English
Related papers

Related papers: Dense Cold Nuclear Matter Study with Cumulative Tr…

200 papers

Muon colliders and neutrino factories are attractive options for achieving the highest lepton-antilepton collision energies and the most precise measurements of the parameters of the neutrino mixing matrix. The performance and cost of these…

Accelerator Physics · Physics 2007-05-23 Daniel M. Kaplan

In the following we stress the advantages of the NICA research programme in the context of studying the spectator-induced electromagnetic phenomena present in proton-nucleus and heavy ion collisions. We point at the specific interest of…

Nuclear Theory · Physics 2013-01-23 Andrzej Rybicki , Antoni Szczurek , Mariola Klusek-Gawenda , Iwona Sputowska

If the cosmic dark matter consists of weakly-interacting massive particles, these particles should be produced in reactions at the next generation of high-energy accelerators. Measurements at these accelerators can then be used to determine…

High Energy Physics - Phenomenology · Physics 2008-11-26 Edward A. Baltz , Marco Battaglia , Michael E. Peskin , Tommer Wizansky

We report a combined experimental and theoretical study of collision-induced dipolar relaxation in a cold spin-polarized gas of atomic nitrogen (N). We use buffer gas cooling to create trapped samples of 14N and 15N atoms with densities…

Atomic Physics · Physics 2011-03-07 T. V. Tscherbul , J. Klos , A. Dalgarno , B. Zygelman , Z. Pavlovic , M. T. Hummon , H-I Lu , E. Tsikata , J. M. Doyle

In the vicinity of the Milky Way Galactic Center, celestial bodies, including neutron stars, reside within a dense dark matter environment. This study explores the accumulation of dark matter by neutron stars through dark matter-nucleon…

High Energy Physics - Phenomenology · Physics 2024-12-02 Thong T. Q. Nguyen

The hot and dense medium created at RHIC, called Quark and Gluon Plasma (QGP) has been a hot topic in the last ten years. Due to the high multiplicities in such heavy-ion collision events, particle correlations using either trigger…

Nuclear Experiment · Physics 2011-10-10 Hua Pei

Dynamical and thermal characterizations of excited nuclear systems produced during the collisions between two heavy ions at intermediate incident energies are presented by means of a review of experimental and theoretical work performed in…

Nuclear Experiment · Physics 2009-11-11 G. Verde , A. Chbihi , R. Ghetti , J. Helgesson

Correlation effects in nuclear matter at finite temperatures are studied for subnuclear densities ($\rho<\rho_0$) and medium excitation energy, where a nonrelativistic potential approach is possible. A quantum statistical approach is given,…

Nuclear Theory · Physics 2009-10-31 G. Roepke , A. Schnell

To reach ultra-low detection thresholds necessary to probe unprecedentedly low Dark Matter masses, target material alternatives and novel detector designs are essential. One such target material is superfluid $^4$He which has the potential…

We suggest the use of moderately superheated liquids in the form of superheated droplet detectors for a new type of neutralino search experiment. The advantage of this method for Dark Matter detection is, that the detector material is…

High Energy Physics - Experiment · Physics 2007-05-23 L. A. Hamel , L. Lessard , V. Zacek , Bhaskar Sur

Dark matter is the name assigned to one of the most important contemporary challenges that fundamental physics research is facing. In recent years, the hypothesis that dark matter might be "light" is gaining interest. Following this idea,…

High Energy Physics - Phenomenology · Physics 2022-01-10 P. Achenbach , L. Doria , M. Battaglieri

There exists considerable interest in dark matter candidates that can reduce cosmological structure at sub-galactic scales through a suppression of the power spectrum of primordial perturbations as well as have a primordial velocity…

Cosmology and Nongalactic Astrophysics · Physics 2009-03-12 Kevork N. Abazajian

Dark Matter (DM) is generally assumed to be massive, cold and collisionless from the structure formation point of view. A more correct statement however is that DM indeed experiences collisional damping, but on a scale which is supposed to…

Astrophysics · Physics 2007-05-23 C. Boehm , H. Mathis , J. Devriendt , J. Silk

Several models of dark matter suggest the existence of dark sectors consisting of SU(3)_C x SU(2)_L x U(1)_Y singlet fields. These sectors of particles do not interact with the ordinary matter directly but could couple to it via gravity. In…

We present an overview of scenarios where the observed Dark Matter (DM) abundance consists of Feebly Interacting Massive Particles (FIMPs), produced non-thermally by the so-called freeze-in mechanism. In contrast to the usual freeze-out…

High Energy Physics - Phenomenology · Physics 2017-11-22 Nicolás Bernal , Matti Heikinheimo , Tommi Tenkanen , Kimmo Tuominen , Ville Vaskonen

We investigate observable cosmological aspects of sterile neutrino dark matter produced via the freeze-in mechanism. The study is performed in a framework that admits many cosmologically interesting variations: high temperature production…

High Energy Physics - Phenomenology · Physics 2017-06-15 Samuel B. Roland , Bibhushan Shakya

