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black dwarf stars and dark matter
How can Y-dwarf stars have such a low temperature?Dark Matter 'Stars'Dark matter and black holeDid dark matter cause the formation of the Solar System?Are black holes in a binary system with white holes, and are they both wormholes?Do clouds of dark matter cool and contract?Direct Dark Matter Detection: relative velocity between WIMPs & NucleiWhen and where was WIMP dark matter formed?Overlap between experimental searches for axion and WIMP dark matterWhat is the theoretical lower mass limit for a white dwarf?
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Today we understand that a black dwarf star represents a hypothetical star that is the result of the complete consumption of the energy of a white dwarf which is the remnant of a star of little or half mass (1 solar mass), once all its hydrogen has been consumed or expelled. This rest is a dense piece of "degenerated matter" that slowly cools and crystallizes by emission of heat radiation. So, if these objects (not yet observed) do not emit light but interact gravitationally with the surrounding matter, we can not say that dark matter may be black dwarf stars that are contained within the galactic halo? To discard weak interaction particles such as WIMP's or its opposite, the MACHO's ("massive compact halo objects")
astrophysics astronomy dark-matter stars wimps
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add a comment |
$begingroup$
Today we understand that a black dwarf star represents a hypothetical star that is the result of the complete consumption of the energy of a white dwarf which is the remnant of a star of little or half mass (1 solar mass), once all its hydrogen has been consumed or expelled. This rest is a dense piece of "degenerated matter" that slowly cools and crystallizes by emission of heat radiation. So, if these objects (not yet observed) do not emit light but interact gravitationally with the surrounding matter, we can not say that dark matter may be black dwarf stars that are contained within the galactic halo? To discard weak interaction particles such as WIMP's or its opposite, the MACHO's ("massive compact halo objects")
astrophysics astronomy dark-matter stars wimps
$endgroup$
$begingroup$
I'm pretty sure the "degenerated matter" of the black dwarf is still made of baryons, so it is not dark matter.
$endgroup$
– N. Steinle
4 hours ago
add a comment |
$begingroup$
Today we understand that a black dwarf star represents a hypothetical star that is the result of the complete consumption of the energy of a white dwarf which is the remnant of a star of little or half mass (1 solar mass), once all its hydrogen has been consumed or expelled. This rest is a dense piece of "degenerated matter" that slowly cools and crystallizes by emission of heat radiation. So, if these objects (not yet observed) do not emit light but interact gravitationally with the surrounding matter, we can not say that dark matter may be black dwarf stars that are contained within the galactic halo? To discard weak interaction particles such as WIMP's or its opposite, the MACHO's ("massive compact halo objects")
astrophysics astronomy dark-matter stars wimps
$endgroup$
Today we understand that a black dwarf star represents a hypothetical star that is the result of the complete consumption of the energy of a white dwarf which is the remnant of a star of little or half mass (1 solar mass), once all its hydrogen has been consumed or expelled. This rest is a dense piece of "degenerated matter" that slowly cools and crystallizes by emission of heat radiation. So, if these objects (not yet observed) do not emit light but interact gravitationally with the surrounding matter, we can not say that dark matter may be black dwarf stars that are contained within the galactic halo? To discard weak interaction particles such as WIMP's or its opposite, the MACHO's ("massive compact halo objects")
astrophysics astronomy dark-matter stars wimps
astrophysics astronomy dark-matter stars wimps
asked 4 hours ago
jormansandovaljormansandoval
918719
918719
$begingroup$
I'm pretty sure the "degenerated matter" of the black dwarf is still made of baryons, so it is not dark matter.
$endgroup$
– N. Steinle
4 hours ago
add a comment |
$begingroup$
I'm pretty sure the "degenerated matter" of the black dwarf is still made of baryons, so it is not dark matter.
$endgroup$
– N. Steinle
4 hours ago
$begingroup$
I'm pretty sure the "degenerated matter" of the black dwarf is still made of baryons, so it is not dark matter.
$endgroup$
– N. Steinle
4 hours ago
$begingroup$
I'm pretty sure the "degenerated matter" of the black dwarf is still made of baryons, so it is not dark matter.
