Title: Black Hole Production at Collider
1Black Hole Production at Collider
- Kin-ya Oda (RIKEN)
- based on work with
- Daisuke Ida (Gakushuin)
- Seong Chan Park (Seoul National Univ)
- PRD67 th/0212108 71 (2005) 73 (2006)
- and also
- Nobuchika Okada (KEK)
- PRD66 ph/0111298
- Manuel Drees and Christian Alig (Bonn)
- ph/0610269 to appear in JHEP
2Outline
- Planck scale can be as low as TeV
- TeV gravity inevitably leads to BH production
- Obtained brane field equations in separable form
-gt greybody factors - Obtained Hawking radiation spectra -gt BH time
evolution - Summary Outlook
3Planck scale can be as low as TeV
Arkani-Hamed, Dimopoulos, Dvali 98
- We live in 3-brane in (4n)-dim bulk
- SM fields trapped on the brane
- massless modes of open strings
- Gravitons propagate in bulk
- massless modes of closed strings
(D4n)
'Gauss law' ? MD2n M42 L -n
free! ? exp free
Fundamental gravitational scale can beas low as
MPTeV!
4Alternative Warped compn
Randall, Sundrum 99
5Is TeV gravity natural?
Bruce Lee Yoda in STARWARS
- Answer 1 Dont think. Feel.
- Naturalness argument thriveswhen theory is
desperately untestable. - Why bothered by metaphysical question when LHC
starts taking datanext-to-next year?
6Is TeV gravity natural?
- Answer 2 Yes, its as natural as MP 1018GeV.
- ADD A little hierarchy L106 MP-1 needed. So
what? - L is a modulus fixed dynamically.
- Note Compn radius L is a flat direction of
(perturbative) string vacua and hece totally
free parameter. - When lifting up flat direction, its all common
to have a huge shift. - RS Generically, string (flux) compactification
is warped! - Throat, warped compn on AdS,can now be seen
everywhere in string theory. - More radically, take
Hewett, Lillie, Rizzo 05
7Outline
- Planck scale can be as low as TeV
- TeV gravity inevitably leads to BH production
- Obtained brane field equations in separable form
-gt greybody factors - Obtained Hawking radiation spectra -gt BH time
evolution - Summary Outlook
8Geometrical cross section
Cross section rises with energy
9TeV gravity inevitably leads toBH production
- Classical cross section grows with energy BH
production dominates over all other interactions
above TeV.t Hooft - low energy string picture will be altered by BH
picture (correspondence principle) Horowitz,
Polchinski - The end of short distance physicsGiddings,
Thomas
Classical production
Eardley, Giddings, Yoshino, Nambu Yoshino Rychkov
10Correspondence principle
Horowitz, Polchinski 96, 97
Also Correspondence in hard scattering
suppression K.O., Okada 02
String picture
There is no complete description
- Truly QG effects will be observed as a deviation
from asymptotic behavior (in BH picture). - It is crucial to predict BH behavioras precisely
as possible!!
11Typical BH event at LHC in Schwarzschild
approximation
A clean signal per second!
Simulation with MBH 8 TeV in ATLAS
and in CMS
from Kobayashi DPF/JPS 06
12BH life in detector
- Balding Phase (negligible?)
- Dynamical production phase
- BH loses its hair.
- Spin Down Phase
- BH loses its mass and angular momentum.
- Schwartzschild Phase
- Angular momentum is small.
- BH loses its mass.
- Planck Phase
- Truly QG, highly unpredictable
- A few quanta would be emitted.
13What follows from BH production
Giddings, Thomas 01 Dimopoulos, Landsberg 01
- Decay
- Radiates mainly on brane
- decay proportional to (dof)h q l v 4
72 18 24 - Typically at LHC
- Produced every second (millions per year)
- M up to 10 TeV
- T above .1 TeV
- Tens of multiple emissions
- Life time 10-27sec
14Outline
- Planck scale can be as low as TeV
- TeV gravity inevitably leads to BH production
- Obtained brane field equations in separable form
-gt greybody factors - Obtained Hawking radiation spectra -gt BH time
evolution - Summary Outlook
15BH is produced with large angular momentum
Ida, KO, Park 02
16Higher dim. Kerr metric(just to show how it
looks)
Mayers, Perry
vanishes on the brane
17Newman Penrose formalism(just to show how it
looks)
Null tetrads
18Field equations on brane
Ida, KO, Park
Separation of variables
angular part
radial part
19Greybody factor determines Hawking radiation and
BH evolution
BH radiates mainly into the brane (SM) fields
via Hawking radiation.
Greybody factors for Brane fields determine the
evolution of BH mass and angular momentum (up to
Planck phase).
20How to get greybody factor
out
in
purely ingoing
in a time-reversed sense
21Greybody factor for vector
Ida, KO, Park
22Outline
- Planck scale can be as low as TeV
- TeV gravity inevitably leads to BH production
- Obtained brane field equations in separable form
-gt greybody factors - Obtained Hawking radiation spectra -gt BH time
evolution - Summary Outlook
23Spinor power/angular spectrum
Ida, KO, Park
24Vector power/angular spectrum
Ida, KO, Park
25Power spectrum for various dim
Ida, KO, Park
Spinor peaks for high rotation are only for
Randall-Sundrum (D5) BH
26Substructure spinor/vector
Ida, KO, Park
27Approx. spinor power, angle dependence
Ida, KO, Park
Similar for vector.
28Spin-down phase issizable
Ida, KO, Park
70 of total energy is radiated during spin-down
phase
29What we found
Ida, K.O., Park 02, 05, 06
- Obtained brane field equations essential for
Hawking radiation - BH is produced with large angular momentum.
- Spin down phase contributesa lot.
- Quarks, leptons and gauge bosons are emitted
along the angular momentum axis perpendicular to
beam axis. polar emissision (except for
extremely high rotation) - (Black ring might form)
30Chromosphere (QG plasma) doesnt form
Alig, Drees, K.O. 06
Simulation based on the heavy ion collision code
30 bins in ? 15 bins in ?
31Summary Outlook
- Balding phase, still disputed
- Can complete time evolution up to Planck phase.
- Comparison with these predictions will guide the
way to quantum gravity!
- Planck scale can be as low as TeV.
- TeV gravity inevitably leads to BH production.
- Precise determination of BH event important
- BH is produced with large angular momentum.
- Hawking radiation is highly anisotropic
- 70 energy is emitted during spin down phase.
- (Black ring might form.)
- QCD QG plasma does not form (w/ Alig Drees)