Dark photons are predicted by various new physics models, and are being intensively studied in a variety of experiments. In the first part of this paper, we obtain partial wave unitarity constraints on the dark photon parameter space from…

High Energy Physics - Phenomenology · Physics 2024-10-25 Yasaman Hosseini , Mojtaba Mohammadi Najafabadi

Large composite dark matter states source a scalar binding field that, when coupled to Standard Model nucleons, provides a potential under which nuclei recoil and accelerate to energies capable of ionization, radiation, and thermonuclear…

High Energy Physics - Phenomenology · Physics 2022-02-08 Javier F. Acevedo , Joseph Bramante , Alan Goodman

The Spin Physics Detector collaboration proposes to install a universal detector in the second interaction point of the NICA collider under construction (JINR, Dubna) to study the spin structure of the proton and deuteron and other…

High Energy Physics - Experiment · Physics 2024-12-19 The SPD Collaboration , V. Abazov , V. Abramov , L. Afanasyev , R. Akhunzyanov , A. Akindinov , I. Alekseev , A. Aleshko , V. Alexakhin , G. Alexeev , L. Alimov , A. Allakhverdieva , A. Amoroso , V. Andreev , V. Andreev , E. Andronov , Yu. Anikin , S. Anischenko , A. Anisenkov , V. Anosov , E. Antokhin , A. Antonov , S. Antsupov , A. Anufriev , K. Asadova , S. Ashraf , V. Astakhov , A. Aynikeev , M. Azarkin , N. Azorskiy , A. Bagulya , D. Baigarashev , A. Baldin , E. Baldina , N. Barbashina , A. Barnyakov , S. Barsov , A. Bartkevich , V. Baryshevsky , K. Basharina , A. Baskakov , V. Baskov , M. Batista , M. Baturitsky , V. Bautin , T. Bedareva , S. Belokurova , A. Belova , E. Belyaeva , A. Berdnikov , Ya. Berdnikov , A. Berezhnoy , A. Berngardt , Yu. Bespalov , V. Bleko , L. Bliznyuk , D. Bogoslovskii , A. Boiko , A. Boikov , M. Bolsunovskya , E. Boos , V. Borisov , V. Borsch , D. Budkouski , S. Bulanova , O. Bulekov , V. Bunichev , N. Burtebayev , D. Bychanok , A. Casanova , G. Cesar , D. Chemezov , A. Chepurnov , L. Chen , V. Chmill , A. Chukanov , A. Chuzo , A. Danilyuk , A. Datta , D. Dedovich , M. Demichev , G. Deng , I. Denisenko , O. Denisov , T. Derbysheva , D. Derkach , A. Didorenko , M. -O. Dima , A. Doinikov , S. Doronin , V. Dronik , F. Dubinin , V. Dunin , A. Durum , A. Egorov , R. El-Kholy , T. Enik , D. Ermak , D. Erofeev , A. Erokhin , D. Ezhov , O. Fedin , Ju. Fedotova , G. Feofilov , Yu. Filatov , S. Filimonov , V. Frolov , K. Galaktionov , A. Galoyan , A. Garkun , O. Gavrishchuk , S. Gerasimov , S. Gerassimov , M. Gilts , L. Gladilin , G. Golovanov , S. Golovnya , V. Golovtsov , A. Golubev , S. Golubykh , P. Goncharov , A. Gongadze , N. Greben , A. Gregoryev , D. Gribkov , A. Gridin , K. Gritsay , D. Gubachev , J. Guo , Yu. Gurchin , A. Gurinovich , Yu. Gurov , A. Guskov , D. Gutierrez , F. Guzman , A. Hakobyan , D. Han , S. Harkusha , Sh. Hu , S. Igolkin , A. Isupov , A. Ivanov , N. Ivanov , V. Ivantchenko , Sh. Jin , S. Kakurin , N. Kalinichenko , Y. Kambar , A. Kantsyrev , I. Kapitonov , V. Karjavine , A. Karpishkov , A. Katcin , G. Kekelidze , D. Kereibay , S. Khabarov , P. Kharyuzov , H. Khodzhibagiyan , E. Kidanov , E. Kidanova , V. Kim , A. Kiryanov , I. Kishchin , E. Kokoulina , A. Kolbasin , V. Komarov , A. Konak , Yu. Kopylov , M. Korjik , M. Korotkov , D. Korovkin , A. Korzenev , B. Kostenko , A. Kotova , A. Kotzinian , V. Kovalenko , N. Kovyazina , M. Kozhin , A. Kraeva , V. Kramarenko , A. Kremnev , U. Kruchonak , A. Kubankin , O. Kuchinskaia , Yu. Kulchitsky , S. Kuleshov , A. Kulikov , V. Kulikov , V. Kurbatov , Zh. Kurmanaliev , Yu. Kurochkin , S. Kutuzov , E. Kuznetsova , I. Kuyanov , E. Ladygin , V. Ladygin , D. Larionova , V. Lebedev , M. Levchuk , P. Li , X. Li , Y. Li , A. Livanov , R. Lednicki , A. Lobanov , A. Lobko , K. Loshmanova , S. Lukashevich , E. Luschevskaya , A. L'vov I. Lyashko , V. Lysan , V. Lyubovitskij , D. Madigozhin , V. Makarenko , N. Makarov , R. Makhmanazarov , V. Maleev , D. Maletic , A. Malinin , A. Maltsev , N. Maltsev , A. Malkhasyan , M. Malyshev , O. Mamoutova , A. Manakonov , A. Marova , M. Merkin , I. Meshkov , V. Metchinsky , O. Minko , Yu. Mitrankov , M. Mitrankova , A. Mkrtchyan , H. Mkrtchyan , R. Mohamed , S. Morozova , A. Morozikhin , E. Mosolova , V. Mossolov , S. Movchan , Y. Mukhamejanov , A. Mukhamejanova , E. Muzyaev , D. Myktybekov , S. Nagorniy , M. Nassurlla , P. Nechaeva , M. Negodaev , V. Nesterov , M. Nevmerzhitsky , G. Nigmatkulov , D. Nikiforov , V. Nikitin , A. Nikolaev , D. Oleynik , V. Onuchin , I. Orlov , A. Orlova , G. Ososkov , D. Panzieri , B. Parsamyan , P. Pavzderin , V. Pavlov , M. Pedraza , V. Perelygin , D. Peshkov , A. Petrosyan , M. Petrov , V. Petrov , K. Petrukhin , A. Piskun , S. Pivovarov , I. Polishchuk , P. Polozov , V. Polyanskii , A. Ponomarev , V. Popov , V. Popov , S. Popovich , D. Prokhorova , N. Prokofiev , F. Prokoshin , A. Puchkov , I. Pudin , E. Pyata , F. Ratnikov , V. Rasin , V. Red'kov , A. Reshetin , S. Reznikov , N. Rogacheva , S. Romakhov , A. Rouba , V. Rudnev , V. Rusinov , D. Rusov , V. Ryltsov , N. Saduyev , A. Safonov , S. Sakhiyev , K. Salamatin , V. Saleev , A. Samartsev , E. Samigullin , O. Samoylov , E. Saprunov , A. Savenkov , A. Seleznev , A. Semak , D. Senkov , A. Sergeev , L. Seryogin , S. Seryubin , A. Shabanov , A. Shahinyan , A. Shavrin , I. Shein , A. Sheremeteva , V. Shevchenko , K. Shilyaev , S. Shimansky , S. Shinbulatov , F. Shipilov , A. Shipilova , S. Shkarovskiy , D. Shoukovy , K. Shpakov , I. Shreyber , K. Shtejer , R. Shulyakovsky , A. Shunko , S. Sinelshchikova , A. Skachkova , A. Skalnenkov , A. Smirnov , S. Smirnov , A. Snesarev , A. Solin , A. Solin , E. Soldatov , V. Solovtsov , J. Song , D. Sosnov , A. Stavinskiy , D. Stekacheva , E. Streletskaya , M. Strikhanov , O. Suarez , A. Sukhikh , S. Sukhovarov , V. Sulin , R. Sultanov , P. Sun , D. Svirida , E. Syresin , V. Tadevosyan , O. Tarasov , E. Tarkovsky , V. Tchekhovsky , E. Tcherniaev , A. Terekhin , A. Terkulov , V. Tereshchenko , O. Teryaev , P. Teterin , A. Tishevsky , V. Tokmenin , N. Topilin , P. Tsiareshka , A. Tumasyan , G. Tyumenkov , E. Usenko , L. Uvarov , V. Uzhinsky , Yu. Uzikov , F. Valiev , E. Vasilieva , A. Vasyukov , V. Vechernin , A. Verkheev , L. Vertogradov , Yu. Vertogradova , R. Vidal , N. Voitishin , I. Volkov , P. Volkov , A. Vorobyov , H. Voskanyan , H. Wang , Y. Wang , T. Xu , A. Yanovich , I. Yeletskikh , N. Yerezhep , S. Yurchenko , A. Zakharov , N. Zamiatin , J. Zamora-Saá , A. Zarochentsev , A. Zelenov , E. Zemlyanichkina , M. Zhabitsky , J. Zhang , Zh. Zhang , A. Zhemchugov , V. Zherebchevsky , A. Zhevlakov , N. Zhigareva , J. Zhou , X. Zhuang , I. Zhukov , N. Zhuravlev , A. Zinin , S. Zmeev , D. Zolotykh , E. Zubarev , A. Zvyagina

A compelling way to address the inflationary period is via the warm inflation scenario, where the interaction of the inflaton field with other degrees of freedom affects its dynamics in such a way that slow-roll inflation is maintained by…

High Energy Physics - Phenomenology · Physics 2025-04-25 Rayff de Souza , Jamerson G. Rodrigues , Clarissa Siqueira , Felipe B. M. dos Santos , Jailson Alcaniz
‹ Prev 1 4 5 6 7 8 10 Next ›