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- W2037616306 abstract "We make steps in a new direction by considering fluids with EoS of more general form<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M1><mml:mrow><mml:mi>F</mml:mi><mml:mo stretchy=false>(</mml:mo><mml:mi>ρ</mml:mi><mml:mo>,</mml:mo><mml:mi>P</mml:mi><mml:mo stretchy=false>)</mml:mo><mml:mo>=</mml:mo><mml:mn>0</mml:mn></mml:mrow></mml:math>. It is thought that there should be interaction between cosmic fluids, but this assumption for this stage carries only phenomenological character opening a room for different kinds of manipulations. In this paper we will consider a modification of an interaction<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M2><mml:mrow><mml:mi>Q</mml:mi></mml:mrow></mml:math>, where we accept that interaction parameter<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M3><mml:mrow><mml:msub><mml:mi>b</mml:mi><mml:mn>1</mml:mn></mml:msub></mml:mrow></mml:math>(order of unity) in<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M4><mml:mrow><mml:mi>Q</mml:mi><mml:mo>=</mml:mo><mml:mn>3</mml:mn><mml:mi>H</mml:mi><mml:msub><mml:mi>b</mml:mi><mml:mn>1</mml:mn></mml:msub><mml:mi>ρ</mml:mi></mml:mrow></mml:math>is time dependent and presented as a linear function of Hubble parameter<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M5><mml:mrow><mml:mi>H</mml:mi></mml:mrow></mml:math>of the form<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M6><mml:mrow><mml:msub><mml:mi>b</mml:mi><mml:mn>0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi>b</mml:mi><mml:mi>t</mml:mi><mml:mi>H</mml:mi></mml:mrow></mml:math>, where<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M7><mml:mrow><mml:mi>b</mml:mi></mml:mrow></mml:math>and<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M8><mml:mrow><mml:msub><mml:mi>b</mml:mi><mml:mn>0</mml:mn></mml:msub></mml:mrow></mml:math>are constants. We consider two different models including modified Chaplygin gas and polytropic gas which have bulk viscosity. Then, we investigate problem numerically and analyze behavior of different cosmological parameters concerning fluids and behavior of the universe." @default.
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- W2037616306 date "2014-01-01" @default.
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- W2037616306 title "Hubble Parameter Corrected Interactions in Cosmology" @default.
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- W2037616306 doi "https://doi.org/10.1155/2014/129085" @default.
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