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Luca Martucci
Flux vacua in String Theory, generalized calibrations and
supersymmetry breaking
Workshop on complex geometry and supersymmetry, IPMU January 4-9 2009
Plan of this talk
Generalized calibrations and fluxes
Calibrations, SUSY-breaking and 4D potential
Generalized calibrations and SUSY vacua
Generalized calibrations and fluxes
Ordinary calibrations
An ordinary calibration is a differential -form such that
Harvey & Lawson `82
1) Algebraic condition:
2) Differential condition:
for any-dim submanifold
Calibrated submanifolds:
Ordinary calibrations
Main property: calibrated cycles are volume minimizing
Harvey & Lawson `82
Ordinary calibrations
Main property: calibrated cycles are volume minimizing
Harvey & Lawson `82
Ordinary calibrations
algebraic condition
Main property: calibrated cycles are volume minimizing
Harvey & Lawson `82
Ordinary calibrations
algebraic condition
differential condition
Main property: calibrated cycles are volume minimizing
Harvey & Lawson `82
Ordinary calibrations
algebraic condition
calibration condition
differential condition
Main property: calibrated cycles are volume minimizing
Harvey & Lawson `82
Supersymmetric branes and calibrations (no fluxes)
Supersymmetric branes and calibrations (no fluxes)
In absence of fluxes, a static -brane wrapping has energy
Supersymmetric branes and calibrations (no fluxes)
We expect BPS bound for supersymmetric branes
if
In absence of fluxes, a static -brane wrapping has energy
Supersymmetric branes and calibrations (no fluxes)
We expect BPS bound for supersymmetric branes
if
In absence of fluxes, a static -brane wrapping has energy
Explicitly realized by calibrations
bulk SUSY
brane SUSY
-calibration
How to include (type II) String Theory fluxes?
How to include (type II) String Theory fluxes?
Type II bulk fields
• NS sector:
• RR sector:
(locally )
(locally )
IIA IIB
, ,
How to include (type II) String Theory fluxes?
Type II bulk fields
• NS sector:
• RR sector:
(locally )
(locally )
IIA IIB
, ,
D-brane world-volume field: flux such that
(locally )
How to include (type II) String Theory fluxes?
D-brane energy density:
Type II bulk fields
• NS sector:
• RR sector:
(locally )
(locally )
IIA IIB
, ,
D-brane world-volume field: flux such that
(locally )
How to include (type II) String Theory fluxes?
D-brane energy density:
Type II bulk fields
• NS sector:
• RR sector:
(locally )
(locally )
IIA IIB
, ,
D-brane world-volume field: flux such that
(locally )
How to include (type II) String Theory fluxes?
D-brane energy density:
Type II bulk fields
• NS sector:
• RR sector:
(locally )
(locally )
IIA IIB
, ,
D-brane world-volume field: flux such that
(locally )
Generalized calibrationsKoerber `05; L.M. & Smyth `05
Generalized calibrationsKoerber `05; L.M. & Smyth `05
A generalized calibration is a background polyform
Generalized calibrationsKoerber `05; L.M. & Smyth `05
A generalized calibration is a background polyform
such that: 1)
2)
Algebraic:
Differential:
Generalized calibrationsKoerber `05; L.M. & Smyth `05
Gutowski, Papadopoulos& Townsend `99
`ordinary’ generalized calibrations
A generalized calibration is a background polyform
such that: 1)
2)
Algebraic:
Differential:
Generalized calibrationsKoerber `05; L.M. & Smyth `05
Gutowski, Papadopoulos& Townsend `99
`ordinary’ generalized calibrations
generalizedgeometry
A generalized calibration is a background polyform
such that: 1)
2)
Algebraic:
Differential:
Generalized calibrationsKoerber `05; L.M. & Smyth `05
Calibrated (or BPS) D-branes:
Gutowski, Papadopoulos& Townsend `99
`ordinary’ generalized calibrations
generalizedgeometry
A generalized calibration is a background polyform
such that: 1)
2)
Algebraic:
Differential:
The stability argument• Main property: calibrated D-branes are stable!
