Photoionization cross section in a strained semimagnetic double quantum well under hydrostatic pressure, nonparabolicity and polaronic mass effects
In this research, we conducted a numerical analysis on the photoionization cross section (PCS) of a shallow donor impurity confined in a diluted magnetic semiconductor (DMS) C d...
Ausführliche Beschreibung
Autor*in: |
Azmi, H. [verfasserIn] Amri, N. [verfasserIn] Nithiananthi, P. [verfasserIn] Jaouane, M. [verfasserIn] El-Bakkari, K. [verfasserIn] Sali, A. [verfasserIn] Ed-Dahmouny, A. [verfasserIn] Fakkahi, A. [verfasserIn] Arraoui, R. [verfasserIn] |
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E-Artikel |
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Sprache: |
Englisch |
Erschienen: |
2024 |
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Schlagwörter: |
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Übergeordnetes Werk: |
Enthalten in: Physica / B - Amsterdam : Elsevier, 1988, 677 |
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Übergeordnetes Werk: |
volume:677 |
DOI / URN: |
10.1016/j.physb.2024.415717 |
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Katalog-ID: |
ELV067071953 |
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245 | 1 | 0 | |a Photoionization cross section in a strained semimagnetic double quantum well under hydrostatic pressure, nonparabolicity and polaronic mass effects |
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520 | |a In this research, we conducted a numerical analysis on the photoionization cross section (PCS) of a shallow donor impurity confined in a diluted magnetic semiconductor (DMS) C d 1 − x w M n x w T e / C d 1 − x b M n x b T e double quantum well (DQW). The effective-mass approximation was employed, and the Schrödinger equation describing the electron motion was solved using the variational method. This study focuses on calculating the binding energy ( E b ) by taking into account the effect of spin polaronic shift. Moreover, we calculated the photoionization cross-section (PCS) considering different polarized light directions, varying well widths ( L w ) , barrier thickness ( L b ) , and different hydrostatic pressure ( P ) values as well as the incorporation of the effect of the non-parabolicity (NP) conduction band and polaronic mass (PM). The results reveal that the overall shape of the PCS depends strongly on the light polarization axis. Additionally, the threshold energy exhibits a blueshift with increasing barrier thickness and hydrostatic pressure, and a redshift with increasing the well width. | ||
650 | 4 | |a Semimagnetic double quantum well | |
650 | 4 | |a Spin polaronic shift | |
650 | 4 | |a Binding energy | |
650 | 4 | |a Hydrostatic pressure | |
650 | 4 | |a Non-parabolicity | |
650 | 4 | |a Photoionization cross-section | |
700 | 1 | |a Amri, N. |e verfasserin |4 aut | |
700 | 1 | |a Nithiananthi, P. |e verfasserin |0 (orcid)0000-0001-7759-1513 |4 aut | |
700 | 1 | |a Jaouane, M. |e verfasserin |4 aut | |
700 | 1 | |a El-Bakkari, K. |e verfasserin |0 (orcid)0000-0003-3649-7373 |4 aut | |
700 | 1 | |a Sali, A. |e verfasserin |0 (orcid)0000-0003-4153-3404 |4 aut | |
700 | 1 | |a Ed-Dahmouny, A. |e verfasserin |0 (orcid)0000-0003-4390-853X |4 aut | |
700 | 1 | |a Fakkahi, A. |e verfasserin |0 (orcid)0000-0003-0025-9066 |4 aut | |
700 | 1 | |a Arraoui, R. |e verfasserin |4 aut | |
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allfields |
