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Talk:Alcubierre drive/Archive 1

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416:. In fact, the ADM form of the metric guarantees that Alcubierre style warp drive spacetimes do not admit any closed timelike curves, if that is what you had in mind. Hint: construct a simplified two-dimensional warp drive using a compact bump function with metric in ADM form as in the Alcubierre spacetimes. Draw some light cones. Study the nature of the timelike geodesics. You will see that in fact the ADM form guarantees that they cannot turn around in time. --- 433: 31: 152:(no mass-energy other than the field energy of an electromagnetic field) must have Einstein tensors which agree with matter tensors having the form appropriate for an electromagnetic field (as described in Maxwell's theory). Furthermore, their definition must include specifying an antisymmetric second order tensor field 274:. Can you read that (and hopefully the CQG papers I cited) before making any drastic changes in the article? Again, because of the edit conflict problem with current Wikiware, let's try to settle this on the talk page, since neither of us want to lose a lot of work if an edit conflict messes up the article itself! 252:
Also I disagree about the statement on falsibility. Mathematically the EFF *is* unfalsibility because it is consistent. The physical question is whether or not EFF matches observations. To illustrate the point I'm making, you can't argue on mathematical grounds that Newtonian physics is incorrect.
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I think the present version fairly describes the currently dubious status of warp bubbles in the research literature, but could add much more detail in support of my comments regarding the apparently "unphysical" energy flux near an Alcubierre bubble, and their suspiciously "spontaneous" appearance
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Hi, Roadrunner, we might have an edit conflict since I was actually modifying the page just now, not knowing that you were also doing so. Did you know that the new Wiki software has a problem? I didn't want to lose my work and couldn't see what you did, so maybe we should avoid making drastic
190:(according to Maxwell's theory, and following some general principles for getting from a field equation to the corresponding contribution to the matter tensor), and of course this stress-energy tensor must match the Einstein tensor computed directly from the Riemann tensor. 221:
Einstein himself had a rather stringent notion of 'solution' in mind, similar to what I described above in the special case of 'electrovacuum'. Others with a more speculative turn of mind have proposed to allow matter tensors which merely satisfy one or more of a list of
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are easy to recognize, since the matter tensor vanishes identically in a vacuum region, so vacuum solutions have purely a mathematical characterization: they are Lorentzian manifolds whose Einstein tensor vanishes (equivalently, whose Ricci tensor vanishes).
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Lorentzian spacetime is a 'solution' of the EFE! If we allowed this, gtr would be unfalsifiable-- hence useless! Of course, it is not useless, because in fact physicists have stringent expectations about what can stand as a legal matter tensor.
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Put in other words: in principle, we could take any Lorentzian spacetime, compute its Einstein tensor, and declare this to be the 'matter tensor' of some funky field. But this would be an absurd procedure, since it would imply that
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which may (or may not) characterize some properties shared by all (or some) known matter tensors which everyone would agree are acceptable, such as electromagnetic field energy/momentum/stress, or a perfect fluid.
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I added a bit more about the interpretation of the warp bubble and pointed out a significant difference between the Alcubierre and Notario warp drives. I still think the existing article on
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OK, I rewrote the article and added citations to the series of CQG papers. A bibliographic note: according to Broeck, the proper way to parse his name is Broeck, Chris Van Den. ---
209:) there is no well-defined classical field theory which gives contributions to the matter tensor which could match the Einstein tensor of a nontrivial Alcubierre spacetime. 389:. If so, I think you missed my point. If we allowed any symmetric second rank tensor field on any Lorentzian spacetime to be a "solution" to the EFE, we would have no 412:
Hi, 63.201.230.31 from SBC, the statement you added is meaningless as stated, and the page you cited certainly doesn't imply anything about time travel in the sense of
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should be deleted, since I think this one adequately describes the concept. However, there might be some reason for a similar article on
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I have extensively discussed elsewhere the question of what it means to be a "solution" of the EFE. See for example the article on
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I've been looking everywhere for my "statement on falsifiability" and can't find it. Unless you mean what I said about "divide
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and disappearance. If anyone is greatly interested in seeing that, say so here and I'll add it to my list---
