BCS–BEC crossover in cold atomic and in nuclear systems
We review the BCS (Bardeen–Cooper–Schrieffer)–BEC (Bose–Einstein condensation) crossover phenomenon discussed in an ultracold Fermi atomic gas and a neutron superfluid in the low-density crust regime of a neutron star. A purpose of this paper is to show that these two very different atomic and nucle...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Ohashi, Y. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2020transfer abstract |
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| Übergeordnetes Werk: |
Enthalten in: Novel insights into an “old” phenomenon: the no reflow - Durante, Alessandro ELSEVIER, 2015transfer abstract, Oxford [u.a.] |
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| Übergeordnetes Werk: |
volume:111 ; year:2020 ; pages:0 |
| Links: |
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| DOI / URN: |
10.1016/j.ppnp.2019.103739 |
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| 520 | |a We review the BCS (Bardeen–Cooper–Schrieffer)–BEC (Bose–Einstein condensation) crossover phenomenon discussed in an ultracold Fermi atomic gas and a neutron superfluid in the low-density crust regime of a neutron star. A purpose of this paper is to show that these two very different atomic and nuclear systems can be closely related to each other from the viewpoint of this quantum many-body phenomenon. We explain how the BCS–BEC crossover is realized in the former atomic system by using the novel pairing mechanism called Feshbach resonance. We present a simple explanation for this crossover phenomenon to grasp the essence, as well as detailed microscopic theories that can cover the entire BCS–BEC crossover region. In the latter, we point out that the ordinary BCS theory already has the ability to describe the BCS–BEC crossover at T = 0 . At finite temperatures T > 0 , however, we need to go beyond this mean-field theory. Besides general aspects of the BCS–BEC crossover phenomenon, we also pick up special topics peculiar to each atomic gas and neutron fluid. The first one is the pseudogap phenomenon in the normal state of a Fermi atomic gas. The second one is the problem of non-zero effective range in an s -wave neutron superfluid. | ||
| 520 | |a We review the BCS (Bardeen–Cooper–Schrieffer)–BEC (Bose–Einstein condensation) crossover phenomenon discussed in an ultracold Fermi atomic gas and a neutron superfluid in the low-density crust regime of a neutron star. A purpose of this paper is to show that these two very different atomic and nuclear systems can be closely related to each other from the viewpoint of this quantum many-body phenomenon. We explain how the BCS–BEC crossover is realized in the former atomic system by using the novel pairing mechanism called Feshbach resonance. We present a simple explanation for this crossover phenomenon to grasp the essence, as well as detailed microscopic theories that can cover the entire BCS–BEC crossover region. In the latter, we point out that the ordinary BCS theory already has the ability to describe the BCS–BEC crossover at T = 0 . At finite temperatures T > 0 , however, we need to go beyond this mean-field theory. Besides general aspects of the BCS–BEC crossover phenomenon, we also pick up special topics peculiar to each atomic gas and neutron fluid. The first one is the pseudogap phenomenon in the normal state of a Fermi atomic gas. The second one is the problem of non-zero effective range in an s -wave neutron superfluid. | ||
| 650 | 7 | |a Neutron star |2 Elsevier | |
| 650 | 7 | |a Fermi superfluids |2 Elsevier | |
| 650 | 7 | |a Bose–Einstein condensation |2 Elsevier | |
| 650 | 7 | |a BCS-BEC crossover |2 Elsevier | |
| 650 | 7 | |a Ultracold Fermi gas |2 Elsevier | |
| 650 | 7 | |a Strong-coupling phenomenon |2 Elsevier | |
| 700 | 1 | |a Tajima, H. |4 oth | |
| 700 | 1 | |a van Wyk, P. |4 oth | |
