Is the term 'matter' in 'dark matter' misleading?

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If the only evidence for dark matter we have is gravitational, why call it 'matter' rather than 'observed space-time geometry that does not match predictions'?



General Relativity tells us that mass distorts local space-time but as far as I know, it doesn't say that it is the only thing that does so - isn't for all we know space-time is more fundamental than mass and can have local distortions caused by the big bang / inflationary epoch / flying-spaghetti-monster blueprints?










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  • 1




    It's not just mass. GR says that stress-energy induces spacetime curvature.
    – PM 2Ring
    4 hours ago










  • +1 for invoking the flying-spaghetti-monster. Einstein must have missed that one ;)
    – Time4Tea
    2 hours ago










  • Yes, but it doesn't matter.
    – Evargalo
    1 hour ago














up vote
2
down vote

favorite












If the only evidence for dark matter we have is gravitational, why call it 'matter' rather than 'observed space-time geometry that does not match predictions'?



General Relativity tells us that mass distorts local space-time but as far as I know, it doesn't say that it is the only thing that does so - isn't for all we know space-time is more fundamental than mass and can have local distortions caused by the big bang / inflationary epoch / flying-spaghetti-monster blueprints?










share|cite|improve this question









New contributor




AlternativelyBaryonic is a new contributor to this site. Take care in asking for clarification, commenting, and answering.
Check out our Code of Conduct.















  • 1




    It's not just mass. GR says that stress-energy induces spacetime curvature.
    – PM 2Ring
    4 hours ago










  • +1 for invoking the flying-spaghetti-monster. Einstein must have missed that one ;)
    – Time4Tea
    2 hours ago










  • Yes, but it doesn't matter.
    – Evargalo
    1 hour ago












up vote
2
down vote

favorite









up vote
2
down vote

favorite











If the only evidence for dark matter we have is gravitational, why call it 'matter' rather than 'observed space-time geometry that does not match predictions'?



General Relativity tells us that mass distorts local space-time but as far as I know, it doesn't say that it is the only thing that does so - isn't for all we know space-time is more fundamental than mass and can have local distortions caused by the big bang / inflationary epoch / flying-spaghetti-monster blueprints?










share|cite|improve this question









New contributor




AlternativelyBaryonic is a new contributor to this site. Take care in asking for clarification, commenting, and answering.
Check out our Code of Conduct.











If the only evidence for dark matter we have is gravitational, why call it 'matter' rather than 'observed space-time geometry that does not match predictions'?



General Relativity tells us that mass distorts local space-time but as far as I know, it doesn't say that it is the only thing that does so - isn't for all we know space-time is more fundamental than mass and can have local distortions caused by the big bang / inflationary epoch / flying-spaghetti-monster blueprints?







general-relativity dark-matter






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edited 5 hours ago





















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  • 1




    It's not just mass. GR says that stress-energy induces spacetime curvature.
    – PM 2Ring
    4 hours ago










  • +1 for invoking the flying-spaghetti-monster. Einstein must have missed that one ;)
    – Time4Tea
    2 hours ago










  • Yes, but it doesn't matter.
    – Evargalo
    1 hour ago












  • 1




    It's not just mass. GR says that stress-energy induces spacetime curvature.
    – PM 2Ring
    4 hours ago










  • +1 for invoking the flying-spaghetti-monster. Einstein must have missed that one ;)
    – Time4Tea
    2 hours ago










  • Yes, but it doesn't matter.
    – Evargalo
    1 hour ago







1




1




It's not just mass. GR says that stress-energy induces spacetime curvature.
– PM 2Ring
4 hours ago




It's not just mass. GR says that stress-energy induces spacetime curvature.
– PM 2Ring
4 hours ago












+1 for invoking the flying-spaghetti-monster. Einstein must have missed that one ;)
– Time4Tea
2 hours ago




+1 for invoking the flying-spaghetti-monster. Einstein must have missed that one ;)
– Time4Tea
2 hours ago












Yes, but it doesn't matter.
– Evargalo
1 hour ago




Yes, but it doesn't matter.
– Evargalo
1 hour ago










2 Answers
2






active

oldest

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up vote
8
down vote













As the universe expands you would expect the density of the stuff in it to decrease for the obvious reason that the amount of stuff remains constant while the volume increases. So you'd expect something like:



$$ rho propto frac1V propto frac1a^3 $$



where $a$ is the linear scale factor (i.e. $a^3$ is the volume scale factor).



However things are more complicated than this. For radiation and highly relativistic matter the energy density decreases as $a^-4$, while for a cosmological constant the energy density doesn't decrease at all but remains constant. It is only matter, and specifically pressureless matter, that decreases as $a^-3$.



And the stuff that we call dark matter decreases as $a^-3$ just like regular matter, so whatever it is it behaves like matter. Hence the name dark matter.






