Mu problem (original) (raw)
뮤(μ) 문제는 초대칭 표준모형에서 발생하는 문제로, 뮤 파라메터의 값이 전약력깨짐을 설명하기 위해 자연스럽게 힉스 보손의 진공 기댓값과 비슷한 값(약 1 TeV)이 되는지를 설명하는 문제다. 초대칭 깨짐을 설명하는 자연스러운 크기인 플랑크 상수나, 중간 스케일 값보다 훨씬 작은 힉스 보손 진공 기댓값을 자연스럽게 설명하지 못하기 때문에 일종의 위계 문제라 할 수 있다.
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| dbo:abstract | In theoretical physics, the μ problem is a problem of supersymmetric theories, concerned with understanding the parameters of the theory. The supersymmetric Higgs mass parameter μ appears as the following term in the superpotential: μHuHd. It is necessary to provide a mass for the fermionic superpartners of the Higgs bosons, i.e. the higgsinos, and it enters as well the scalar potential of the Higgs bosons. To ensure that Hu and Hd get a non-zero vacuum expectation value after electroweak symmetry breaking, μ should be of the order of magnitude of the electroweak scale, many orders of magnitude smaller than the Planck scale, which is the natural cutoff scale. This brings about a problem of naturalness: why is that scale so much smaller than the cutoff scale? And why, if the μ term in the superpotential has different physical origins, do the corresponding scale happen to fall so close to each other? Before LHC, it was thought that the soft supersymmetry breaking terms should also be of the same order of magnitude as the electroweak scale. This was negated by the Higgs mass measurements and limits on supersymmetry models. One proposed solution, known as the Giudice–Masiero mechanism, is that this term does not appear explicitly in the Lagrangian, because it violates some global symmetry, and can therefore be created only via spontaneous breaking of this symmetry. This is proposed to happen together with F-term supersymmetry breaking, with a spurious field X that parameterizes the hidden supersymmetry-breaking sector of the theory (meaning that FX is the non-zero F-term). Let us assume that the Kahler potential includes a term of the form times some dimensionless coefficient which is naturally of order one where Mpl is Planck mass. Then as supersymmetry breaks, FX gets a non-zero vacuum expectation value ⟨FX⟩ and the following effective term is added to the superpotential: , which gives a measured . On the other hand, soft supersymmetry breaking terms are similarly created and also have a natural scale of . (en) 뮤(μ) 문제는 초대칭 표준모형에서 발생하는 문제로, 뮤 파라메터의 값이 전약력깨짐을 설명하기 위해 자연스럽게 힉스 보손의 진공 기댓값과 비슷한 값(약 1 TeV)이 되는지를 설명하는 문제다. 초대칭 깨짐을 설명하는 자연스러운 크기인 플랑크 상수나, 중간 스케일 값보다 훨씬 작은 힉스 보손 진공 기댓값을 자연스럽게 설명하지 못하기 때문에 일종의 위계 문제라 할 수 있다. (ko) |
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| rdfs:comment | 뮤(μ) 문제는 초대칭 표준모형에서 발생하는 문제로, 뮤 파라메터의 값이 전약력깨짐을 설명하기 위해 자연스럽게 힉스 보손의 진공 기댓값과 비슷한 값(약 1 TeV)이 되는지를 설명하는 문제다. 초대칭 깨짐을 설명하는 자연스러운 크기인 플랑크 상수나, 중간 스케일 값보다 훨씬 작은 힉스 보손 진공 기댓값을 자연스럽게 설명하지 못하기 때문에 일종의 위계 문제라 할 수 있다. (ko) In theoretical physics, the μ problem is a problem of supersymmetric theories, concerned with understanding the parameters of the theory. The supersymmetric Higgs mass parameter μ appears as the following term in the superpotential: μHuHd. It is necessary to provide a mass for the fermionic superpartners of the Higgs bosons, i.e. the higgsinos, and it enters as well the scalar potential of the Higgs bosons. To ensure that Hu and Hd get a non-zero vacuum expectation value after electroweak symmetry breaking, μ should be of the order of magnitude of the electroweak scale, many orders of magnitude smaller than the Planck scale, which is the natural cutoff scale. This brings about a problem of naturalness: why is that scale so much smaller than the cutoff scale? And why, if the μ term in the s (en) |
| rdfs:label | Mu problem (en) 뮤 문제 (ko) |
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