10.1016/j.physb.2024.415717 doi (DE-627)ELV067071953 (ELSEVIER)S0921-4526(24)00058-9 DE-627 ger DE-627 rda eng 530 VZ 33.60 bkl 51.00 bkl Azmi, H. verfasserin (orcid)0009-0002-8967-1603 aut Photoionization cross section in a strained semimagnetic double quantum well under hydrostatic pressure, nonparabolicity and polaronic mass effects 2024 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier In this research, we conducted a numerical analysis on the photoionization cross section (PCS) of a shallow donor impurity confined in a diluted magnetic semiconductor (DMS) C d 1 − x w M n x w T e / C d 1 − x b M n x b T e double quantum well (DQW). The effective-mass approximation was employed, and the Schrödinger equation describing the electron motion was solved using the variational method. This study focuses on calculating the binding energy ( E b ) by taking into account the effect of spin polaronic shift. Moreover, we calculated the photoionization cross-section (PCS) considering different polarized light directions, varying well widths ( L w ) , barrier thickness ( L b ) , and different hydrostatic pressure ( P ) values as well as the incorporation of the effect of the non-parabolicity (NP) conduction band and polaronic mass (PM). The results reveal that the overall shape of the PCS depends strongly on the light polarization axis. Additionally, the threshold energy exhibits a blueshift with increasing barrier thickness and hydrostatic pressure, and a redshift with increasing the well width. Semimagnetic double quantum well Spin polaronic shift Binding energy Hydrostatic pressure Non-parabolicity Photoionization cross-section Amri, N. verfasserin aut Nithiananthi, P. verfasserin (orcid)0000-0001-7759-1513 aut Jaouane, M. verfasserin aut El-Bakkari, K. verfasserin (orcid)0000-0003-3649-7373 aut Sali, A. verfasserin (orcid)0000-0003-4153-3404 aut Ed-Dahmouny, A. verfasserin (orcid)0000-0003-4390-853X aut Fakkahi, A. verfasserin (orcid)0000-0003-0025-9066 aut Arraoui, R. verfasserin aut Enthalten in Physica / B Amsterdam : Elsevier, 1988 677 Online-Ressource (DE-627)266015093 (DE-600)1466579-7 (DE-576)074959840 1873-2135 nnns volume:677 GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2088 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.60 Kondensierte Materie: Allgemeines VZ 51.00 Werkstoffkunde: Allgemeines VZ AR 677 |
spelling |
10.1016/j.physb.2024.415717 doi (DE-627)ELV067071953 (ELSEVIER)S0921-4526(24)00058-9 DE-627 ger DE-627 rda eng 530 VZ 33.60 bkl 51.00 bkl Azmi, H. verfasserin (orcid)0009-0002-8967-1603 aut Photoionization cross section in a strained semimagnetic double quantum well under hydrostatic pressure, nonparabolicity and polaronic mass effects 2024 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier In this research, we conducted a numerical analysis on the photoionization cross section (PCS) of a shallow donor impurity confined in a diluted magnetic semiconductor (DMS) C d 1 − x w M n x w T e / C d 1 − x b M n x b T e double quantum well (DQW). The effective-mass approximation was employed, and the Schrödinger equation describing the electron motion was solved using the variational method. This study focuses on calculating the binding energy ( E b ) by taking into account the effect of spin polaronic shift. Moreover, we calculated the photoionization cross-section (PCS) considering different polarized light directions, varying well widths ( L w ) , barrier thickness ( L b ) , and different hydrostatic pressure ( P ) values as well as the incorporation of the effect of the non-parabolicity (NP) conduction band and polaronic mass (PM). The results reveal that the overall shape of the PCS depends strongly on the light polarization axis. Additionally, the threshold energy exhibits a blueshift with increasing barrier thickness and hydrostatic pressure, and a redshift with increasing the well width. Semimagnetic double quantum well Spin polaronic shift Binding energy Hydrostatic pressure Non-parabolicity Photoionization cross-section Amri, N. verfasserin aut Nithiananthi, P. verfasserin (orcid)0000-0001-7759-1513 aut Jaouane, M. verfasserin aut El-Bakkari, K. verfasserin (orcid)0000-0003-3649-7373 aut Sali, A. verfasserin (orcid)0000-0003-4153-3404 aut Ed-Dahmouny, A. verfasserin (orcid)0000-0003-4390-853X aut Fakkahi, A. verfasserin (orcid)0000-0003-0025-9066 aut Arraoui, R. verfasserin aut Enthalten in Physica / B Amsterdam : Elsevier, 1988 677 Online-Ressource (DE-627)266015093 (DE-600)1466579-7 (DE-576)074959840 1873-2135 nnns volume:677 GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2088 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.60 Kondensierte Materie: Allgemeines VZ 51.00 Werkstoffkunde: Allgemeines VZ AR 677 |
