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About Omics Group

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About Omics Group OMICS Group International through its Open Access Initiative is committed to make genuine and reliable contributions to the scientific community. – PowerPoint PPT presentation

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Title: About Omics Group


1
About Omics Group
  • OMICS Group International through its Open Access
    Initiative is committed to make genuine and
    reliable contributions to the scientific
    community. OMICS Group hosts over 400
    leading-edge peer reviewed Open Access Journals
    and organize over 300 International Conferences
    annually all over the world. OMICS Publishing
    Group journals have over 3 million readers and
    the fame and success of the same can be
    attributed to the strong editorial board which
    contains over 30000 eminent personalities that
    ensure a rapid, quality and quick review process. 

2
About Omics Group conferences
  • OMICS Group signed an agreement with more than
    1000 International Societies to make healthcare
    information Open Access. OMICS Group Conferences
    make the perfect platform for global networking
    as it brings together renowned speakers and
    scientists across the globe to a most exciting
    and memorable scientific event filled with much
    enlightening interactive sessions, world class
    exhibitions and poster presentations
  • Omics group has organised 500 conferences,
    workshops and national symposium across the major
    cities including SanFrancisco,Omaha,Orlado,Rayleig
    h,SantaClara,Chicago,Philadelphia,Unitedkingdom,Ba
    ltimore,SanAntanio,Dubai,Hyderabad,Bangaluru and
    Mumbai.

3
Growth and Operation Tolerances for Sb-based
Mid-Infrared Lasers C.H. Grein University of
Illinois at Chicago Collaborators M.E. Flatté
and T.F. Boggess (University of Iowa)
4
Outline
  • Background on Sb-based superlattice mid-infrared
    lasers
  • Sensitivity of optimization of mid-infrared
    InAs/GaInSb superlattice laser active regions to
  • Temperature
  • Superlattice layer thicknesses
  • Structure of intersubband absorption spectrum
  • Initial/final state optimization in four-layer
    superlattices

5
Optimization Strategies
  • Band edge optimization
  • reduce valence band density of states
  • strained layer superlattices heavy hole becomes
    lighter in in-plane direction
  • Intersubband absorption reduction
  • engineering bands which would otherwise provide
    initial or final states for intervalence or
    interconduction transitions at the lasing energy
  • Auger final state optimization
  • band structure engineering to reduce the number
    of final states in Auger transitions

6
  • Superlattice Band Structure Engineering
  • Responsible for order of magnitude or greater
    reductions of Auger rates
  • LWIR
  • Good agreement between theory and expt. for
    ngt1017 cm-3
  • Shockley-Read-Hall dominates for nlt1017 cm-3
  • Youngdale et al., APL 64, 3160 (1994)
  • MWIR
  • Auger coefficient?3
  • R?1 ?2n ?3n2
  • W.W. Bewley et al., APL 93, 041118 (2008)

7
Observed Strained Layer Superlattice and Bulk
Auger Coefficients R?1 ?2n ?3n2
System T (K) ?3 (cm6/s) Ref.
InAs/GaInSb?c8.8 ?m vs. HgCdTe ?c9 ?m 77 1.3x10-27 2x10-25 Youngdale et al. (1994)
InAs/InAsSb ?c9 ?m vs. InSb ?c7 ?m 300 1.4x10-28 1.0x10-26 Ciesla et al. (1996)
InAs/InGaSb/InAs/AlGaInAsSb ?c4.1 ?m vs. InAsSb ?c4.5 ?m 300 2.9x10-27 2.0x10-26 Flatte et al. (1999)
InAs/GaInSb ?c3.6 ?m vs. InAs ?c3.5 ?m 300 4.0x10-27 1.1x10-26 Kost et al. (2005) Vodopyanov et al. (1992)
  • Roughly two orders of magnitude slower Auger
    recombination in LWIR SLs than in bulk
  • Roughly one order of magnitude slower in MWIR

8
K.p Electronic Band Structure Model
  • Expansion in zone-center basis (emphasizing
    zone-center accuracy)
  • k typically less than 0.2Å-1
  • Spherical (8-band) or cubic (14-band) symmetry
  • Relevant region of bulk band structure for
    optical and recombination properties