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Neutralized the wording a bit. Mathematically the Alcubierre metric is a solution of the
119: 423: 306:, since these spacetimes are significantly different from the Alcubierre warp drives. 230:
Accordingly, I propose to rewrite this article to correct the mistaken impression. ---
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and declare the result to be the stress-energy of the spacetime" in the article on
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changes for a few days to the article and discuss our difference of opinion here.
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If you wish to start a new discussion or revive an old one, please do so on the
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If you wish to start a new discussion or revive an old one, please do so on the
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However it is incorrect, because the predictions don't match observerations.
197:, and there are other types of solutions which arise from the notion of a 193:
There are other kinds of classical fields which one can propose besides
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Every Lorentzian manifold has, mathematically speaking, a well-defined
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of the EFE, this must agree (up to a certain constant factor) with a
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observation whatever could be declared to "agree with theory". ---
182:, and this must not only satisfy (a curved spacetime version of) 205:, but AFAIK (and few years ago I read the ENTIRE literature on 100:
This article is seriously misleading in one important respect.
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The Alcubierre spacetimes are a certain family of Lorentzian
368: 338: 158: 86:Note that this page is the archive from the merged 377: 354: 174: 387:exact solutions of Einstein's field equations 96:Criticism of May 2005 Version of this Article 8: 367: 343: 337: 163: 157: 288:Notes on Revised Version of This Article 446:Do not edit the contents of this page. 44:Do not edit the contents of this page. 272:exact solutions in general relativity 7: 24: 122:, which you can compute from its 431: 393:whatever! That would mean that 29: 137:. Consider two easy examples: 408:Time travel? Not neccessarily 1: 424:00:01, 12 October 2005 (UTC) 497: 195:classical electromagnetism 404:1 July 2005 06:36 (UTC) 317:1 July 2005 04:37 (UTC) 284:1 July 2005 05:39 (UTC) 262:1 July 2005 04:54 (UTC) 241:Einstein field equations 124:Riemann curvature tensor 150:electrovacuum solutions 113:Einstein field equation 414:closed timelike curves 379: 356: 355:{\displaystyle G^{ab}} 176: 175:{\displaystyle F_{ab}} 444:of past discussions. 380: 378:{\displaystyle 8\pi } 357: 203:cosmological constant 177: 132:physically reasonable 42:of past discussions. 18:Talk:Alcubierre drive 366: 336: 188:stress-energy tensor 156: 321:Is GTR Falsifiable? 304:Notario warp drives 186:but must rise to a 184:Maxwell's equations 107:, but they are not 375: 352: 201:or from a nonzero 172: 484: 483: 456: 455: 450:current talk page 224:energy conditions 88:Alcubierre metric 82: 81: 54: 53: 48:current talk page 488: 465: 458: 457: 435: 434: 428: 384: 382: 381: 376: 361: 359: 358: 353: 351: 350: 300:Alcubierre drive 181: 179: 178: 173: 171: 170: 142:vacuum solutions 63: 56: 55: 33: 32: 26: 496: 495: 491: 490: 489: 487: 486: 485: 461: 432: 410: 364: 363: 339: 334: 333: 327:User:Roadrunner 323: 290: 159: 154: 153: 120:Einstein tensor 98: 59: 30: 22: 21: 20: 12: 11: 5: 494: 492: 482: 481: 476: 471: 466: 454: 453: 436: 409: 406: 374: 371: 349: 346: 342: 322: 319: 289: 286: 265: 257: 256: 255: 254: 247: 246: 245: 244: 169: 166: 162: 97: 94: 93: 92: 80: 79: 74: 69: 64: 52: 51: 34: 23: 15: 14: 13: 10: 9: 6: 4: 3: 2: 493: 480: 477: 475: 472: 470: 467: 464: 460: 459: 451: 447: 443: 442: 437: 430: 429: 426: 425: 422: 419: 415: 407: 405: 403: 400: 396: 392: 388: 372: 369: 347: 344: 340: 330: 328: 320: 318: 316: 313: 307: 305: 301: 296: 295: 287: 285: 283: 280: 275: 273: 268: 263: 261: 251: 250: 249: 248: 242: 238: 237: 236: 235: 234: 233: 232:Chris Hillman 228: 225: 219: 216: 210: 208: 204: 200: 199:perfect fluid 196: 191: 189: 185: 167: 164: 160: 151: 146: 143: 138: 136: 135:matter tensor 133: 129: 125: 121: 116: 114: 110: 106: 101: 95: 91: 89: 84: 83: 78: 75: 73: 70: 68: 65: 62: 58: 57: 49: 45: 41: 40: 35: 28: 27: 19: 462: 445: 439: 411: 394: 391:nonsolutions 390: 331: 324: 308: 297: 291: 276: 269: 264: 258: 229: 220: 214: 211: 206: 192: 147: 139: 131: 127: 126:. To be a 117: 108: 102: 99: 85: 60: 43: 37: 438:This is an 207:warp drives 36:This is an 325:Hi again, 260:Roadrunner 105:spacetimes 479:ArchiveĀ 4 474:ArchiveĀ 3 469:ArchiveĀ 2 463:ArchiveĀ 1 109:solutions 77:ArchiveĀ 4 72:ArchiveĀ 3 67:ArchiveĀ 2 61:ArchiveĀ 1 128:solution 441:archive 111:of the 90:article 39:archive 421:(talk) 402:(talk) 315:(talk) 282:(talk) 215:every 16:< 418:CH 399:CH 395:any 362:by 312:CH 279:CH 277:-- 148:2. 140:1. 373:Ļ€ 329:, 294:CH 115:. 452:. 370:8 348:b 345:a 341:G 168:b 165:a 161:F 50:.

Index

Talk:Alcubierre drive
archive
current talk page
ArchiveĀ 1
ArchiveĀ 2
ArchiveĀ 3
ArchiveĀ 4
Alcubierre metric
spacetimes
Einstein field equation
Einstein tensor
Riemann curvature tensor
matter tensor
vacuum solutions
electrovacuum solutions
Maxwell's equations
stress-energy tensor
classical electromagnetism
perfect fluid
cosmological constant
energy conditions
Chris Hillman
Einstein field equations
Roadrunner
exact solutions in general relativity
CH
(talk)
CH
Alcubierre drive
Notario warp drives

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