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10.1016/j.ppnp.2019.103739 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001046.pica (DE-627)ELV049330675 (ELSEVIER)S0146-6410(19)30074-2 DE-627 ger DE-627 rakwb eng 610 VZ 630 640 610 VZ Ohashi, Y. verfasserin aut BCS–BEC crossover in cold atomic and in nuclear systems 2020transfer abstract nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We review the BCS (Bardeen–Cooper–Schrieffer)–BEC (Bose–Einstein condensation) crossover phenomenon discussed in an ultracold Fermi atomic gas and a neutron superfluid in the low-density crust regime of a neutron star. A purpose of this paper is to show that these two very different atomic and nuclear systems can be closely related to each other from the viewpoint of this quantum many-body phenomenon. We explain how the BCS–BEC crossover is realized in the former atomic system by using the novel pairing mechanism called Feshbach resonance. We present a simple explanation for this crossover phenomenon to grasp the essence, as well as detailed microscopic theories that can cover the entire BCS–BEC crossover region. In the latter, we point out that the ordinary BCS theory already has the ability to describe the BCS–BEC crossover at T = 0 . At finite temperatures T > 0 , however, we need to go beyond this mean-field theory. Besides general aspects of the BCS–BEC crossover phenomenon, we also pick up special topics peculiar to each atomic gas and neutron fluid. The first one is the pseudogap phenomenon in the normal state of a Fermi atomic gas. The second one is the problem of non-zero effective range in an s -wave neutron superfluid. We review the BCS (Bardeen–Cooper–Schrieffer)–BEC (Bose–Einstein condensation) crossover phenomenon discussed in an ultracold Fermi atomic gas and a neutron superfluid in the low-density crust regime of a neutron star. A purpose of this paper is to show that these two very different atomic and nuclear systems can be closely related to each other from the viewpoint of this quantum many-body phenomenon. We explain how the BCS–BEC crossover is realized in the former atomic system by using the novel pairing mechanism called Feshbach resonance. We present a simple explanation for this crossover phenomenon to grasp the essence, as well as detailed microscopic theories that can cover the entire BCS–BEC crossover region. In the latter, we point out that the ordinary BCS theory already has the ability to describe the BCS–BEC crossover at T = 0 . At finite temperatures T > 0 , however, we need to go beyond this mean-field theory. Besides general aspects of the BCS–BEC crossover phenomenon, we also pick up special topics peculiar to each atomic gas and neutron fluid. The first one is the pseudogap phenomenon in the normal state of a Fermi atomic gas. The second one is the problem of non-zero effective range in an s -wave neutron superfluid. Neutron star Elsevier Fermi superfluids Elsevier Bose–Einstein condensation Elsevier BCS-BEC crossover Elsevier Ultracold Fermi gas Elsevier Strong-coupling phenomenon Elsevier Tajima, H. oth van Wyk, P. oth Enthalten in Pergamon Press Durante, Alessandro ELSEVIER Novel insights into an “old” phenomenon: the no reflow 2015transfer abstract Oxford [u.a.] (DE-627)ELV012849391 volume:111 year:2020 pages:0 https://doi.org/10.1016/j.ppnp.2019.103739 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_21 GBV_ILN_39 GBV_ILN_50 GBV_ILN_60 GBV_ILN_2001 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2010 GBV_ILN_2015 GBV_ILN_2056 GBV_ILN_2280 AR 111 2020 0 |
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10.1016/j.ppnp.2019.103739 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001046.pica (DE-627)ELV049330675 (ELSEVIER)S0146-6410(19)30074-2 DE-627 ger DE-627 rakwb eng 610 VZ 630 640 610 VZ Ohashi, Y. verfasserin aut BCS–BEC crossover in cold atomic and in nuclear systems 2020transfer abstract nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We review the BCS (Bardeen–Cooper–Schrieffer)–BEC (Bose–Einstein condensation) crossover phenomenon discussed in an ultracold Fermi atomic gas and a neutron superfluid in the low-density crust regime of a neutron star. A purpose of this paper is to show that these two very different atomic and nuclear systems can be closely related to each other from the viewpoint of this quantum many-body phenomenon. We explain how the BCS–BEC crossover is realized in the former atomic system by using the novel pairing mechanism called Feshbach resonance. We present a simple explanation for this crossover phenomenon to grasp the essence, as well as detailed microscopic theories that can cover the entire BCS–BEC crossover region. In the