black dwarf stars and dark matterHow 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?

How is it possible for user's password to be changed after storage was encrypted? (on OS X, Android)

Are white and non-white police officers equally likely to kill black suspects?

Accidentally leaked the solution to an assignment, what to do now? (I'm the prof)

What is the offset in a seaplane's hull?

Is it tax fraud for an individual to declare non-taxable revenue as taxable income? (US tax laws)

How to make payment on the internet without leaving a money trail?

How can I fix this gap between bookcases I made?

Why are 150k or 200k jobs considered good when there are 300k+ births a month?

Why doesn't Newton's third law mean a person bounces back to where they started when they hit the ground?

How can bays and straits be determined in a procedurally generated map?

I’m planning on buying a laser printer but concerned about the life cycle of toner in the machine

DOS, create pipe for stdin/stdout of command.com(or 4dos.com) in C or Batch?

Is there a minimum number of transactions in a block?

My colleague's body is amazing

Copycat chess is back

Can a German sentence have two subjects?

Patience, young "Padovan"

Why is "Reports" in sentence down without "The"

least quadratic residue under GRH: an EXPLICIT bound

Why CLRS example on residual networks does not follows its formula?

What defenses are there against being summoned by the Gate spell?

XeLaTeX and pdfLaTeX ignore hyphenation

Why has Russell's definition of numbers using equivalence classes been finally abandoned? ( If it has actually been abandoned).

declaring a variable twice in IIFE



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?













2












$begingroup$


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")










share|cite|improve this question









$endgroup$











  • $begingroup$
    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
    5 hours ago










  • $begingroup$
    Dark baryonic matter is baryonic matter that doesn't emit sufficient light to be detected.
    $endgroup$
    – Cinaed Simson
    33 mins ago















2












$begingroup$


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")










share|cite|improve this question









$endgroup$











  • $begingroup$
    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
    5 hours ago










  • $begingroup$
    Dark baryonic matter is baryonic matter that doesn't emit sufficient light to be detected.
    $endgroup$
    – Cinaed Simson
    33 mins ago













2












2








2





$begingroup$


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")










share|cite|improve this question









$endgroup$




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






share|cite|improve this question













share|cite|improve this question











share|cite|improve this question




share|cite|improve this question










asked 5 hours ago









jormansandovaljormansandoval

923719




923719











  • $begingroup$
    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
    5 hours ago










  • $begingroup$
    Dark baryonic matter is baryonic matter that doesn't emit sufficient light to be detected.
    $endgroup$
    – Cinaed Simson
    33 mins 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
    5 hours ago










  • $begingroup$
    Dark baryonic matter is baryonic matter that doesn't emit sufficient light to be detected.
    $endgroup$
    – Cinaed Simson
    33 mins 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
5 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
5 hours ago












$begingroup$
Dark baryonic matter is baryonic matter that doesn't emit sufficient light to be detected.
$endgroup$
– Cinaed Simson
33 mins ago




$begingroup$
Dark baryonic matter is baryonic matter that doesn't emit sufficient light to be detected.
$endgroup$
– Cinaed Simson
33 mins ago










1 Answer
1






active

oldest

votes


















2












$begingroup$

Three reasons:



  1. 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.


  2. Microlensing experiments rule out "massive compact halo objects", like cold white dwarfs or black holes as a significant contributor to dark matter.


  3. 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.






share|cite|improve this answer









$endgroup$












  • $begingroup$
    Most of the dark matter needs to be non baryonic in the Big Bang model since the galaxies wouldn't have formed. If one needs to invoke "magic" to get a cosmological model to form galaxies, then model is probably broken.
    $endgroup$
    – Cinaed Simson
    31 mins ago












Your Answer





StackExchange.ifUsing("editor", function ()
return StackExchange.using("mathjaxEditing", function ()
StackExchange.MarkdownEditor.creationCallbacks.add(function (editor, postfix)
StackExchange.mathjaxEditing.prepareWmdForMathJax(editor, postfix, [["$", "$"], ["\\(","\\)"]]);
);
);
, "mathjax-editing");