allfields_unstemmed |
10.1016/j.physb.2024.415717 doi (DE-627)ELV067071953 (ELSEVIER)S0921-4526(24)00058-9 DE-627 ger DE-627 rda eng 530 VZ 33.60 bkl 51.00 bkl Azmi, H. verfasserin (orcid)0009-0002-8967-1603 aut Photoionization cross section in a strained semimagnetic double quantum well under hydrostatic pressure, nonparabolicity and polaronic mass effects 2024 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier In this research, we conducted a numerical analysis on the photoionization cross section (PCS) of a shallow donor impurity confined in a diluted magnetic semiconductor (DMS) C d 1 − x w M n x w T e / C d 1 − x b M n x b T e double quantum well (DQW). The effective-mass approximation was employed, and the Schrödinger equation describing the electron motion was solved using the variational method. This study focuses on calculating the binding energy ( E b ) by taking into account the effect of spin polaronic shift. Moreover, we calculated the photoionization cross-section (PCS) considering different polarized light directions, varying well widths ( L w ) , barrier thickness ( L b ) , and different hydrostatic pressure ( P ) values as well as the incorporation of the effect of the non-parabolicity (NP) conduction band and polaronic mass (PM). The results reveal that the overall shape of the PCS depends strongly on the light polarization axis. Additionally, the threshold energy exhibits a blueshift with increasing barrier thickness and hydrostatic pressure, and a redshift with increasing the well width. Semimagnetic double quantum well Spin polaronic shift Binding energy Hydrostatic pressure Non-parabolicity Photoionization cross-section Amri, N. verfasserin aut Nithiananthi, P. verfasserin (orcid)0000-0001-7759-1513 aut Jaouane, M. verfasserin aut El-Bakkari, K. verfasserin (orcid)0000-0003-3649-7373 aut Sali, A. verfasserin (orcid)0000-0003-4153-3404 aut Ed-Dahmouny, A. verfasserin (orcid)0000-0003-4390-853X aut Fakkahi, A. verfasserin (orcid)0000-0003-0025-9066 aut Arraoui, R. verfasserin aut Enthalten in Physica / B Amsterdam : Elsevier, 1988 677 Online-Ressource (DE-627)266015093 (DE-600)1466579-7 (DE-576)074959840 1873-2135 nnns volume:677 GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2088 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.60 Kondensierte Materie: Allgemeines VZ 51.00 Werkstoffkunde: Allgemeines VZ AR 677 |
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10.1016/j.physb.2024.415717 doi (DE-627)ELV067071953 (ELSEVIER)S0921-4526(24)00058-9 DE-627 ger DE-627 rda eng 530 VZ 33.60 bkl 51.00 bkl Azmi, H. verfasserin (orcid)0009-0002-8967-1603 aut Photoionization cross section in a strained semimagnetic double quantum well under hydrostatic pressure, nonparabolicity and polaronic mass effects 2024 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier In this research, we conducted a numerical analysis on the photoionization cross section (PCS) of a shallow donor impurity confined in a diluted magnetic semiconductor (DMS) C d 1 − x w M n x w T e / C d 1 − x b M n x b T e double quantum well (DQW). The effective-mass approximation was employed, and the Schrödinger equation describing the electron motion was solved using the variational method. This study focuses on calculating the binding energy ( E b ) by taking into account the effect of spin polaronic shift. Moreover, we calculated the photoionization cross-section (PCS) considering different polarized light directions, varying well widths ( L w ) , barrier thickness ( L b ) , and different hydrostatic pressure ( P ) values as well as the incorporation of the effect of the non-parabolicity (NP) conduction band and polaronic mass (PM). The results reveal that the overall shape of the PCS depends strongly on the light polarization axis. Additionally, the threshold energy exhibits a blueshift with increasing barrier thickness and hydrostatic pressure, and a redshift