latter, we point out that the ordinary BCS theory already has the ability to describe the BCS–BEC crossover at T = 0 . At finite temperatures T > 0 , however, we need to go beyond this mean-field theory. Besides general aspects of the BCS–BEC crossover phenomenon, we also pick up special topics peculiar to each atomic gas and neutron fluid. The first one is the pseudogap phenomenon in the normal state of a Fermi atomic gas. The second one is the problem of non-zero effective range in an s -wave neutron superfluid. We review the BCS (Bardeen–Cooper–Schrieffer)–BEC (Bose–Einstein condensation) crossover phenomenon discussed in an ultracold Fermi atomic gas and a neutron superfluid in the low-density crust regime of a neutron star. A purpose of this paper is to show that these two very different atomic and nuclear systems can be closely related to each other from the viewpoint of this quantum many-body phenomenon. We explain how the BCS–BEC crossover is realized in the former atomic system by using the novel pairing mechanism called Feshbach resonance. We present a simple explanation for this crossover phenomenon to grasp the essence, as well as detailed microscopic theories that can cover the entire BCS–BEC crossover region. In the latter, we point out that the ordinary BCS theory already has the ability to describe the BCS–BEC crossover at T = 0 . At finite temperatures T > 0 , however, we need to go beyond this mean-field theory. Besides general aspects of the BCS–BEC crossover phenomenon, we also pick up special topics peculiar to each atomic gas and neutron fluid. The first one is the pseudogap phenomenon in the normal state of a Fermi atomic gas. The second one is the problem of non-zero effective range in an s -wave neutron superfluid. Neutron star Elsevier Fermi superfluids Elsevier Bose–Einstein condensation Elsevier BCS-BEC crossover Elsevier Ultracold Fermi gas Elsevier Strong-coupling phenomenon Elsevier Tajima, H. oth van Wyk, P. oth Enthalten in Pergamon Press Durante, Alessandro ELSEVIER Novel insights into an “old” phenomenon: the no reflow 2015transfer abstract Oxford [u.a.] (DE-627)ELV012849391 volume:111 year:2020 pages:0 https://doi.org/10.1016/j.ppnp.2019.103739 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_21 GBV_ILN_39 GBV_ILN_50 GBV_ILN_60 GBV_ILN_2001 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2010 GBV_ILN_2015 GBV_ILN_2056 GBV_ILN_2280 AR 111 2020 0 |
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10.1016/j.ppnp.2019.103739 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001046.pica (DE-627)ELV049330675 (ELSEVIER)S0146-6410(19)30074-2 DE-627 ger DE-627 rakwb eng 610 VZ 630 640 610 VZ Ohashi, Y. verfasserin aut BCS–BEC crossover in cold atomic and in nuclear systems 2020transfer abstract nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We review the BCS (Bardeen–Cooper–Schrieffer)–BEC (Bose–Einstein condensation) crossover phenomenon discussed in an ultracold Fermi atomic gas and a neutron superfluid in the low-density crust regime of a neutron star. A purpose of this paper is to show that these two very different atomic and nuclear systems can be closely related to each other from the viewpoint of this quantum many-body phenomenon. We explain how the BCS–BEC crossover is realized in the former atomic system by using the novel pairing mechanism called Feshbach resonance. We present a simple explanation for this crossover phenomenon to grasp the essence, as well as detailed microscopic theories that can cover the entire BCS–BEC crossover region. In the latter, we point out that the ordinary BCS theory already has the ability to describe the BCS–BEC crossover at T = 0 . At finite temperatures T > 0 , however, we need to go beyond this mean-field theory. Besides general aspects of the BCS–BEC crossover phenomenon, we also pick up special topics peculiar to each atomic gas and neutron fluid. The first one is the pseudogap phenomenon in the normal state of a Fermi atomic gas. The second one is the problem of non-zero effective range in an s -wave neutron superfluid. We review the BCS (Bardeen–Cooper–Schrieffer)–BEC (Bose–Einstein condensation) crossover phenomenon discussed in an ultracold Fermi atomic gas and a neutron superfluid in the low-density crust regime of a neutron