StackExchange.ready(function()
var channelOptions =
tags: "".split(" "),
id: "151"
;
initTagRenderer("".split(" "), "".split(" "), channelOptions);

StackExchange.using("externalEditor", function()
// Have to fire editor after snippets, if snippets enabled
if (StackExchange.settings.snippets.snippetsEnabled)
StackExchange.using("snippets", function()
createEditor();
);

else
createEditor();

);

function createEditor()
StackExchange.prepareEditor(
heartbeatType: 'answer',
autoActivateHeartbeat: false,
convertImagesToLinks: false,
noModals: true,
showLowRepImageUploadWarning: true,
reputationToPostImages: null,
bindNavPrevention: true,
postfix: "",
imageUploader:
brandingHtml: "Powered by u003ca class="icon-imgur-white" href="https://imgur.com/"u003eu003c/au003e",
contentPolicyHtml: "User contributions licensed under u003ca href="https://creativecommons.org/licenses/by-sa/3.0/"u003ecc by-sa 3.0 with attribution requiredu003c/au003e u003ca href="https://stackoverflow.com/legal/content-policy"u003e(content policy)u003c/au003e",
allowUrls: true
,
noCode: true, onDemand: true,
discardSelector: ".discard-answer"
,immediatelyShowMarkdownHelp:true
);



);













draft saved

draft discarded


















StackExchange.ready(
function ()
StackExchange.openid.initPostLogin('.new-post-login', 'https%3a%2f%2fphysics.stackexchange.com%2fquestions%2f471183%2fblack-dwarf-stars-and-dark-matter%23new-answer', 'question_page');

);

Post as a guest















Required, but never shown

























1 Answer
1






active

oldest

votes








1 Answer
1






active

oldest

votes









active

oldest

votes






active

oldest

votes









2












$begingroup$

Three reasons:



  1. 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.


  2. Microlensing experiments rule out "massive compact halo objects", like cold white dwarfs or black holes as a significant contributor to dark matter.


  3. 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.






share|cite|improve this answer









$endgroup$












  • $begingroup$
    Most of the dark matter needs to be non baryonic in the Big Bang model since the galaxies wouldn't have formed. If one needs to invoke "magic" to get a cosmological model to form galaxies, then model is probably broken.
    $endgroup$
    – Cinaed Simson
    31 mins ago
















2












$begingroup$

Three reasons:



  1. 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.


  2. Microlensing experiments rule out "massive compact halo objects", like cold white dwarfs or black holes as a significant contributor to dark matter.


  3. 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.






share|cite|improve this answer









$endgroup$












  • $begingroup$
    Most of the dark matter needs to be non baryonic in the Big Bang model since the galaxies wouldn't have formed. If one needs to invoke "magic" to get a cosmological model to form galaxies, then model is probably broken.
    $endgroup$
    – Cinaed Simson
    31 mins ago














2












2








2





$begingroup$

Three reasons:



  1. 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.


  2. Microlensing experiments rule out "massive compact halo objects", like cold white dwarfs or black holes as a significant contributor to dark matter.


  3. 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.






share|cite|improve this answer









$endgroup$



Three reasons:



  1. 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.


  2. Microlensing experiments rule out "massive compact halo objects", like cold white dwarfs or black holes as a significant contributor to dark matter.


  3. 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.







share|cite|improve this answer












share|cite|improve this answer



share|cite|improve this answer










answered 5 hours ago









Rob JeffriesRob Jeffries

70.3k7142243




70.3k7142243











  • $begingroup$
    Most of the dark matter needs to be non baryonic in the Big Bang model since the galaxies wouldn't have formed. If one needs to invoke "magic" to get a cosmological model to form galaxies, then model is probably broken.
    $endgroup$
    – Cinaed Simson
    31 mins ago

















  • $begingroup$
    Most of the dark matter needs to be non baryonic in the Big Bang model since the galaxies wouldn't have formed. If one needs to invoke "magic" to get a cosmological model to form galaxies, then model is probably broken.
    $endgroup$
    – Cinaed Simson
    31 mins ago
