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  • What results are considered to observe this 'stuff' decrease as $a^-3$ rather than not-enough regular matter decreasing as $a^-3$ ?
    – AlternativelyBaryonic
    5 hours ago







  • 1




    @AlternativelyBaryonic the current best measurements of the dark energy density and behaviour come from the Planck experiment to observe the microwave background.
    – John Rennie
    4 hours ago










  • Dark matter or dark energym Is this really dark matter?
    – Vladimir F
    1 hour ago

















up vote
0
down vote













According to the Einstein-Cartan version of gravity, there are two sources which "distort" local space-time:




  1. Mass (or more generally energy-momentum tensor), which induces space-time curvature.


  2. Spin current (from Dirac fermions), which induces space-time torsion.

As an alternative to missing/dark mass, we could attribute the "observed space-time geometry that does not match predictions" to dark spin current (or dubbed as " flying-spaghetti-monster", if you will).



As per Poplawski, the spin current/torsion approach has another nice property that "averts the unphysical big-bang singularity, replacing it with a cusp-like bounce at a finite minimum scale factor, before which the Universe was contracting".






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    2 Answers
    2






    active

    oldest

    votes








    2 Answers
    2






    active

    oldest

    votes









    active

    oldest

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    active

    oldest

    votes








    up vote
    8
    down vote













    As the universe expands you would expect the density of the stuff in it to decrease for the obvious reason that the amount of stuff remains constant while the volume increases. So you'd expect something like:



    $$ rho propto frac1V propto frac1a^3 $$



    where $a$ is the linear scale factor (i.e. $a^3$ is the volume scale factor).



    However things are more complicated than this. For radiation and highly relativistic matter the energy density decreases as $a^-4$, while for a cosmological constant the energy density doesn't decrease at all but remains constant. It is only matter, and specifically pressureless matter, that decreases as $a^-3$.



    And the stuff that we call dark matter decreases as $a^-3$ just like regular matter, so whatever it is it behaves like matter. Hence the name dark matter.






    share|cite|improve this answer




















    • What results are considered to observe this 'stuff' decrease as $a^-3$ rather than not-enough regular matter decreasing as $a^-3$ ?
      – AlternativelyBaryonic
      5 hours ago







    • 1




      @AlternativelyBaryonic the current best measurements of the dark energy density and behaviour come from the Planck experiment to observe the microwave background.
      – John Rennie
      4 hours ago










    • Dark matter or dark energym Is this really dark matter?
      – Vladimir F
      1 hour ago














    up vote
    8
    down vote













    As the universe expands you would expect the density of the stuff in it to decrease for the obvious reason that the amount of stuff remains constant while the volume increases. So you'd expect something like:



    $$ rho propto frac1V propto frac1a^3 $$



    where $a$ is the linear scale factor (i.e. $a^3$ is the volume scale factor).



    However things are more complicated than this. For radiation and highly relativistic matter the energy density decreases as $a^-4$, while for a cosmological constant the energy density doesn't decrease at all but remains constant. It is only matter, and specifically pressureless matter, that decreases as $a^-3$.



    And the stuff that we call dark matter decreases as $a^-3$ just like regular matter, so whatever it is it behaves like matter. Hence the name dark matter.






    share|cite|improve this answer




















    • What results are considered to observe this 'stuff' decrease as $a^-3$ rather than not-enough regular matter decreasing as $a^-3$ ?
      – AlternativelyBaryonic
      5 hours ago







    • 1




      @AlternativelyBaryonic the current best measurements of the dark energy density and behaviour come from the Planck experiment to observe the microwave background.
      – John Rennie
      4 hours ago










    • Dark matter or dark energym Is this really dark matter?
      – Vladimir F
      1 hour ago












    up vote
    8
    down vote










    up vote
    8
    down vote









    As the universe expands you would expect the density of the stuff in it to decrease for the obvious reason that the amount of stuff remains constant while the volume increases. So you'd expect something like:



    $$ rho propto frac1V propto frac1a^3 $$



    where $a$ is the linear scale factor (i.e. $a^3$ is the volume scale factor).



    However things are more complicated than this. For radiation and highly relativistic matter the energy density decreases as $a^-4$, while for a cosmological constant the energy density doesn't decrease at all but remains constant. It is only matter, and specifically pressureless matter, that decreases as $a^-3$.



    And the stuff that we call dark matter decreases as $a^-3$ just like regular matter, so whatever it is it behaves like matter. Hence the name dark matter.






    share|cite|improve this answer












    As the universe expands you would expect the density of the stuff in it to decrease for the obvious reason that the amount of stuff remains constant while the volume increases. So you'd expect something like:



    $$ rho propto frac1V propto frac1a^3 $$



    where $a$ is the linear scale factor (i.e. $a^3$ is the volume scale factor).



    However things are more complicated than this. For radiation and highly relativistic matter the energy density decreases as $a^-4$, while for a cosmological constant the energy density doesn't decrease at all but remains constant. It is only matter, and specifically pressureless matter, that decreases as $a^-3$.