The stability argument• Main property: calibrated D-branes are stable!
The stability argument• Main property: calibrated D-branes are stable!
algebraic condition
The stability argument• Main property: calibrated D-branes are stable!
algebraic condition
differential condition
The stability argument• Main property: calibrated D-branes are stable!
algebraic condition
differential condition
D-brane calibration condition
Generalized calibrations and type II SUSY vacua
N=1 vacua and pure spinors
w
(or )
,plus ,
,
General 4+6 backgrounds:
Ordinary Killing spinors:
N=1 vacua and pure spinors
w
(or )
,
Ordinary Killing spinors: S0(6,6) pure spinors
N=1 vacua and pure spinors
w
(or )
,
Ordinary Killing spinors:
in IIB
in IIA
S0(6,6) pure spinors
N=1 vacua and pure spinors
w
(or )
,
Ordinary Killing spinors: S0(6,6) pure spinors
N=1 vacua and pure spinors
w
(or )
contain completeinformation about:
and
, and
and
NS sector:( excluded)
Internal spinors:
,
N=1 vacua and calibrationsL.M. & Smyth `05
SUSY conditions
w
Graña, Minasian, Petrini & Tomasiello `05 ,
N=1 vacua and calibrationsL.M. & Smyth `05
SUSY conditions
w
Graña, Minasian, Petrini & Tomasiello `05 ,
N=1 vacua and calibrationsL.M. & Smyth `05
SUSY conditions
w
Graña, Minasian, Petrini & Tomasiello `05
defines integrable generalized CY structure!
,
N=1 vacua and calibrationsL.M. & Smyth `05
SUSY conditions
They have a natural interpretation in terms of D-brane generalized calibrations!
w
Graña, Minasian, Petrini & Tomasiello `05
defines integrable generalized CY structure!
,
N=1 vacua and calibrationsL.M. & Smyth `05
is a generalized calibration for space-filling D-branes
space-filling
N=1 vacua and calibrationsL.M. & Smyth `05
is a generalized calibration for space-filling D-branes
space-filling
For SUSY (BPS) space-filling D-branes, internal satisfies:
N=1 vacua and calibrationsL.M. & Smyth `05
is a generalized calibration for space-filling D-branes
space-filling
For SUSY (BPS) space-filling D-branes, internal satisfies:
is generalized complex submanifold
w.r.t. GCS defined by
satisfies the `speciality’ condition
(F-flatness)
(D-flatness)
BPS lower bound for D-brane energy
no open-string tachyons!
N=1 vacua and calibrationsL.M. & Smyth `05
BPS lower bound for D-brane energy
no open-string tachyons!
N=1 vacua and calibrationsL.M. & Smyth `05
GaugeBPSness
For space-filling D-branes, it originates in bulk SUSY condition
N=1 vacua and calibrationsL.M. & Smyth `05
is a generalized calibration for D-strings
stringsstring
BPSness
N=1 vacua and calibrationsL.M. & Smyth `05
is a generalized calibration for D-strings
stringsstring
BPSness
is a generalized calibration for domain walls
domain wallsDWBPSness
Summarizing
Equation D-brane BPSness 4D SUGRA int.
gauge BPSness
string BPSness
DW BPSness
Graña, Minasian, Petrini
& Tomasiello `05 L.M. & Smyth`05 Koerber & L.M. `07
In N=1 compactifications (to flat ) we have
chiral fields:
(N=2 vect. mult.)
(N=2 hypermult.)
