{"id":8221,"date":"2017-01-20T21:43:54","date_gmt":"2017-01-21T02:43:54","guid":{"rendered":"https:\/\/spinor.info\/weblog\/?p=8221"},"modified":"2024-04-27T00:45:13","modified_gmt":"2024-04-27T04:45:13","slug":"trace-free-gravity","status":"publish","type":"post","link":"https:\/\/spinor.info\/weblog\/?p=8221","title":{"rendered":"Trace-free gravity"},"content":{"rendered":"<p>Enough blogging about politics. It&#8217;s time to think about physics. Been a while since I last did that.<\/p>\n<p>A Facebook <a href=\"https:\/\/www.facebook.com\/sabine.hossenfelder\/posts\/10155106961549574\">post by Sabine Hossenfelder<\/a> made me look at this recent\u00a0<a href=\"https:\/\/arxiv.org\/abs\/1604.04183\">paper by Josset et al<\/a>. Indeed, the post inspired me to create a meme:<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" class=\"aligncenter wp-image-8226\" src=\"https:\/\/spinor.info\/weblog\/wp-content\/uploads\/2017\/01\/boromir-friedmann.jpg\" width=\"400\" height=\"300\" srcset=\"https:\/\/spinor.info\/weblog\/wp-content\/uploads\/2017\/01\/boromir-friedmann.jpg 700w, https:\/\/spinor.info\/weblog\/wp-content\/uploads\/2017\/01\/boromir-friedmann-300x225.jpg 300w\" sizes=\"(max-width: 400px) 100vw, 400px\" \/><\/p>\n<p>The\u00a0paper in question\u00a0contemplates the possibility that &#8220;dark energy&#8221;, i.e., the mysterious factor that leads to the observed accelerating expansion of the cosmos, is in fact due to a violation of energy conservation.<\/p>\n<p>Sounds kooky, right? Except that the violation that the authors consider is a very specific one.<\/p>\n<p>Take Einstein&#8217;s field equation,<\/p>\n<p>$$R_{\\mu\\nu}-\\tfrac{1}{2}Rg_{\\mu\\nu}+\\Lambda g_{\\mu\\nu}=8\\pi GT_{\\mu\\nu},$$<\/p>\n<p>and subtract from it a quarter of its trace times the metric. The trace of the left-hand side is \\(-R+4\\Lambda\\), the right-hand side is \\(8\\pi GT\\), so we get<\/p>\n<p>$$R_{\\mu\\nu}-\\tfrac{1}{4}Rg_{\\mu\\nu}=8\\pi G(T_{\\mu\\nu}-\\tfrac{1}{4}Tg_{\\mu\\nu}).$$<\/p>\n<p>Same equation? Not quite. For starters, the cosmological constant \\(\\Lambda\\) is gone. Furthermore, this equation is manifestly trace-free: its trace is \\(0=0\\). This theory, which was incidentally considered already almost a century ago by Einstein, is called <a href=\"https:\/\/arxiv.org\/abs\/1008.1196\">trace-free<\/a> or unimodular gravity. It is called unimodular gravity because it can be derived from the Einstein-Hilbert Lagrangian by imposing the constraint \\(\\sqrt{-g}=1\\), i.e., that the volume element is constant and not subject to variation.<\/p>\n<p>Unimodular gravity has some interesting properties. Most notably, it no longer implies the conservation law \\(\\nabla_\\mu T^{\\mu\\nu}=0\\).<\/p>\n<p>On the other hand, \\(\\nabla_\\mu(R^{\\mu\\nu}-\\tfrac{1}{2}Rg^{\\mu\\nu})=0\\) still holds, thus the gradient of the new field equation yields<\/p>\n<p>$$\\nabla_\\mu(\\tfrac{1}{4}Rg^{\\mu\\nu})=8\\pi G\\nabla_\\mu(T^{\\mu\\nu}-\\tfrac{1}{4}Tg^{\\mu\\nu}).$$<\/p>\n<p>So what happens if \\(T_{\\mu\\nu}\\) is conserved? Then we get<\/p>\n<p>$$\\nabla_\\mu(\\tfrac{1}{4}Rg^{\\mu\\nu})=-8\\pi G\\nabla_\\mu(\\tfrac{1}{4}Tg^{\\mu\\nu}),$$<\/p>\n<p>which implies the existence of the conserved quantity \\(\\hat{\\Lambda}=\\tfrac{1}{4}(R+8\\pi GT)\\).<\/p>\n<p>Using this quantity to eliminate \\(T\\) from the unimodular field equation, we obtain<\/p>\n<p>$$R_{\\mu\\nu}-\\tfrac{1}{2}Rg_{\\mu\\nu}+\\hat{\\Lambda} g_{\\mu\\nu}=8\\pi GT_{\\mu\\nu}.$$<\/p>\n<p>This is Einstein&#8217;s original field equation, but now \\(\\hat{\\Lambda}\\) is no longer a cosmological constant; it is now an integration constant that arises from a conservation law.<\/p>\n<p>The vacuum solutions of unimodular gravity are the same as those of general relativity. But what about matter solutions? It appears that if we separately impose the conservation law \\(\\nabla_\\mu T^{\\mu\\nu}\\), we pretty much get back general relativity. What we gain is a different origin, or explanation, of the cosmological constant.<\/p>\n<p>On the other hand, if we do not impose the conservation law for matter, things get interesting. In this case, we end up with an effective cosmological term that&#8217;s no longer constant. And it is this term that is the subject of the paper by Josset et al.<\/p>\n<p>That being said, a term that is time-varying in the case of a homogeneous and isotropic universe surely acquires a dependence on spatial coordinates in a nonhomogeneous environment. In particular, the nonconservation of \\(T_{\\mu\\nu}\\) should lead to testable deviations in certain Parameterized Post-Newtonian (PPN) parameters. There are some reasonably stringent limits on these parameters (notably, the parameters \\(\\alpha_3\\) and \\(\\zeta_i\\) in the notation used by Clifford Will in the 1993 revision of his book, <em>Theory and experiment in gravitational physics<\/em>) and I wonder if Josset et al. might already be in violation of these limits.<\/p>\n<fb:like href='https:\/\/spinor.info\/weblog\/?p=8221' send='true' layout='standard' show_faces='true' width='450' height='65' action='like' colorscheme='light' font='lucida grande'><\/fb:like>","protected":false},"excerpt":{"rendered":"<p>Enough blogging about politics. It&#8217;s time to think about physics. Been a while since I last did that. A Facebook post by Sabine Hossenfelder made me look at this recent\u00a0paper by Josset et al. Indeed, the post inspired me to create a meme: The\u00a0paper in question\u00a0contemplates the possibility that &#8220;dark energy&#8221;, i.e., the mysterious factor <a href='https:\/\/spinor.info\/weblog\/?p=8221' class='excerpt-more'>[&#8230;]<\/a><\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[3],"tags":[],"class_list":["post-8221","post","type-post","status-publish","format-standard","hentry","category-physics","category-3-id","post-seq-1","post-parity-odd","meta-position-corners","fix"],"_links":{"self":[{"href":"https:\/\/spinor.info\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/8221","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/spinor.info\/weblog\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/spinor.info\/weblog\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/spinor.info\/weblog\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/spinor.info\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=8221"}],"version-history":[{"count":8,"href":"https:\/\/spinor.info\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/8221\/revisions"}],"predecessor-version":[{"id":12595,"href":"https:\/\/spinor.info\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/8221\/revisions\/12595"}],"wp:attachment":[{"href":"https:\/\/spinor.info\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=8221"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spinor.info\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=8221"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spinor.info\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=8221"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}