    And the stuff that we call dark matter decreases as $a^-3$ just like regular matter, so whatever it is it behaves like matter. Hence the name dark matter.







    share|cite|improve this answer












    share|cite|improve this answer



    share|cite|improve this answer










    answered 6 hours ago









    John Rennie

    265k41518765




    265k41518765











    • What results are considered to observe this 'stuff' decrease as $a^-3$ rather than not-enough regular matter decreasing as $a^-3$ ?
      – AlternativelyBaryonic
      5 hours ago







    • 1




      @AlternativelyBaryonic the current best measurements of the dark energy density and behaviour come from the Planck experiment to observe the microwave background.
      – John Rennie
      4 hours ago










    • Dark matter or dark energym Is this really dark matter?
      – Vladimir F
      1 hour ago
















    • What results are considered to observe this 'stuff' decrease as $a^-3$ rather than not-enough regular matter decreasing as $a^-3$ ?
      – AlternativelyBaryonic
      5 hours ago







    • 1




      @AlternativelyBaryonic the current best measurements of the dark energy density and behaviour come from the Planck experiment to observe the microwave background.
      – John Rennie
      4 hours ago










    • Dark matter or dark energym Is this really dark matter?
      – Vladimir F
      1 hour ago















    What results are considered to observe this 'stuff' decrease as $a^-3$ rather than not-enough regular matter decreasing as $a^-3$ ?
    – AlternativelyBaryonic
    5 hours ago





    What results are considered to observe this 'stuff' decrease as $a^-3$ rather than not-enough regular matter decreasing as $a^-3$ ?
    – AlternativelyBaryonic
    5 hours ago





    1




    1




    @AlternativelyBaryonic the current best measurements of the dark energy density and behaviour come from the Planck experiment to observe the microwave background.
    – John Rennie
    4 hours ago




    @AlternativelyBaryonic the current best measurements of the dark energy density and behaviour come from the Planck experiment to observe the microwave background.
    – John Rennie
    4 hours ago












    Dark matter or dark energym Is this really dark matter?
    – Vladimir F
    1 hour ago




    Dark matter or dark energym Is this really dark matter?
    – Vladimir F
    1 hour ago










    up vote
    0
    down vote













    According to the Einstein-Cartan version of gravity, there are two sources which "distort" local space-time:




    1. Mass (or more generally energy-momentum tensor), which induces space-time curvature.


    2. Spin current (from Dirac fermions), which induces space-time torsion.

    As an alternative to missing/dark mass, we could attribute the "observed space-time geometry that does not match predictions" to dark spin current (or dubbed as " flying-spaghetti-monster", if you will).



    As per Poplawski, the spin current/torsion approach has another nice property that "averts the unphysical big-bang singularity, replacing it with a cusp-like bounce at a finite minimum scale factor, before which the Universe was contracting".






    share|cite|improve this answer


























      up vote
      0
      down vote













      According to the Einstein-Cartan version of gravity, there are two sources which "distort" local space-time:




      1. Mass (or more generally energy-momentum tensor), which induces space-time curvature.


      2. Spin current (from Dirac fermions), which induces space-time torsion.

      As an alternative to missing/dark mass, we could attribute the "observed space-time geometry that does not match predictions" to dark spin current (or dubbed as " flying-spaghetti-monster", if you will).



      As per Poplawski, the spin current/torsion approach has another nice property that "averts the unphysical big-bang singularity, replacing it with a cusp-like bounce at a finite minimum scale factor, before which the Universe was contracting".






      share|cite|improve this answer
























        up vote
        0
        down vote










        up vote
        0
        down vote









        According to the Einstein-Cartan version of gravity, there are two sources which "distort" local space-time:




        1. Mass (or more generally energy-momentum tensor), which induces space-time curvature.


        2. Spin current (from Dirac fermions), which induces space-time torsion.

        As an alternative to missing/dark mass, we could attribute the "observed space-time geometry that does not match predictions" to dark spin current (or dubbed as " flying-spaghetti-monster", if you will).



        As per Poplawski, the spin current/torsion approach has another nice property that "averts the unphysical big-bang singularity, replacing it with a cusp-like bounce at a finite minimum scale factor, before which the Universe was contracting".






        share|cite|improve this answer














        According to the Einstein-Cartan version of gravity, there are two sources which "distort" local space-time:




        1. Mass (or more generally energy-momentum tensor), which induces space-time curvature.


        2. Spin current (from Dirac fermions), which induces space-time torsion.

        As an alternative to missing/dark mass, we could attribute the "observed space-time geometry that does not match predictions" to dark spin current (or dubbed as " flying-spaghetti-monster", if you will).



        As per Poplawski, the spin current/torsion approach has another nice property that "averts the unphysical big-bang singularity, replacing it with a cusp-like bounce at a finite minimum scale factor, before which the Universe was contracting".







        share|cite|improve this answer














        share|cite|improve this answer



        share|cite|improve this answer








        edited 2 hours ago

























        answered 2 hours ago









        MadMax

        201110




        201110




















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