$endgroup$
– N. Steinle
4 hours ago
add a comment |
1 Answer
1
active
oldest
votes
$begingroup$
Three reasons:
As you correctly point out, black dwarfs are "hypothetical objects". There has been insufficient time since the first stars were born for white dwarfs to cool below about 3000 K. i.e. Whilst there are faint white dwarfs with luminosities below a few $10^-5 L_odot$, they are not invisible.
Microlensing experiments rule out "massive compact halo objects", like cold white dwarfs or black holes as a significant contributor to dark matter.
Most of the dark matter needs to be non baryonic and to interact very weakly with normal matter in order to form the structures that we see today in the universe; and to reconcile the inferred primordial abundances of helium, deuterium and lithium with the total amount of matter deduced to be in galaxies and clusters of galaxies. Cold white dwarfs are baryonic, so cannot represent the bulk of dark matter.
$endgroup$
add a comment |
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1 Answer
1
active
oldest
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1 Answer
1
active
oldest
votes
active
oldest
votes
active
oldest
votes
$begingroup$
Three reasons:
As you correctly point out, black dwarfs are "hypothetical objects". There has been insufficient time since the first stars were born for white dwarfs to cool below about 3000 K. i.e. Whilst there are faint white dwarfs with luminosities below a few $10^-5 L_odot$, they are not invisible.
Microlensing experiments rule out "massive compact halo objects", like cold white dwarfs or black holes as a significant contributor to dark matter.
Most of the dark matter needs to be non baryonic and to interact very weakly with normal matter in order to form the structures that we see today in the universe; and to reconcile the inferred primordial abundances of helium, deuterium and lithium with the total amount of matter deduced to be in galaxies and clusters of galaxies. Cold white dwarfs are baryonic, so cannot represent the bulk of dark matter.
$endgroup$
add a comment |
$begingroup$
Three reasons:
As you correctly point out, black dwarfs are "hypothetical objects". There has been insufficient time since the first stars were born for white dwarfs to cool below about 3000 K. i.e. Whilst there are faint white dwarfs with luminosities below a few $10^-5 L_odot$, they are not invisible.
Microlensing experiments rule out "massive compact halo objects", like cold white dwarfs or black holes as a significant contributor to dark matter.
Most of the dark matter needs to be non baryonic and to interact very weakly with normal matter in order to form the structures that we see today in the universe; and to reconcile the inferred primordial abundances of helium, deuterium and lithium with the total amount of matter deduced to be in galaxies and clusters of galaxies. Cold white dwarfs are baryonic, so cannot represent the bulk of dark matter.
$endgroup$
add a comment |
$begingroup$
Three reasons:
As you correctly point out, black dwarfs are "hypothetical objects". There has been insufficient time since the first stars were born for white dwarfs to cool below about 3000 K. i.e. Whilst there are faint white dwarfs with luminosities below a few $10^-5 L_odot$, they are not invisible.
Microlensing experiments rule out "massive compact halo objects", like cold white dwarfs or black holes as a significant contributor to dark matter.
Most of the dark matter needs to be non baryonic and to interact very weakly with normal matter in order to form the structures that we see today in the universe; and to reconcile the inferred primordial abundances of helium, deuterium and lithium with the total amount of matter deduced to be in galaxies and clusters of galaxies. Cold white dwarfs are baryonic, so cannot represent the bulk of dark matter.
$endgroup$
Three reasons:
As you correctly point out, black dwarfs are "hypothetical objects". There has been insufficient time since the first stars were born for white dwarfs to cool below about 3000 K. i.e. Whilst there are faint white dwarfs with luminosities below a few $10^-5 L_odot$, they are not invisible.
Microlensing experiments rule out "massive compact halo objects", like cold white dwarfs or black holes as a significant contributor to dark matter.
Most of the dark matter needs to be non baryonic and to interact very weakly with normal matter in order to form the structures that we see today in the universe; and to reconcile the inferred primordial abundances of helium, deuterium and lithium with the total amount of matter deduced to be in galaxies and clusters of galaxies. Cold white dwarfs are baryonic, so cannot represent the bulk of dark matter.
answered 4 hours ago
Rob JeffriesRob Jeffries
70.3k7142243
70.3k7142243
add a comment |
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I'm pretty sure the "degenerated matter" of the black dwarf is still made of baryons, so it is not dark matter.
$endgroup$
– N. Steinle
4 hours ago