SUCCESSES Simplicity Parameters connected 1-1
with experiments Energy levels and masses 5-10
meV Absorption/gain spectra 10 fundamental
absorption (inc. excitons) 20 differential
transmission in SLMQW Auger/radiative
rates Within factor of 2 for several material
systems
CHALLENGES Indirect constituents e.g.
AlSb Defects Sometimes require full Brillouin
zone Interface roughness For islands of diameter
less than 15Å
9
InAs/GaSb A Type II Broken Gap Superlattice With
Controllable Interface Bonds
10
Carrier Recombination Calculations
  • Auger recombination
  • three dimensional formalism
  • non-parabolic bands splined from K?p
  • dispersion in matrix elements, splined from K?p
  • possible degenerate carrier statistics
  • modified version of well-tested superlattice code
  • typical factor of 2 agreement with experiment
  • Radiative recombination
  • excludes photon recycling
  • based on van Roosbroeck- Shockley
  • Impurity and defect mediated recombination
  • Neglected ?theoretical upper bounds to carrier
    lifetimes

11
Auger Recombination Formalism
Rate for band-to-band transitions (Fermis Golden
Rule)
Matrix element is
Common approximations (not employed
here) -parabolic and isotropic bands -constant
matrix elements -Boltzmann statistics -limitations
to i, f -neglect Umklapp-neglect T-dependence
of bands -neglect dopant/phonon/defect-assisted
Auger
49.7Å InAs/57Å Ga0.9In0.1Sb Auger-1 most probable
carriers at 40 K (electrons-solid circles holes
and empty states-hollow circles)
12
Experiment vs. Theory Auger Recombination Rates
13
Case Study 15 Micron Cutoff SLs and In
Importance of Strain
  • 49.7Å InAs/57Å Ga0.9In0.1Sb (10 In)
  • 47Å InAs/21.5Å Ga0.75In0.25Sb (25 In)
  • Vary In but keep band gap fixed
  • Test effects of band structure on Auger
    recombination

14
Hole-Hole Auger Transitions ?15 ?m, T40 K
49.7Å InAs/57Å Ga0.9In0.1Sb (10 In) ?A75.2x10-9
s
47Å InAs/21.5Å Ga0.75In0.25Sb (25 In) ?A7 gt 1 s
15
Temperature Sensitivity of Optimization
  • Valence bands approximately one energy gap below
    top of valence band provide
  • initial states for intersubband absorption
  • final states for dominant Auger processes at room
    temperature (AM-7)
  • Temperature changes move valence bands through
    resonance region
  • Two-layer MWIR superlattices
  • 16.7Å InAs/35Å In0.25Ga0.75Sb-optimization
    ceases above 150 K To good figure of merit
  • 12.5Å InAs/39Å In0.25Ga0.75Sb- optimized from 250
    K to 350 K To figure of merit inapplicable

16
Temperature Sensitivity of Electronic Band
Structure
17
Valence Intersubband Absorption
12.5Å InAs/39Å In0.25Ga0.75Sb
18
Intersubband Absorption, Threshold Carrier and
Threshold Current Densities
19
Layer Thickness Sensitivity of Optimization
  • Band structures for superlattices with same
    energy gap but different In0.25Ga0.75Sb layer
    thicknesses (300 K)

20
Intersubband Absorption, Threshold Carrier and
Current Densities
Require growth accuracy 3.5 Å for InGaSb, 0.25
Å for InAs
21
MWIR Four-Layer Superlattice
  • Incorporate strain-compensating quintarnary
    layer InAs/In0.25Ga0.75Sb/InAs/Al0.30Ga0.42In0.28
    A0.50Sb0.50
  • strain compensation occurs over 100 Å SL period
  • provides Auger recombination and intersubband
    absorption optimization
  • 3.7 µm wavelength at 300 K

22
Importance of Umklapp and Saturation
23
Temperature Sensitivity of Auger Final State
Optimization
Blue valence subbands 4, 5, 6
24
Artificially Shift Valence Subbands 4, 5, 6
  • Increasing temperature has a profound impact on
    final-state optimization for Auger suppression
  • At 77 K the final-state optimization is very
    important
  • At 300 K the final-state optimization has just
    ceased to be of any importance
  • -this structure it may still be important at
    temperatures just slightly lower

25
SUMMARY
  • Details of temperature dependent valence band
    structure particularly important for optimizing
    design of Sb-based MWIR active regions
  • Strong intersubband absorption structure can make
    To parameterization inapplicable
  • Observe saturation of Auger recombination at high
    carrier densities
  • Occurs when holes become degenerate?hh Auger
    dominant
  • Superlattice Umklapp processes provide about half
    of total Auger rate

26
Let Us Meet Again
  • We welcome all to our future group conferences of
    Omics group international
  • Please visit
  • www.omicsgroup.com
  • www.Conferenceseries.com
  • http//optics.conferenceseries.com/
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