Scikid

Hello Scikid! Welcome to Wikipedia! Thank you for your contributions. Its very important that you browse through the links below so as to become familier with how Wikipedia works. If you need help you ask me on my talk page, or place {{helpme}} on your talk page and another Wikipedian will show up shortly. Please remember to sign your name on talk pages by clicking or by typing four tildes "~~~~"; this will automatically produce your name and the date. If you are already loving Wikipedia and plan on becoming a Wikipedian you might consider being "adopted" by a more experienced editor, just paste {{Adoptme}} into your userpage and wait a few hours! Finally, please do your best to always fill in the edit summary field. Happy editing! frummer 07:12, 27 December 2006 (UTC) Getting Started Wikipedia Tutorial • The five pillars of Wikipedia How to: edit a page • upload an image Getting Help Frequently Asked Questions Where to ask questions or make comments Request administrator attention Policies and Guidelines Neutral point of view • Reliable sources Verifiability • Citing sources • No original research What Wikipedia is not • Biographies of living persons Manual of Style • Three-revert rule • Sock puppetry Copyrights • Fair use • Image use policy External links • Spam • Vandalism Deletion policy • Conflict of interest • Notability The Community Build consensus • Resolving disputes Assume good faith • Civility • Etiquette No personal attacks • No legal threats Community Portal • Village pump Signpost • IRC channels • Mailing lists Things to do Be bold in editing • Help develop an article Pages needing attention • Peer review Join a WikiProject • Translating articles Cleaning up: General • Spam • Vandalism Miscellaneous Categories • Disambiguity • Stubs User pages • Talk pages Useful templates • Tools • User scripts

Dark matter edits

Please note that the edits you have made to dark matter articles violate WP:WEIGHT and therefore must be removed until the idea receives more notability within the scientific community. ScienceApologist (talk) 21:06, 11 January 2008 (UTC)

BEC or Scalar field dark matter model (SFDM) of halos is not an extrem minority theory.

BEC or Scalar field dark matter model (SFDM) of halos is not an extrem minority theory. Actually, this model is a main alternative to standard cold dark matter model and the most successful model in explaing the rotation curves. This model is famous in the physics and cosmology community. It has many different names such as fuzzy, fluid, repulsive, scalar field, boson halo and so on.(Please see a review article in Science [1].)This model solves many problems of cold dark model (CDM) such as cuspy halo and missing satellite. There are already hundres of journal papers published about this idea and also many works saying the model predicts the observed rotation curves of galaxies and dwarf galaxies very well.(Please see review [2] page 21 and [3,4,5]) No other dark matter model have succeeded at this level in explaining the curves. Note that SFDM also behaves as CDM at the scale larger than galaxy, so it also explain large scale strures as much as CDM. Thus, I think, for balance, this model deserve space at least as much as the modified gravity theories which seems to be even not accepted by majority of physics community currently. As far as I understand, the philosophy of wikipedia is that users themselves make contents and the others review and edit the contents. Many experts in this field is already reading and editing this subject.(I am one of them) So, if my statements are wrong, missing something, or the model is an extremly minority which does not deserve publication, they will soon edit it. So please let the experts do it. [1] "New Light on Dark Matter" Jeremiah P. Ostriker and Paul Steinhardt Science 20 June 2003: Vol. 300. no. 5627, pp. 1909 - 1913 [2] "TOPICAL REVIEW: General relativistic boson stars" Franz E Schunck and Eckehard W Mielke arXiv:0801.0307v1 [astro-ph] [3] "Is dark matter a BEC or scalar field?"Jae-Weon Lee arXiv:0801.1442v1 [astro-ph] [4] "Mini-review on Scalar Field Dark Matter" L. Arturo Ure˜na–L´opez [5] "Scalar Field Dark Matter: head-on interaction between two structures" Phys.Rev. D74 (2006) 103002

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