Pre-GG Example: type IIB warped CYGraña & Polchinski `00;
Giddings, Kachru & Polchinski`01
The internal metric is CY, up to warping:
Pre-GG Example: type IIB warped CYGraña & Polchinski `00;
Giddings, Kachru & Polchinski`01
The internal metric is CY, up to warping:
Pre-GG Example: type IIB warped CYGraña & Polchinski `00;
Giddings, Kachru & Polchinski`01
In this case: ,
The internal metric is CY, up to warping:
SUSY wCY and calibrations
SUSY wCY and calibrations
Gauge BPSness:calibrated
D3 & D7 branes
SUSY wCY and calibrations
String BPSness:calibrated
D3 & D7 branes
Gauge BPSness:calibrated
D3 & D7 branes
SUSY wCY and calibrations
String BPSness:calibrated
D3 & D7 branes
DW BPSness: calibratedD5 & D7 branes
Gauge BPSness:calibrated
D3 & D7 branes
Calibrations, SUSY-breakingand 4D potential
Lüst, Marchesano, L.M. & Tsimpis`07
SUSY breaking?
Pre-GG prototypical example: IIB wCYGraña & Polchinski `00;
Giddings, Kachru & Polchinski`01
SUSY breaking?
Pre-GG prototypical example: IIB wCYGraña & Polchinski `00;
Giddings, Kachru & Polchinski`01
with 03/O7 and D3/D7
N=1 and N=0 shear the same geometry
SUSY breaking?
Pre-GG prototypical example: IIB wCYGraña & Polchinski `00;
Giddings, Kachru & Polchinski`01
with 03/O7 and D3/D7
N=1 and N=0 shear the same geometry
flux induced SUSY-breaking:
SUSY breaking?
Pre-GG prototypical example: IIB wCYGraña & Polchinski `00;
Giddings, Kachru & Polchinski`01
with 03/O7 and D3/D7
N=1 and N=0 shear the same geometry
Many `phenomenological’ models are based on these classical vacua
Kachru, Kallosh,, Linde & Trivedi `03; + MacAllister & Maldacena `03
Balasubramanian,, Berglund,, Conlon & Quevedo `05
e.g.
flux induced SUSY-breaking:
SUSY wCY and calibrations
In this case: ,
Gauge BPSness:
String BPSness:
DW (non)BPSness:
calibratedD3 & D7 branes
calibratedD3 & D7 branes
calibratedD5 & D7 branes( )
Generalized SUSY-breaking
Generalized SUSY-breaking
We are led to consider backgrounds that fulfill gauge and string BPSness, but not DW BPSness
Generalized SUSY-breaking
We are led to consider backgrounds that fulfill gauge and string BPSness, but not DW BPSness
domain wallsstringsspace-filling
, ,
BPS bounds for
Generalized SUSY-breaking
We are led to consider backgrounds that fulfill gauge and string BPSness, but not DW BPSness
DWSB backgrounds
domain wallsstringsspace-filling
, ,
BPS bounds for
Generalized SUSY-breaking
DWSB backgrounds
Equation D-brane BPSness 4D SUGRA int.
gauge BPSness
string BPSness
DW (non)BPSness
Generalized SUSY-breaking
In wCY, the DWSB has rather specific form
crucial to solve10D e.o.m.
Generalized SUSY-breaking
In wCY, the DWSB has rather specific form
crucial to solve10D e.o.m.
Can we analogously restrict the generalized DWSB?
?
1-parameter DWSB
1-parameter DWSB Take generalized fibration
(Dirac structure)
1-parameter DWSB
spanned by mobile D-branes
Take generalized fibration(Dirac structure)
1-parameter DWSB
spanned by mobile D-branes
Take generalized fibration(Dirac structure)
Consider DWSB of the form
1-parameter DWSB
spanned by mobile D-branes
Take generalized fibration(Dirac structure)
SUSY-breaking parameter
Consider DWSB of the form
1-parameter DWSB Take generalized fibration
(Dirac structure)
Consider DWSB of the form
In wCY case:
SUSY-breaking parameter
spanned by mobile D-branes
1-parameter DWSB Take generalized fibration
(Dirac structure)
Consider DWSB of the form
In wCY case: (and thus )
SUSY-breaking parameter
spanned by mobile D-branes
1-parameter DWSB Take generalized fibration
(Dirac structure)
Consider DWSB of the form
In wCY case:
spanned by mobile D3
(and thus )
SUSY-breaking parameter
spanned by mobile D-branes
1-parameter DWSB Take generalized fibration
(Dirac structure)
Consider DWSB of the form
In wCY case:
spanned by mobile D3
(and thus )
SUSY-breaking parameter
spanned by mobile D-branes
1-parameter DWSB Take generalized fibration
(Dirac structure)
Consider DWSB of the form
In wCY case:
spanned by mobile D3
(and thus )
,
SUSY-breaking parameter
spanned by mobile D-branes
1-parameter DWSB Take generalized fibration
(Dirac structure)
How to check that 10D e.o.m. are satisfied?