$begingroup$
Most of the dark matter needs to be non baryonic in the Big Bang model since the galaxies wouldn't have formed. If one needs to invoke "magic" to get a cosmological model to form galaxies, then model is probably broken.
$endgroup$
– Cinaed Simson
31 mins ago





$begingroup$
Most of the dark matter needs to be non baryonic in the Big Bang model since the galaxies wouldn't have formed. If one needs to invoke "magic" to get a cosmological model to form galaxies, then model is probably broken.
$endgroup$
– Cinaed Simson
31 mins ago


















draft saved

draft discarded
















































Thanks for contributing an answer to Physics Stack Exchange!


  • Please be sure to answer the question. Provide details and share your research!

But avoid


  • Asking for help, clarification, or responding to other answers.

  • Making statements based on opinion; back them up with references or personal experience.

Use MathJax to format equations. MathJax reference.


To learn more, see our tips on writing great answers.




draft saved


draft discarded














StackExchange.ready(
function ()
StackExchange.openid.initPostLogin('.new-post-login', 'https%3a%2f%2fphysics.stackexchange.com%2fquestions%2f471183%2fblack-dwarf-stars-and-dark-matter%23new-answer', 'question_page');

);

Post as a guest















Required, but never shown





















































Required, but never shown














Required, but never shown












Required, but never shown







Required, but never shown

































Required, but never shown














Required, but never shown












Required, but never shown







Required, but never shown







Popular posts from this blog

How to create a command for the “strange m” symbol in latex? Announcing the arrival of Valued Associate #679: Cesar Manara Planned maintenance scheduled April 23, 2019 at 23:30 UTC (7:30pm US/Eastern)How do you make your own symbol when Detexify fails?Writing bold small caps with mathpazo packageplus-minus symbol with parenthesis around the minus signGreek character in Beamer document titleHow to create dashed right arrow over symbol?Currency symbol: Turkish LiraDouble prec as a single symbol?Plus Sign Too Big; How to Call adfbullet?Is there a TeX macro for three-legged pi?How do I get my integral-like symbol to align like the integral?How to selectively substitute a letter with another symbol representing the same letterHow do I generate a less than symbol and vertical bar that are the same height?

Българска екзархия Съдържание История | Български екзарси | Вижте също | Външни препратки | Литература | Бележки | НавигацияУстав за управлението на българската екзархия. Цариград, 1870Слово на Ловешкия митрополит Иларион при откриването на Българския народен събор в Цариград на 23. II. 1870 г.Българската правда и гръцката кривда. От С. М. (= Софийски Мелетий). Цариград, 1872Предстоятели на Българската екзархияПодмененият ВеликденИнформационна агенция „Фокус“Димитър Ризов. Българите в техните исторически, етнографически и политически граници (Атлас съдържащ 40 карти). Berlin, Königliche Hoflithographie, Hof-Buch- und -Steindruckerei Wilhelm Greve, 1917Report of the International Commission to Inquire into the Causes and Conduct of the Balkan Wars

Чепеларе Съдържание География | История | Население | Спортни и природни забележителности | Културни и исторически обекти | Религии | Обществени институции | Известни личности | Редовни събития | Галерия | Източници | Литература | Външни препратки | Навигация41°43′23.99″ с. ш. 24°41′09.99″ и. д. / 41.723333° с. ш. 24.686111° и. д.*ЧепелареЧепеларски Linux fest 2002Начало на Зимен сезон 2005/06Национални хайдушки празници „Капитан Петко Войвода“Град ЧепелареЧепеларе – народният ски курортbgrod.orgwww.terranatura.hit.bgСправка за населението на гр. Исперих, общ. Исперих, обл. РазградМузей на родопския карстМузей на спорта и скитеЧепеларебългарскибългарскианглийскитукИстория на градаСки писти в ЧепелареВремето в ЧепелареРадио и телевизия в ЧепелареЧепеларе мами с родопски чар и добри пистиЕвтин туризъм и снежни атракции в ЧепелареМестоположениеИнформация и снимки от музея на родопския карст3D панорами от ЧепелареЧепелареррр