with increasing the well width. Semimagnetic double quantum well Spin polaronic shift Binding energy Hydrostatic pressure Non-parabolicity Photoionization cross-section Amri, N. verfasserin aut Nithiananthi, P. verfasserin (orcid)0000-0001-7759-1513 aut Jaouane, M. verfasserin aut El-Bakkari, K. verfasserin (orcid)0000-0003-3649-7373 aut Sali, A. verfasserin (orcid)0000-0003-4153-3404 aut Ed-Dahmouny, A. verfasserin (orcid)0000-0003-4390-853X aut Fakkahi, A. verfasserin (orcid)0000-0003-0025-9066 aut Arraoui, R. verfasserin aut Enthalten in Physica / B Amsterdam : Elsevier, 1988 677 Online-Ressource (DE-627)266015093 (DE-600)1466579-7 (DE-576)074959840 1873-2135 nnns volume:677 GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2088 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.60 Kondensierte Materie: Allgemeines VZ 51.00 Werkstoffkunde: Allgemeines VZ AR 677 |
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10.1016/j.physb.2024.415717 doi (DE-627)ELV067071953 (ELSEVIER)S0921-4526(24)00058-9 DE-627 ger DE-627 rda eng 530 VZ 33.60 bkl 51.00 bkl Azmi, H. verfasserin (orcid)0009-0002-8967-1603 aut Photoionization cross section in a strained semimagnetic double quantum well under hydrostatic pressure, nonparabolicity and polaronic mass effects 2024 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier In this research, we conducted a numerical analysis on the photoionization cross section (PCS) of a shallow donor impurity confined in a diluted magnetic semiconductor (DMS) C d 1 − x w M n x w T e / C d 1 − x b M n x b T e double quantum well (DQW). The effective-mass approximation was employed, and the Schrödinger equation describing the electron motion was solved using the variational method. This study focuses on calculating the binding energy ( E b ) by taking into account the effect of spin polaronic shift. Moreover, we calculated the photoionization cross-section (PCS) considering different polarized light directions, varying well widths ( L w ) , barrier thickness ( L b ) , and different hydrostatic pressure ( P ) values as well as the incorporation of the effect of the non-parabolicity (NP) conduction band and polaronic mass (PM). The results reveal that the overall shape of the PCS depends strongly on the light polarization axis. Additionally, the threshold energy exhibits a blueshift with increasing barrier thickness and hydrostatic pressure, and a redshift with increasing the well width. Semimagnetic double quantum well Spin polaronic shift Binding energy Hydrostatic pressure Non-parabolicity Photoionization cross-section Amri, N. verfasserin aut Nithiananthi, P. verfasserin (orcid)0000-0001-7759-1513 aut Jaouane, M. verfasserin aut El-Bakkari, K. verfasserin (orcid)0000-0003-3649-7373 aut Sali, A. verfasserin (orcid)0000-0003-4153-3404 aut Ed-Dahmouny, A. verfasserin (orcid)0000-0003-4390-853X aut Fakkahi, A. verfasserin (orcid)0000-0003-0025-9066 aut Arraoui, R. verfasserin aut Enthalten in Physica / B Amsterdam : Elsevier, 1988 677 Online-Ressource (DE-627)266015093 (DE-600)1466579-7 (DE-576)074959840 1873-2135 nnns volume:677 GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2088 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.60 Kondensierte Materie: Allgemeines VZ 51.00 Werkstoffkunde: Allgemeines VZ AR 677 |
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530 VZ 33.60 bkl 51.00 bkl Photoionization cross section in a strained semimagnetic double quantum well under hydrostatic pressure, nonparabolicity and polaronic mass effects Semimagnetic double quantum well Spin polaronic shift Binding energy Hydrostatic pressure Non-parabolicity Photoionization cross-section |
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Photoionization cross section in a strained semimagnetic double quantum well under hydrostatic pressure, nonparabolicity and polaronic mass effects |
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photoionization cross section in a strained semimagnetic double quantum well under hydrostatic pressure, nonparabolicity and polaronic mass effects |
