Knowledge (XXG)

Fuzzy cold dark matter

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Mocz, Philip; Fialkov, Anastasia; Vogelsberger, Mark; Becerra, Fernando; Amin, Mustafa A.; Bose, Sownak; Boylan-Kolchin, Michael; Chavanis, Pierre-Henri; Hernquist, Lars; Lancaster, Lachlan; Marinacci, Federico; Robles, Victor H.; Zavala, JesĂşs (2019). "First Star-Forming Structures in Fuzzy Cosmic
65: 539: 482: 75:. Fuzzy cold dark matter halos in dwarf galaxies would manifest wave behavior on astrophysical scales, and the cusps would be avoided through the 101:
New research (2023) has uncovered evidence that fuzzy dark matter, specifically ultralight axions, may better fit gravitational lens data than
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Bohua Li; Tanja Rindler-Daller; Paul R. Shapiro (2014). "Cosmological Constraints on Bose-Einstein-Condensed Scalar Field Dark Matter".
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Schive, Hsi-Yu; Chiueh, Tzihong; Broadhurst, Tom (2014). "Cosmic structure as the quantum interference of a coherent dark wave".
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Hu, Wayne; Barkana, Rennan; Gruzinov, Andrei (2000). "Cold and Fuzzy Dark Matter".
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centers, and cylindrical soliton-like cores in dark matter cosmic web filaments.
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Lee, Jae-Weon (2018). "Brief History of Ultra-light Scalar Dark Matter Models".
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Hypothetical form of cold dark matter proposed to solve the cuspy halo problem
275: 283: 160: 135: 413:"No WIMPS! Heavy particles don't explain gravitational lensing oddities" 80: 213: 372: 250: 319: 196: 79:. The wave behavior leads to interference patterns, spherical 513: 456: 40: 59: 94:without self-interaction. It is governed by the 533: 476: 8: 540: 526: 483: 469: 371: 318: 249: 195: 134: 48: 39: 113: 30:. It would consist of extremely light 90:Fuzzy cold dark matter is a limit of 7: 494: 492: 437: 435: 512:. You can help Knowledge (XXG) by 455:. You can help Knowledge (XXG) by 14: 496: 439: 77:Heisenberg uncertainty principle 60:{\displaystyle \approx 10^{-22}} 268:10.1103/PhysRevLett.123.141301 1: 390:10.1051/epjconf/201816806005 96:Schrödinger–Poisson equation 34:with masses on the order of 411:Timmer, John (2023-04-21). 153:10.1103/PhysRevLett.85.1158 590: 491: 434: 337:10.1103/PhysRevD.89.083536 22:is a hypothetical form of 574:Physical cosmology stubs 92:scalar field dark matter 238:Physical Review Letters 123:Physical Review Letters 569:Particle physics stubs 508:-related article is a 451:–related article is a 360:EPJ Web of Conferences 61: 26:proposed to solve the 20:Fuzzy cold dark matter 62: 564:Hypothetical objects 38: 382:2018EPJWC.16806005L 329:2014PhRvD..89h3536L 260:2019PhRvL.123n1301M 206:2014NatPh..10..496S 145:2000PhRvL..85.1158H 506:physical cosmology 71:on the order of 1 69:Compton wavelength 57: 28:cuspy halo problem 521: 520: 464: 463: 214:10.1038/nphys2996 581: 542: 535: 528: 500: 493: 485: 478: 471: 449:particle