Which conditions must fullfill?
SUSY-breaking parameter
Consider DWSB of the form
10D e.o.m. from 4D potential General configurations of the form
,plus ,D-branes & orientifolds
,
10D e.o.m. from 4D potential General configurations of the form
,plus ,D-branes & orientifolds
,
The full set of 10D e.o.m. can be obtained from
10D e.o.m. from 4D potential General configurations of the form
We need to express the potential in terms of and
,plus ,D-branes & orientifolds
,
The full set of 10D e.o.m. can be obtained from
Potential and pure spinorsWe found, schematically (see also Cassani `08)
(...)
Potential and pure spinorsWe found, schematically (see also Cassani `08)
(...)
>- 0
>- 0
>- 0
>- 0
<- 0
<- 0
Potential and pure spinorsWe found, schematically (see also Cassani `08)
(...)
>- 0
>- 0
>- 0
>- 0
<- 0
<- 0
(gauge BPSness)2
(string BPSness)2
(DW BPSness)2
(D-brane BPS bound)
(DW BPSness)2
(string + DW BPSness)2
~
~
~
~
~
>- 0
-
>- 0
>- 0
> 0
Potential for 1-param. DWSB
>- 0
>- 0
>- 0
>- 0
calibrated D-branes
Potential for 1-param. DWSB
>- 0
>- 0
>- 0
gauge BPSness ( )
Potential for 1-param. DWSB
>- 0
>- 0
>- 0
>- 0
string BPSness ( )
Potential for 1-param. DWSB
>- 0
>- 0
>- 0
>- 0
calibrated generalized fibration
( )
Potential for 1-param. DWSB
>- 0
>- 0
>- 0
>- 0
calibrated generalized fibration
( )-dependence disappears: no-scale structure
Potential for 1-param. DWSB
>- 0
An example
Example: SU(3)-structure with D5/O5[cfr. Camara & Graña `07]
Example: SU(3)-structure with D5/O5[cfr. Camara & Graña `07]
In this case: ,
Example: SU(3)-structure with D5/O5[cfr. Camara & Graña `07]
In this case: ,
Gauge + string BPSness:
non-Kähler
ISD
Example: SU(3)-structure with D5/O5[cfr. Camara & Graña `07]
In this case: ,
Gauge + string BPSness:
non-Kähler
ISD
DWSB:
Example: SU(3)-structure with D5/O5[cfr. Camara & Graña `07]
In this case: ,
Gauge + string BPSness:
non-Kähler
ISD
DWSB:
Notice that: non-integrable complex structure if
Explicit example on twisted torus
Explicit example on twisted torus
Explicit example on twisted torus
Twisted periodicity in 3 direction:rd
Explicit example on twisted torus
Twisted periodicity in 3 direction:rd
Metric and fields
,
Explicit example on twisted torus
Twisted periodicity in 3 direction:rd
Metric and fields
,
SU(3)-structure
Explicit example on twisted torus
Twisted periodicity in 3 direction:rd
Metric and fields
,
SU(3)-structure
twist-induced DWSB DWSB
Conclusion
Conclusion
Generic type II flux compactifications are naturally described by generalized calibrations
Conclusion
Generic type II flux compactifications are naturally described by generalized calibrations
SUSY
• emergent N=1 4D effective structures
• integrable GC and calibration structures
Conclusion
Generic type II flux compactifications are naturally described by generalized calibrations
SUSY
• emergent N=1 4D effective structures
• integrable GC and calibration structures
SUSY
• less clear N=1 4D structures
• integrable GC but still calibration structures