title_auth |
Photoionization cross section in a strained semimagnetic double quantum well under hydrostatic pressure, nonparabolicity and polaronic mass effects |
abstract |
In this research, we conducted a numerical analysis on the photoionization cross section (PCS) of a shallow donor impurity confined in a diluted magnetic semiconductor (DMS) C d 1 − x w M n x w T e / C d 1 − x b M n x b T e double quantum well (DQW). The effective-mass approximation was employed, and the Schrödinger equation describing the electron motion was solved using the variational method. This study focuses on calculating the binding energy ( E b ) by taking into account the effect of spin polaronic shift. Moreover, we calculated the photoionization cross-section (PCS) considering different polarized light directions, varying well widths ( L w ) , barrier thickness ( L b ) , and different hydrostatic pressure ( P ) values as well as the incorporation of the effect of the non-parabolicity (NP) conduction band and polaronic mass (PM). The results reveal that the overall shape of the PCS depends strongly on the light polarization axis. Additionally, the threshold energy exhibits a blueshift with increasing barrier thickness and hydrostatic pressure, and a redshift with increasing the well width. |
abstractGer |
In this research, we conducted a numerical analysis on the photoionization cross section (PCS) of a shallow donor impurity confined in a diluted magnetic semiconductor (DMS) C d 1 − x w M n x w T e / C d 1 − x b M n x b T e double quantum well (DQW). The effective-mass approximation was employed, and the Schrödinger equation describing the electron motion was solved using the variational method. This study focuses on calculating the binding energy ( E b ) by taking into account the effect of spin polaronic shift. Moreover, we calculated the photoionization cross-section (PCS) considering different polarized light directions, varying well widths ( L w ) , barrier thickness ( L b ) , and different hydrostatic pressure ( P ) values as well as the incorporation of the effect of the non-parabolicity (NP) conduction band and polaronic mass (PM). The results reveal that the overall shape of the PCS depends strongly on the light polarization axis. Additionally, the threshold energy exhibits a blueshift with increasing barrier thickness and hydrostatic pressure, and a redshift with increasing the well width. |
abstract_unstemmed |
In this research, we conducted a numerical analysis on the photoionization cross section (PCS) of a shallow donor impurity confined in a diluted magnetic semiconductor (DMS) C d 1 − x w M n x w T e / C d 1 − x b M n x b T e double quantum well (DQW). The effective-mass approximation was employed, and the Schrödinger equation describing the electron motion was solved using the variational method. This study focuses on calculating the binding energy ( E b ) by taking into account the effect of spin polaronic shift. Moreover, we calculated the photoionization cross-section (PCS) considering different polarized light directions, varying well widths ( L w ) , barrier thickness ( L b ) , and different hydrostatic pressure ( P ) values as well as the incorporation of the effect of the non-parabolicity (NP) conduction band and polaronic mass (PM). The results reveal that the overall shape of the PCS depends strongly on the light polarization axis. Additionally, the threshold energy exhibits a blueshift with increasing barrier thickness and hydrostatic pressure, and a redshift with increasing the well width. |
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title_short |
Photoionization cross section in a strained semimagnetic double quantum well under hydrostatic pressure, nonparabolicity and polaronic mass effects |
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Amri, N. Nithiananthi, P. Jaouane, M. El-Bakkari, K. Sali, A. Ed-Dahmouny, A. Fakkahi, A. Arraoui, R. |
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score |
7.399315 |