star. A purpose of this paper is to show that these two very different atomic and nuclear systems can be closely related to each other from the viewpoint of this quantum many-body phenomenon. We explain how the BCS–BEC crossover is realized in the former atomic system by using the novel pairing mechanism called Feshbach resonance. We present a simple explanation for this crossover phenomenon to grasp the essence, as well as detailed microscopic theories that can cover the entire BCS–BEC crossover region. In the latter, we point out that the ordinary BCS theory already has the ability to describe the BCS–BEC crossover at T = 0 . At finite temperatures T > 0 , however, we need to go beyond this mean-field theory. Besides general aspects of the BCS–BEC crossover phenomenon, we also pick up special topics peculiar to each atomic gas and neutron fluid. The first one is the pseudogap phenomenon in the normal state of a Fermi atomic gas. The second one is the problem of non-zero effective range in an s -wave neutron superfluid. Neutron star Elsevier Fermi superfluids Elsevier Bose–Einstein condensation Elsevier BCS-BEC crossover Elsevier Ultracold Fermi gas Elsevier Strong-coupling phenomenon Elsevier Tajima, H. oth van Wyk, P. oth Enthalten in Pergamon Press Durante, Alessandro ELSEVIER Novel insights into an “old” phenomenon: the no reflow 2015transfer abstract Oxford [u.a.] (DE-627)ELV012849391 volume:111 year:2020 pages:0 https://doi.org/10.1016/j.ppnp.2019.103739 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_21 GBV_ILN_39 GBV_ILN_50 GBV_ILN_60 GBV_ILN_2001 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2010 GBV_ILN_2015 GBV_ILN_2056 GBV_ILN_2280 AR 111 2020 0 |
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10.1016/j.ppnp.2019.103739 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001046.pica (DE-627)ELV049330675 (ELSEVIER)S0146-6410(19)30074-2 DE-627 ger DE-627 rakwb eng 610 VZ 630 640 610 VZ Ohashi, Y. verfasserin aut BCS–BEC crossover in cold atomic and in nuclear systems 2020transfer abstract nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We review the BCS (Bardeen–Cooper–Schrieffer)–BEC (Bose–Einstein condensation) crossover phenomenon discussed in an ultracold Fermi atomic gas and a neutron superfluid in the low-density crust regime of a neutron star. A purpose of this paper is to show that these two very different atomic and nuclear systems can be closely related to each other from the viewpoint of this quantum many-body phenomenon. We explain how the BCS–BEC crossover is realized in the former atomic system by using the novel pairing mechanism called Feshbach resonance. We present a simple explanation for this crossover phenomenon to grasp the essence, as well as detailed microscopic theories that can cover the entire BCS–BEC crossover region. In the latter, we point out that the ordinary BCS theory already has the ability to describe the BCS–BEC crossover at T = 0 . At finite temperatures T > 0 , however, we need to go beyond this mean-field theory. Besides general aspects of the BCS–BEC crossover phenomenon, we also pick up special topics peculiar to each atomic gas and neutron fluid. The first one is the pseudogap phenomenon in the normal state of a Fermi atomic gas. The second one is the problem of non-zero effective range in an s -wave neutron superfluid. We review the BCS (Bardeen–Cooper–Schrieffer)–BEC (Bose–Einstein condensation) crossover phenomenon discussed in an ultracold Fermi atomic gas and a neutron superfluid in the low-density crust regime of a neutron star. A purpose of this paper is to show that these two very different atomic and nuclear systems can be closely related to each other from the viewpoint of this quantum many-body phenomenon. We explain how the BCS–BEC crossover is realized in the former atomic system by using the novel pairing mechanism called Feshbach resonance. We present a simple explanation for this crossover phenomenon to grasp the essence, as well as detailed microscopic theories that can cover the entire BCS–BEC crossover region. In the latter, we point out that the ordinary BCS theory already has the ability to describe the BCS–BEC crossover at T = 0 . At finite temperatures T > 0 , however, we need to go beyond this mean-field theory. Besides general