Coupled dark energy and dark matter from dilatation anomaly
Cosmological runaway solutions may exhibit an exact dilatation symmetry in the asymptotic limit of infinite time. In this limit, the massless dilaton or cosmon could be accompanied by another massless scalar field - the bolon. At finite time, small time-dependent masses for both the cosmon and the b...
Gespeichert in:
| Hauptverfasser: | , , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2011
|
| In: |
Physical review. D, Particles, fields, gravitation, and cosmology
Year: 2011, Jahrgang: 84, Heft: 2, Pages: 1-6 |
| ISSN: | 1550-2368 |
| Online-Zugang: | Verlag, Volltext: http://prd.aps.org/abstract/PRD/v84/i2/e023010 Verlag, Volltext: http://link.aps.org/doi/10.1103/PhysRevD.84.023010 
|
| Verfasserangaben: | J. Beyer; S. Nurmi; C. Wetterich |
MARC
| LEADER | 00000caa a22000002c 4500 | ||
|---|---|---|---|
| 001 | 1470879433 | ||
| 003 | DE-627 | ||
| 005 | 20241205154730.0 | ||
| 007 | cr uuu---uuuuu | ||
| 008 | 140210s2011 xx |||||o 00| ||eng c | ||
| 024 | 7 | |a 10.1103/PhysRevD.84.023010 |2 doi | |
| 035 | |a (DE-627)1470879433 | ||
| 035 | |a (DE-576)400879433 | ||
| 035 | |a (DE-599)BSZ400879433 | ||
| 035 | |a (OCoLC)1389793524 | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rakwb | ||
| 041 | |a eng | ||
| 084 | |a 29 |2 sdnb | ||
| 100 | 1 | |a Beyer, Joschka |0 (DE-588)104730841X |0 (DE-627)778093964 |0 (DE-576)33972191X |4 aut | |
| 245 | 1 | 0 | |a Coupled dark energy and dark matter from dilatation anomaly |c J. Beyer; S. Nurmi; C. Wetterich |
| 264 | 1 | |c 2011 | |
| 300 | |a 6 | ||
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a Computermedien |b c |2 rdamedia | ||
| 338 | |a Online-Ressource |b cr |2 rdacarrier | ||
| 500 | |a Gesehen am 10.02.2014 | ||
| 520 | |a Cosmological runaway solutions may exhibit an exact dilatation symmetry in the asymptotic limit of infinite time. In this limit, the massless dilaton or cosmon could be accompanied by another massless scalar field - the bolon. At finite time, small time-dependent masses for both the cosmon and the bolon are still present due to imperfect dilatation symmetry. For a sufficiently large mass, the bolon will start oscillating and play the role of dark matter, while the cosmon is responsible for dark energy. The common origin of the mass of both fields leads to an effective interaction between dark matter and dark energy. Realistic cosmologies are possible for a simple form of the effective cosmon-bolon potential. We find an inverse bolon mass of a size where it could reduce subgalactic structure formation | ||
| 700 | 1 | |a Nurmi, Sami |0 (DE-588)1047309122 |0 (DE-627)778094960 |0 (DE-576)400879204 |4 aut | |
| 700 | 1 | |a Wetterich, Christof |d 1952- |0 (DE-588)109400070 |0 (DE-627)683447629 |0 (DE-576)356552608 |4 aut | |
| 773 | 0 | 8 | |i In |t Physical review. D, Particles, fields, gravitation, and cosmology |d [Erscheinungsort nicht ermittelbar] : Soc., 1970 |g 84(2011), 2, Artikel-ID 023010, Seite 1-6 |h Online-Ressource |w (DE-627)253787017 |w (DE-600)1461167-3 |w (DE-576)07279531X |x 1550-2368 |7 nnas |a Coupled dark energy and dark matter from dilatation anomaly |
| 773 | 1 | 8 | |g volume:84 |g year:2011 |g number:2 |g elocationid:023010 |g pages:1-6 |g extent:6 |a Coupled dark energy and dark matter from dilatation anomaly |
| 856 | 4 | 0 | |u http://prd.aps.org/abstract/PRD/v84/i2/e023010 |x Verlag |3 Volltext |
| 856 | 4 | 0 | |u http://link.aps.org/doi/10.1103/PhysRevD.84.023010 |x Verlag |3 Volltext |
| 951 | |a AR | ||
| 992 | |a 20140210 | ||
| 993 | |a Article | ||
| 994 | |a 2011 | ||
| 998 | |g 109400070 |a Wetterich, Christof |m 109400070:Wetterich, Christof |d 130000 |d 130300 |e 130000PW109400070 |e 130300PW109400070 |k 0/130000/ |k 1/130000/130300/ |p 3 |y j | ||
| 998 | |g 1047309122 |a Nurmi, Sami |m 1047309122:Nurmi, Sami |p 2 | ||
| 998 | |g 104730841X |a Beyer, Joschka |m 104730841X:Beyer, Joschka |p 1 |x j | ||
| 999 | |a KXP-PPN1470879433 |e 2782722832 | ||
| BIB | |a Y | ||
| SER | |a journal | ||
| JSO | |a {"title":[{"title":"Coupled dark energy and dark matter from dilatation anomaly","title_sort":"Coupled dark energy and dark matter from dilatation anomaly"}],"person":[{"role":"aut","display":"Beyer, Joschka","given":"Joschka","family":"Beyer"},{"display":"Nurmi, Sami","role":"aut","family":"Nurmi","given":"Sami"},{"given":"Christof","family":"Wetterich","role":"aut","display":"Wetterich, Christof"}],"type":{"media":"Online-Ressource","bibl":"article-journal"},"note":["Gesehen am 10.02.2014"],"language":["eng"],"recId":"1470879433","origin":[{"dateIssuedKey":"2011","dateIssuedDisp":"2011"}],"id":{"doi":["10.1103/PhysRevD.84.023010"],"eki":["1470879433"]},"name":{"displayForm":["J. Beyer; S. Nurmi; C. Wetterich"]},"physDesc":[{"extent":"6 S."}],"relHost":[{"pubHistory":["3.Ser. 1.1970 - 92.2015"],"part":{"year":"2011","pages":"1-6","issue":"2","text":"84(2011), 2, Artikel-ID 023010, Seite 1-6","volume":"84","extent":"6"},"titleAlt":[{"title":"Physical review / D"},{"title":"D online"}],"disp":"Coupled dark energy and dark matter from dilatation anomalyPhysical review. D, Particles, fields, gravitation, and cosmology","type":{"media":"Online-Ressource","bibl":"periodical"},"note":["ISSN-Portal 1089-4918: Particles and fields","Gesehen am 22. Januar 2016"],"language":["eng"],"corporate":[{"display":"American Institute of Physics","roleDisplay":"Herausgebendes Organ","role":"isb"},{"role":"isb","roleDisplay":"Herausgebendes Organ","display":"American Physical Society"}],"recId":"253787017","title":[{"partname":"Particles, fields, gravitation, and cosmology","title_sort":"Physical review","title":"Physical review"}],"physDesc":[{"extent":"Online-Ressource"}],"origin":[{"dateIssuedDisp":"1970-2015","dateIssuedKey":"1970","publisher":"Soc.","publisherPlace":"[Erscheinungsort nicht ermittelbar]"}],"id":{"zdb":["1461167-3"],"eki":["253787017"],"issn":["1550-2368","1089-4918"]},"name":{"displayForm":["publ. by the American Physical Society through the American Institute of Physics"]}}]} | ||
| SRT | |a BEYERJOSCHCOUPLEDDAR2011 | ||