optical emissions from pulsars. Nature, 221, 529-531, doi:10.1038/221529a0.
Lee, H.J., V. Canuto, H.-Y. Chiu, and C. Chiuderi, 1969: New state of ferromagnetism in degenerate electron gas and magnetic fields in collapsed bodies. Phys. Rev. Lett., 23, 390-393, doi:10.1103/PhysRevLett.23.390.
Canuto, V., and H.-Y. Chiu, 1968: Magnetic moment of a magnetized Fermi gas. Phys. Rev., 173, 1229-1235, doi:10.1103/PhysRev.173.1229.
Canuto, V., and H.-Y. Chiu, 1968: Thermodynamic properties of a magnetized Fermi gas. Phys. Rev., 173, 1220-1228, doi:10.1103/PhysRev.173.1220.
Canuto, V., and H.-Y. Chiu, 1968: Quantum theory of an electron gas in intense magnetic fields. Phys. Rev., 173, 1210-1219, doi:10.1103/PhysRev.173.1210.
Chiu, H.-Y., and V. Canuto, 1968: Properties of high-density matter in intense magnetic fields. Phys. Rev. Lett., 21, 110-113, doi:10.1103/PhysRevLett.21.110.
Chiu, H.-Y., and V. Canuto, 1968: Problem of intense magnetic field in gravitational collapse. Astrophys. J., 153, L157-L161.
Chiu, H.-Y., V. Canuto, and L. Fassio-Canuto, 1968: Quantum theory of an electron gas with anomalous magnetic moments in intense magnetic fields. Phys. Rev., 176, 1438-1442, doi:10.1103/PhysRev.176.1438.