aspects of the BCS–BEC crossover phenomenon, we also pick up special topics peculiar to each atomic gas and neutron fluid. The first one is the pseudogap phenomenon in the normal state of a Fermi atomic gas. The second one is the problem of non-zero effective range in an s -wave neutron superfluid. Neutron star Elsevier Fermi superfluids Elsevier Bose–Einstein condensation Elsevier BCS-BEC crossover Elsevier Ultracold Fermi gas Elsevier Strong-coupling phenomenon Elsevier Tajima, H. oth van Wyk, P. oth Enthalten in Pergamon Press Durante, Alessandro ELSEVIER Novel insights into an “old” phenomenon: the no reflow 2015transfer abstract Oxford [u.a.] (DE-627)ELV012849391 volume:111 year:2020 pages:0 https://doi.org/10.1016/j.ppnp.2019.103739 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_21 GBV_ILN_39 GBV_ILN_50 GBV_ILN_60 GBV_ILN_2001 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2010 GBV_ILN_2015 GBV_ILN_2056 GBV_ILN_2280 AR 111 2020 0 |
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10.1016/j.ppnp.2019.103739 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001046.pica (DE-627)ELV049330675 (ELSEVIER)S0146-6410(19)30074-2 DE-627 ger DE-627 rakwb eng 610 VZ 630 640 610 VZ Ohashi, Y. verfasserin aut BCS–BEC crossover in cold atomic and in nuclear systems 2020transfer abstract nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We review the BCS (Bardeen–Cooper–Schrieffer)–BEC (Bose–Einstein condensation) crossover phenomenon discussed in an ultracold Fermi atomic gas and a neutron superfluid in the low-density crust regime of a neutron star. A purpose of this paper is to show that these two very different atomic and nuclear systems can be closely related to each other from the viewpoint of this quantum many-body phenomenon. We explain how the BCS–BEC crossover is realized in the former atomic system by using the novel pairing mechanism called Feshbach resonance. We present a simple explanation for this crossover phenomenon to grasp the essence, as well as detailed microscopic theories that can cover the entire BCS–BEC crossover region. In the latter, we point out that the ordinary BCS theory already has the ability to describe the BCS–BEC crossover at T = 0 . At finite temperatures T > 0 , however, we need to go beyond this mean-field theory. Besides general aspects of the BCS–BEC crossover phenomenon, we also pick up special topics peculiar to each atomic gas and neutron fluid. The first one is the pseudogap phenomenon in the normal state of a Fermi atomic gas. The second one is the problem of non-zero effective range in an s -wave neutron superfluid. We review the BCS (Bardeen–Cooper–Schrieffer)–BEC (Bose–Einstein condensation) crossover phenomenon discussed in an ultracold Fermi atomic gas and a neutron superfluid in the low-density crust regime of a neutron star. A purpose of this paper is to show that these two very different atomic and nuclear systems can be closely related to each other from the viewpoint of this quantum many-body phenomenon. We explain how the BCS–BEC crossover is realized in the former atomic system by using the novel pairing mechanism called Feshbach resonance. We present a simple explanation for this crossover phenomenon to grasp the essence, as well as detailed microscopic theories that can cover the entire BCS–BEC crossover region. In the latter, we point out that the ordinary BCS theory already has the ability to describe the BCS–BEC crossover at T = 0 . At finite temperatures T > 0 , however, we need to go beyond this mean-field theory. Besides general aspects of the BCS–BEC crossover phenomenon, we also pick up special topics peculiar to each atomic gas and neutron fluid. The first one is the pseudogap phenomenon in the normal state of a Fermi atomic gas. The second one is the problem of non-zero effective range in an s -wave neutron superfluid. Neutron star Elsevier Fermi superfluids Elsevier Bose–Einstein condensation Elsevier BCS-BEC crossover Elsevier Ultracold Fermi gas Elsevier Strong-coupling phenomenon Elsevier Tajima, H. oth van Wyk, P. oth Enthalten in Pergamon Press Durante, Alessandro ELSEVIER Novel insights into an “old” phenomenon: the no reflow 2015transfer abstract Oxford [u.a.] (DE-627)ELV012849391 volume:111 year:2020 pages:0 https://doi.org/10.1016/j.ppnp.2019.103739 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_21 GBV_ILN_39 GBV_ILN_50 GBV_ILN_60 GBV_ILN_2001 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2010 GBV_ILN_2015 GBV_ILN_2056 GBV_ILN_2280 AR 111 2020 0 |