physics 443: 436: 427: 426: 424: 423: 408: 402: 401: 375: 355: 349: 348: 322: 302: 296: 295: 253: 232: 226: 225: 199: 179: 173: 172: 138: 136:astro-ph/0003365 118: 85:dark matter halo 66: 64: 63: 58: 56: 55: 32:scalar particles 24:cold dark matter 589: 588: 584: 583: 582: 580: 579: 578: 549: 548: 547: 546: 490: 489: 432: 430: 421: 419: 410: 409: 405: 357: 356: 352: 304: 303: 299: 234: 233: 229: 181: 180: 176: 120: 119: 115: 111: 44: 36: 35: 17: 12: 11: 5: 587: 585: 577: 576: 571: 566: 561: 551: 550: 545: 544: 537: 530: 522: 519: 518: 501: 488: 487: 480: 473: 465: 462: 461: 444: 429: 428: 403: 350: 297: 244:(14): 141301. 227: 190:(7): 496–499. 184:Nature Physics 174: 129:(6): 1158–61. 112: 110: 107: 54: 51: 47: 43: 15: 13: 10: 9: 6: 4: 3: 2: 586: 575: 572: 570: 567: 565: 562: 560: 557: 556: 554: 543: 538: 536: 531: 529: 524: 523: 517: 515: 511: 507: 502: 499: 495: 486: 481: 479: 474: 472: 467: 466: 460: 458: 454: 450: 445: 442: 438: 433: 418: 414: 407: 404: 399: 395: 391: 387: 383: 379: 374: 369: 365: 361: 354: 351: 346: 342: 338: 334: 330: 326: 321: 316: 313:(8): 083536. 312: 308: 301: 298: 293: 289: 285: 281: 277: 273: 269: 265: 261: 257: 252: 247: 243: 239: 231: 228: 223: 219: 215: 211: 207: 203: 198: 193: 189: 185: 178: 175: 170: 166: 162: 158: 154: 150: 146: 142: 137: 132: 128: 124: 117: 114: 108: 106: 105:dark matter. 104: 99: 97: 93: 88: 86: 82: 78: 74: 70: 52: 49: 45: 41: 33: 29: 25: 21: 514:expanding it 503: 457:expanding it 446: 431: 420:. Retrieved 417:Ars Technica 416: 406: 363: 359: 353: 310: 307:Phys. Rev. D 306: 300: 241: 237: 236:Filaments". 230: 187: 183: 177: 126: 122: 116: 100: 89: 19: 18: 559:Dark matter 553:Categories 422:2023-06-08 373:1704.05057 251:1910.01653 73:light year 366:: 06005. 345:118654592 320:1310.6061 292:203734641 276:0031-9007 222:118725080 197:1406.6586 169:118938504 83:cores in 67:eV; so a 50:− 42:≈ 398:54649264 284:31702225 161:10991501 378:Bibcode 325:Bibcode 256:Bibcode 202:Bibcode 141:Bibcode 81:soliton 396:  343:  290:  282:  274:  220:  167:  159:  504:This 447:This 394:S2CID 368:arXiv 341:S2CID 315:arXiv 288:S2CID 246:arXiv 218:S2CID 192:arXiv 165:S2CID 131:arXiv 109:Notes 510:stub 453:stub 280:PMID 272:ISSN 157:PMID 103:WIMP 386:doi 364:168 333:doi 264:doi 242:123 210:doi 149:doi 555:: 415:. 392:. 384:. 376:. 362:. 339:. 331:. 323:. 311:89 309:. 286:. 278:. 270:. 262:. 254:. 240:. 216:. 208:. 200:. 188:10 186:. 163:. 155:. 147:. 139:. 127:85 125:. 98:. 53:22 46:10 541:e 534:t 527:v 516:. 484:e 477:t 470:v 459:. 425:. 400:. 388:: 380:: 370:: 347:. 335:: 327:: 317:: 294:. 266:: 258:: 248:: 224:. 212:: 204:: 194:: 171:. 151:: 143:: 133::

Index

cold dark matter
cuspy halo problem
scalar particles
Compton wavelength
light year
Heisenberg uncertainty principle
soliton
dark matter halo
scalar field dark matter
Schrödinger–Poisson equation
WIMP
arXiv
astro-ph/0003365
Bibcode
2000PhRvL..85.1158H
doi
10.1103/PhysRevLett.85.1158
PMID
10991501
S2CID
118938504
arXiv
1406.6586
Bibcode
2014NatPh..10..496S
doi
10.1038/nphys2996
S2CID
118725080
arXiv

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