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Even the elusive neutrinos are trapped in matter, albeit transiently, in several astrophysical circumstances. Their interactions with the ambient matter not only reveal the properties of such exotic matter itself, but also shed light on the…

天体物理学 · 物理学 2009-11-06 M. Prakash , J. M. Lattimer , R. F. Sawyer , R. R. Volkas

Phonon, the collective excitation of lattice vibration in the crystal, has been put forward as a means to search for light dark matter. However, the accurate modeling of the multi-phonon production process is challenging in theory. The…

高能物理 - 唯象学 · 物理学 2024-12-25 Jun Guo , Lei Wu , Bin Zhu

Solar neutrino studies triggered and largely motivated the major developments in neutrino physics in the last 50 years. Theory of neutrino propagation in different media with matter and fields has been elaborated. It includes oscillations…

高能物理 - 唯象学 · 物理学 2017-01-18 Michele Maltoni , Alexei Yu. Smirnov

The anomalously slow rotation of the solar core is just one from a remarkable lists of fundamental indications showing that the solar core is somehow coupled to the surface activity cycle. On the other hand, the atmospheric, LSND and solar…

天体物理学 · 物理学 2007-05-23 Attila Grandpierre

A number of characteristics of the new fundamental interaction are described. The interaction is carried by a massless pseudoscalar boson and extends to at least the electron neutrino, proton, and neutron. A substantiation of the existence…

高能物理 - 唯象学 · 物理学 2021-06-22 L. M. Slad

As dark matter appears to comprise most of the Galactic mass, some of it may accumulate in the cores of stars, thereby making the Sun a laboratory for constraining various dark matter theories. We consider the effects on the solar structure…

太阳与恒星天体物理 · 物理学 2025-05-06 Earl Patrick Bellinger , Matt E. Caplan

We discuss the relation between the observed CC, ES, and NC fluxes with the flavor fractional content of the solar neutrino flux seen by SNO. By using existing estimates of the cross sections for the charged and neutral current reactions…

高能物理 - 唯象学 · 物理学 2009-11-07 A. Aguilar-Arevalo , J. C. Dolivo

The next generation of solar neutrino detectors will provide a precision measure of the $^8$B electron-neutrino spectrum in the energy range from 1-15 MeV. Although the neutrino spectrum emitted by $^8$B $\beta$-decay reactions in the Sun's…

高能物理 - 唯象学 · 物理学 2019-01-23 Ilídio Lopes , Joseph Silk

Models in which the "dark" halo particles have mutual and potentially also appreciable nuclear interactions have been considered by various authors. In this note we briefly point out strategies for a most sensitive search for these…

高能物理 - 唯象学 · 物理学 2007-05-23 Itzhak Goldman , Shmuel Nussinov

We review the discovery of the neutrino and outline the history of neutrino physics. Many interesting phenomena involving the neutrino are exhibited. We also discuss the long-standing solar neutrino puzzle and the properties of the neutrino…

综合物理 · 物理学 2014-10-20 Y. H. Yuan

What if the dark matter-nucleon scattering cross section is too small to be detected by direct detection experiments? It is well known in the literature that some interactions lead to dark matter-nucleon scattering cross sections that can…

高能物理 - 唯象学 · 物理学 2021-10-19 Tarak Nath Maity , Farinaldo S Queiroz

We point out that solar neutrino oscillations with large mixing angle as evidenced in current solar neutrino data have a strong impact on strategies for diagnosing collapse-driven supernova (SN) through neutrino observations. Such…

高能物理 - 唯象学 · 物理学 2009-09-17 H. Minakata , H. Nunokawa , R. Tomas , J. W. F. Valle

We discuss various aspects of the solar neutrino spectrum distortion and time variations of fluxes. (i) Oscillations of neutrinos which cross the mantle and the core of the Earth can be parametrically enhanced. The parametric effect gives…

高能物理 - 唯象学 · 物理学 2009-10-31 A. Yu. Smirnov

The ultra-light dark matter is a new class of dark matter candidates. Unlike traditional dark matter particle candidates, the ultra-light dark matter behaves like a classical field, which saturates the entire Milky Way galaxy with a…

高能物理 - 唯象学 · 物理学 2024-02-29 Carlos A. Argüelles , Kareem Farrag , Teppei Katori

Neutrino interactions with matter play an important role in determining the nucleosynthesis outcome in explosive astrophysical environments such as core-collapse supernovae or mergers of compact objects. In this article, we first discuss…

高能天体物理现象 · 物理学 2016-03-16 Meng-Ru Wu , Gabriel Martinez-Pinedo , Yong-Zhong Qian

Regarding the proximity of dark energy scale and neutrino mass, one can get new insight into the probe signatures of vector field dark energy component on neutrino flavor conversion. A vector field is assumed to be conformally coupled to…

高能物理 - 唯象学 · 物理学 2024-11-19 H. Yazdani Ahmadabadi , H. Mohseni Sadjadi

The possibility that the Gallium data effectively indicates a time modulation of the solar active neutrino flux in possible connection to solar activity is examined on the light of spin flavour precession to sterile neutrinos as a…

高能物理 - 唯象学 · 物理学 2009-11-11 Bhag C. Chauhan , Joao Pulido , R. S. Raghavan

Current problems with the solar model may be alleviated if a significant amount of dark matter from the galactic halo is captured in the Sun. We discuss the capture process in the case where the dark matter is a Dirac fermion and the…

高能物理 - 唯象学 · 物理学 2015-08-20 Mattias Blennow , Stefan Clementz

Recently, stellar collapse involving black hole formation from massive stars is suggested to emit enormous fluxes of neutrinos on par with ordinary core-collapse supernovae. We investigate their detectability for the currently operating…

天体物理学 · 物理学 2014-11-18 Ken'ichiro Nakazato , Kohsuke Sumiyoshi , Hideyuki Suzuki , Shoichi Yamada

We present updated standard solar models (SSMs) that incorporate the latest results for nuclear fusion rates, recently published. We show helioseismic results for high and low metallicity compositions and also for an alternative set of…

太阳与恒星天体物理 · 物理学 2011-09-14 Aldo Serenelli