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BCS–BEC crossover in cold atomic and in nuclear systems |
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We review the BCS (Bardeen–Cooper–Schrieffer)–BEC (Bose–Einstein condensation) crossover phenomenon discussed in an ultracold Fermi atomic gas and a neutron superfluid in the low-density crust regime of a neutron star. A purpose of this paper is to show that these two very different atomic and nuclear systems can be closely related to each other from the viewpoint of this quantum many-body phenomenon. We explain how the BCS–BEC crossover is realized in the former atomic system by using the novel pairing mechanism called Feshbach resonance. We present a simple explanation for this crossover phenomenon to grasp the essence, as well as detailed microscopic theories that can cover the entire BCS–BEC crossover region. In the latter, we point out that the ordinary BCS theory already has the ability to describe the BCS–BEC crossover at T = 0 . At finite temperatures T > 0 , however, we need to go beyond this mean-field theory. Besides general aspects of the BCS–BEC crossover phenomenon, we also pick up special topics peculiar to each atomic gas and neutron fluid. The first one is the pseudogap phenomenon in the normal state of a Fermi atomic gas. The second one is the problem of non-zero effective range in an s -wave neutron superfluid. |
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We review the BCS (Bardeen–Cooper–Schrieffer)–BEC (Bose–Einstein condensation) crossover phenomenon discussed in an ultracold Fermi atomic gas and a neutron superfluid in the low-density crust regime of a neutron star. A purpose of this paper is to show that these two very different atomic and nuclear systems can be closely related to each other from the viewpoint of this quantum many-body phenomenon. We explain how the BCS–BEC crossover is realized in the former atomic system by using the novel pairing mechanism called Feshbach resonance. We present a simple explanation for this crossover phenomenon to grasp the essence, as well as detailed microscopic theories that can cover the entire BCS–BEC crossover region. In the latter, we point out that the ordinary BCS theory already has the ability to describe the BCS–BEC crossover at T = 0 . At finite temperatures T > 0 , however, we need to go beyond this mean-field theory. Besides general aspects of the BCS–BEC crossover phenomenon, we also pick up special topics peculiar to each atomic gas and neutron fluid. The first one is the pseudogap phenomenon in the normal state of a Fermi atomic gas. The second one is the problem of non-zero effective range in an s -wave neutron superfluid. |
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We review the BCS (Bardeen–Cooper–Schrieffer)–BEC (Bose–Einstein condensation) crossover phenomenon discussed in an ultracold Fermi atomic gas and a neutron superfluid in the low-density crust regime of a neutron star. A purpose of this paper is to show that these two very different atomic and nuclear systems can be closely related to each other from the viewpoint of this quantum many-body phenomenon. We explain how the BCS–BEC crossover is realized in the former atomic system by using the novel pairing mechanism called Feshbach resonance. We present a simple explanation for this crossover phenomenon to grasp the essence, as well as detailed microscopic theories that can cover the entire BCS–BEC crossover region. In the latter, we point out that the ordinary BCS theory already has the ability to describe the BCS–BEC crossover at T = 0 . At finite temperatures T > 0 , however, we need to go beyond this mean-field theory. Besides general aspects of the BCS–BEC crossover phenomenon, we also pick up special topics peculiar to each atomic gas and neutron fluid. The first one is the pseudogap phenomenon in the normal state of a Fermi atomic gas. The second one is the problem of non-zero effective range in an s -wave neutron superfluid. |
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