The imperfect fluid behind kinetic gravity braiding

We present a standard hydrodynamical description for non-canonical scalar field theories with kinetic gravity braiding. In particular, this picture applies to the simplest galileons and k-essence. The fluid variables not only have a clear physical meaning but also drastically simplify the analysis o...

Full description

Saved in:
Bibliographic Details
Main Authors: Pujolàs, Oriol (Author) , Sawicki, Ignacy (Author) , Vikman, Alexander (Author)
Format: Article (Journal)
Language:English
Published: 30 November 2011
In: Journal of high energy physics
Year: 2011, Issue: 11, Pages: 1-33
ISSN:1029-8479
DOI:10.1007/JHEP11(2011)156
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1007/JHEP11(2011)156
Get full text
Author Notes:Oriol Pujolàs, Ignacy Sawicki and Alexander Vikman

MARC

LEADER 00000caa a2200000 c 4500
001 1831536447
003 DE-627
005 20230710094737.0
007 cr uuu---uuuuu
008 230119s2011 xx |||||o 00| ||eng c
024 7 |a 10.1007/JHEP11(2011)156  |2 doi 
035 |a (DE-627)1831536447 
035 |a (DE-599)KXP1831536447 
035 |a (OCoLC)1389738407 
040 |a DE-627  |b ger  |c DE-627  |e rda 
041 |a eng 
084 |a 29  |2 sdnb 
100 1 |a Pujolàs, Oriol  |e VerfasserIn  |0 (DE-588)1278626514  |0 (DE-627)1831537648  |4 aut 
245 1 4 |a The imperfect fluid behind kinetic gravity braiding  |c Oriol Pujolàs, Ignacy Sawicki and Alexander Vikman 
264 1 |c 30 November 2011 
300 |a 33 
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 19.01.2023 
520 |a We present a standard hydrodynamical description for non-canonical scalar field theories with kinetic gravity braiding. In particular, this picture applies to the simplest galileons and k-essence. The fluid variables not only have a clear physical meaning but also drastically simplify the analysis of the system. The fluid carries charges corresponding to shifts in field space. This shift-charge current contains a spatial part responsible for diffusion of the charges. Moreover, in the incompressible limit, the equation of motion becomes the standard diffusion equation. The fluid is indeed imperfect because the energy flows neither along the field gradient nor along the shift current. The fluid has zero vorticity and is not dissipative: there is no entropy production, the energy-momentum is exactly conserved, the temperature vanishes and there is no shear viscosity. Still, in an expansion around a perfect fluid one can identify terms which correct the pressure in the manner of bulk viscosity. We close by formulating the non-trivial conditions for the thermodynamic equilibrium of this imperfect fluid. 
650 4 |a Classical Theories of Gravity 
650 4 |a Cosmology of Theories beyond the SM 
650 4 |a Global Symmetries 
650 4 |a Nonperturbative Effects 
700 1 |a Sawicki, Ignacy  |d 1977-  |e VerfasserIn  |0 (DE-588)1038777585  |0 (DE-627)766452360  |0 (DE-576)392817950  |4 aut 
700 1 |a Vikman, Alexander  |d 1978-  |e VerfasserIn  |0 (DE-588)133751724  |0 (DE-627)555757501  |0 (DE-576)30007297X  |4 aut 
773 0 8 |i Enthalten in  |t Journal of high energy physics  |d Berlin : Springer, 1997  |g (2011), 11, Artikel-ID 156, Seite 1-33  |h Online-Ressource  |w (DE-627)320910571  |w (DE-600)2027350-2  |w (DE-576)095428305  |x 1029-8479  |7 nnas  |a The imperfect fluid behind kinetic gravity braiding 
773 1 8 |g year:2011  |g number:11  |g elocationid:156  |g pages:1-33  |g extent:33  |a The imperfect fluid behind kinetic gravity braiding 
856 4 0 |u https://doi.org/10.1007/JHEP11(2011)156  |x Verlag  |x Resolving-System  |z lizenzpflichtig  |3 Volltext 
951 |a AR 
992 |a 20230119 
993 |a Article 
994 |a 2011 
998 |g 1038777585  |a Sawicki, Ignacy  |m 1038777585:Sawicki, Ignacy  |d 130000  |d 130300  |e 130000PS1038777585  |e 130300PS1038777585  |k 0/130000/  |k 1/130000/130300/  |p 2 
999 |a KXP-PPN1831536447  |e 4249852067 
BIB |a Y 
SER |a journal 
JSO |a {"language":["eng"],"recId":"1831536447","note":["Gesehen am 19.01.2023"],"type":{"bibl":"article-journal","media":"Online-Ressource"},"title":[{"title":"The imperfect fluid behind kinetic gravity braiding","title_sort":"imperfect fluid behind kinetic gravity braiding"}],"person":[{"family":"Pujolàs","given":"Oriol","roleDisplay":"VerfasserIn","display":"Pujolàs, Oriol","role":"aut"},{"role":"aut","display":"Sawicki, Ignacy","roleDisplay":"VerfasserIn","given":"Ignacy","family":"Sawicki"},{"role":"aut","roleDisplay":"VerfasserIn","display":"Vikman, Alexander","given":"Alexander","family":"Vikman"}],"relHost":[{"physDesc":[{"extent":"Online-Ressource"}],"id":{"eki":["320910571"],"zdb":["2027350-2"],"issn":["1029-8479"]},"origin":[{"publisher":"Springer ; SISSA ; IOP Publ.","dateIssuedKey":"1997","dateIssuedDisp":"1997-","publisherPlace":"Berlin ; Heidelberg ; [Trieste] ; Bristol"}],"part":{"issue":"11","pages":"1-33","year":"2011","extent":"33","text":"(2011), 11, Artikel-ID 156, Seite 1-33"},"titleAlt":[{"title":"JHEP"}],"pubHistory":["Nachgewiesen 1997 -"],"language":["eng"],"corporate":[{"display":"Institute of Physics","roleDisplay":"Herausgebendes Organ","role":"isb"}],"recId":"320910571","note":["Gesehen am 02.12.20"],"disp":"The imperfect fluid behind kinetic gravity braidingJournal of high energy physics","type":{"media":"Online-Ressource","bibl":"periodical"},"title":[{"title_sort":"Journal of high energy physics","subtitle":"JHEP ; a refereed journal written, run, and distributed by electronic means","title":"Journal of high energy physics"}]}],"physDesc":[{"extent":"33 S."}],"id":{"doi":["10.1007/JHEP11(2011)156"],"eki":["1831536447"]},"origin":[{"dateIssuedDisp":"30 November 2011","dateIssuedKey":"2011"}],"name":{"displayForm":["Oriol Pujolàs, Ignacy Sawicki and Alexander Vikman"]}} 
SRT |a PUJOLASORIIMPERFECTF3020